GAVO DC TAPivo://org.gavo.dc/tapThe GAVO DC teamGAVO Data Centrehttp://vo.ari.uni-heidelberg.de/docs/GavoTiny.png2024-08-08T11:41:27ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837virtual-observatoriescatalogsThe GAVO Data Center's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. In GAVO's data center, we in particular hold several large catalogs like PPMXL, 2MASS PSC, USNO-B2, UCAC4, WISE, SDSS DR16, HSOY, and several Gaia data releases and ancillary resources for you to use in crossmatches, possibly with uploaded tables. Tables exposed through this endpoint include: nucand from the amanda schema, main from the annisred schema, data from the antares schema, data from the antares10 schema, dr10 from the apass schema, frames from the apo schema, main from the applause schema, gfh, id, identified, master, nid, unidentified from the arigfh schema, main from the arihip schema, main from the auger schema, ev_inclined, ev_sd1500, ev_sd750, scaler from the auger3 schema, data, phot_all from the bgds schema, lc_all, lc_b, lc_ha, lc_i, lc_nb, lc_oiii, lc_r, lc_sii, lc_u, lc_v, lc_z, matched, phot_all, phot_b, phot_u, phot_v, phot_z, ssa_time_series from the bgds2 schema, data from the boydende schema, cat from the browndwarfs schema, cubes, fluxposv1200, fluxposv500, fluxv1200, fluxv500, objects, spectra from the califadr3 schema, data, objects, rvs, ts_ssa from the carmenes schema, images, srccat from the cars schema, meta from the carsarcs schema, line_tap from the casa_lines schema, lines from the chianti schema, main from the citigbot schema, main from the cns5 schema, main from the cns5update schema, main from the cs82morphoz schema, geo from the cstl schema, data from the danish schema, narrow_plates, plates, wide_plates from the dasch schema, main from the dfbsplates schema, raw_spectra, spectra, ssa from the dfbsspec schema, main from the dmubin schema, main from the emi schema, data from the feros schema, fk6join, part1, part3 from the fk6 schema, data from the flare_survey schema, data, ordersmeta from the flashheros schema, data from the fornax schema, dr2_ts_ssa, dr2epochflux, dr2light, dr3lite, edr3lite from the gaia schema, hyacob, maglims5, maglims6, maglims7, main, missing_10mas, rejected, resolvedss from the gcns schema, data from the gcpms schema, main from the gdr2ap schema, main from the gdr2dist schema, main, photometry from the gdr2mock schema, spectra, ssameta, withpos from the gdr3spec schema, main from the gedr3auto schema, litewithdist, main from the gedr3dist schema, generated_data, maglim_5, maglim_6, maglim_7, main, parsec_props from the gedr3mock schema, main from the gedr3spur schema, columns, services, tables from the glots schema, main from the gps1 schema, data, meta from the hamburg_eso schema, main from the hdgaia schema, data from the hiicounter schema, main from the hipparcos schema, main from the hppunion schema, main from the hsoy schema, nucand from the icecube schema, data from the inflight schema, obs_radio, obscore from the ivoa schema, events, photpoints, timeseries from the k2c9vst schema, plates from the kapteyn schema, katkat from the katkat schema, data from the lamost5 schema, ssa_lrs, ssa_mrs from the lamost6 schema, disk_basic, h_link, ident, mes_binary, mes_h_link, mes_mass_pl, mes_mass_st, mes_radius_st, mes_sep_ang, mes_teff_st, object, planet_basic, provider, source, star_basic from the life_td schema, geocounts, measurements, stations from the lightmeter schema, rawframes from the liverpool schema, rmtable, spectra, ssameta from the lotsspol schema, main from the lspm schema, plates, wolfpalisa from the lsw schema, main from the magic schema, reduced from the maidanak schema, exts from the mcextinct schema, cubes, slitspectra from the mlqso schema, epn_core, mpcorb from the mpc schema, main, stars from the mwsc schema, main, stars from the mwsce14a schema, data from the obscode schema, bibrefs, maps, masers, monitor from the ohmaser schema, measurements, ssa from the onebigb schema, data, shapes from the openngc schema, main from the pcc schema, data from the plc schema, data from the plc2 schema, data from the plc3 schema, data from the plts schema, data from the polcatsmc schema, cubes, maps from the ppakm31 schema, data from the ppmx schema, main, usnocorr from the ppmxl schema, map10, map6, map7, map8, map9, map_union from the prdust schema, dr2, dr3, dr4, main from the rave schema, data from the robott schema, images, time_series from the rome schema, images, photons from the rosat schema, alt_identifier, authorities, capability, g_num_stat, interface, intf_param, registries, relationship, res_date, res_detail, res_role, res_schema, res_subject, res_table, resource, stc_spatial, stc_spectral, stc_temporal, subject_uat, table_column, tap_table, validation from the rr schema, objects, photpar from the sasmirala schema, main from the sdssdr16 schema, sources from the sdssdr7 schema, main from the smakced schema, main from the species schema, main from the spm4 schema, sources from the supercosmos schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, main from the taptest schema, main from the tenpc schema, main from the tgas schema, data from the theossa schema, data, line_tap from the toss schema, data from the twomass schema, icrscorr, main, ppmxlcross from the ucac3 schema, main from the ucac4 schema, main from the ucac5 schema, main from the ucdc schema, main from the urat1 schema, data, platecorrs, plates, ppmxcross, spurious, twomasscross from the usnob schema, data from the veronqsos schema, stripe82 from the vlastripe82 schema, main from the wdsdss10 schema, archives, main from the wfpdb schema, main from the wise schema, main from the xpparams schema, covs, main from the xpparams2 schema, data from the zcosmos schema.https://dc.g-vo.org/__system__/tap/run/infoIsServiceForGAVO RegTAP ServiceGloTS, the Global TAP SchemaARI Catalog of CatalogsARI Catalog of CatalogsThe first U.S. Naval Observatory Astrometric Robotic Telescope Catalog URAT1 star catalogGAVO Data Center Obscore TableCHIANTI Lines in LineTAPApache Point observations of lensed quasarsApache Point observations of lensed quasarsGaia DR2 source catalogue "light"Gaia DR2 epoch fluxesOpenNGCOpenNGCMiNDSTEP Danish Observatory Lens ImagesMiNDSTEP Danish Observatory Lens ImagesGloTS, the Global TAP SchemaSDSS DR7 PhotoObjAllTOSS -- Tübingen Oscillator Strengths ServiceTOSS -- Tübingen Oscillator Strengths ServiceGaia DR3 source catalogue "light"The Gaia eDR3 Catalogue of Nearby Stars GCNSThe Gaia eDR3 Catalogue of Nearby Stars GCNSGaia DR2 source catalogue "light"Gaia DR2 epoch fluxesQuasars and Active Galactic Nuclei (8th Ed.)A Gaia DR2 mock stellar catalogHipparcos CatalogueLiverpool Quasar Lens MonitoringLiverpool Quasar Lens MonitoringPlates From Münster Flare Star Survey 1986-1991Plates From Münster Flare Star Survey 1986-1991Stellar Proper Motions in the Ogle II Galactic Bulge FieldsDASCH in the VODASCH in the VOThe Sixth Fundamental Catalogue (FK6)The Sixth Fundamental Catalogue (FK6)Gaia DR3 source catalogue "light"CALIFA DR3 tablesCALIFA DR3 tablesGAVO Data Center Obscore TableA classifier for spurious astrometric solutions in Gaia EDR3PPAKM31 – Optical Integral Field Spectroscopy of Star-Forming Regions in M31The 2MASS point source catalogGAVO RegTAP ServiceBoyden Station ADH Plates in GermanyBoyden Station ADH Plates in GermanyMaidanak Observatory Lens ImagesMaidanak Observatory Lens ImagesARIGFH object catalogTGAS catalogueThe LIFE Target Star Database LIFETDThe LIFE Target Star Database LIFETDGaia eDR3 AutocorrelationSplatalogue CASA LineTAPPotsdam Kapteyn Series PlatesPotsdam Kapteyn Series PlatesGaia early DR3 Mock Catalogue (gedr3mock)Pierre Auger Observatory public DR3Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3 (eDR3)Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3 (eDR3)The USNO-B 1.0 CatalogThe USNO-B 1.0 CatalogPlate data for the USNO-B 1.0 Catalogue.ICRS Corrections by USNO-B1 PlateThe USNO-B 1.0 CatalogThe USNO-B 1.0 CatalogICRS Corrections by USNO-B1 PlateDwarfArchives.org – Photometry, spectroscopy, and astrometry of L, T, and Y dwarfsDwarfArchives.org – Photometry, spectroscopy, and astrometry of L, T, and Y dwarfsMinor Planet Center - Asteroid Orbital Data EPN-TAP table for MPC Asteroid Orbital DataMinor Planet Center - Asteroid Orbital Data EPN-TAP table for MPC Asteroid Orbital DataThe Lepine-Shara Catalog of High Proper Motion StarsGAVO Data Center obs_radio TableARIGFH object catalogThe 2MASS point source catalogRAdial Velocity Experiment: RAVE DR5RAdial Velocity Experiment: RAVE DR5Gaia DR3 RP/BP (XP) Monte Carlo sampled spectraGaia DR3 RP/BP (XP) Monte Carlo sampled spectraGAVO Data Center obs_radio TablePlate data for the USNO-B 1.0 Catalogue.Joined Bayestar17 3D Dust MapScans of the Palomar-Leiden Trojan Survey PlatesScans of the Palomar-Leiden Trojan Survey PlatesUCAC3 nocrossDigitized First Byurakan Survey (DFBS) Extracted SpectraDigitized First Byurakan Survey (DFBS) Extracted SpectraA Gaia DR2 mock stellar catalogDASCH in the VODASCH in the VOGaia early DR3 Mock Catalogue (gedr3mock)PPAKM31 – Optical Integral Field Spectroscopy of Star-Forming Regions in M31UCAC3 nocrossThe Lepine-Shara Catalog of High Proper Motion StarsPierre Auger Observatory public DR3Splatalogue CASA LineTAPCHIANTI Lines in LineTAPStellar Proper Motions in the Ogle II Galactic Bulge FieldsGaia eDR3 AutocorrelationA classifier for spurious astrometric solutions in Gaia EDR3Hipparcos CatalogueJoined Bayestar17 3D Dust MapSDSS DR7 PhotoObjAllTGAS catalogueThe first U.S. Naval Observatory Astrometric Robotic Telescope Catalog URAT1 star catalogQuasars and Active Galactic Nuclei (8th Ed.)CALIFA DR3 tablesCALIFA DR3 tablesMars Craters Lagainhttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapObscore-1.1Registry 1.2GloTS 1.0ADQL2.02.1The Astronomical Data Query Language is the standard IVOA dialect of SQL; it contains a very general SELECT statement as well as some extensions for spherical geometry and higher mathematics.

gavo_apply_pm(ra DOUBLE PRECISION, dec DOUBLE PRECISION, pmra DOUBLE PRECISION, pmde DOUBLE PRECISION, epdist DOUBLE PRECISION) -> POINT

Returns a POINT (in the UNDEFINED reference frame) for the position an object at ra/dec with proper motion pmra/pmde has after epdist years. positions must be in degrees, PMs in should be in julian years (i.e., proper motions are expected in degrees/year). pmra is assumed to contain cos(delta). This function goes through the tangential plane. Since it does not have information on distance and radial velocity, it cannot reconstruct the true space motion, and hence its results will degrade over time. This function should not be used in new queries; use ivo_epoch_prop instead.

gavo_getauthority(ivoid TEXT) -> TEXT

returns the authority part of an ivoid (or, more generally a URI). So, ivo://org.gavo.dc/foo/bar#baz becomes org.gavo.dc. The behaviour for anything that's not a full URI is undefined.

gavo_ipix(long REAL, lat REAL) -> BIGINT

gavo_ipix returns the q3c ipix for a long/lat pair (it simply wraps the 13c_ang2ipix function). This is probably only relevant when you play tricks with indices or PPMXL ids.

gavo_match(pattern TEXT, string TEXT) -> INTEGER

gavo_match returns 1 if the POSIX regular expression pattern matches anything in string, 0 otherwise.

gavo_mocintersect(moc1 MOC, moc2 MOC) -> MOC

returns the intersection of two MOCs.

gavo_mocunion(moc1 MOC, moc2 MOC) -> MOC

returns the union of two MOCs.

gavo_specconv(expr DOUBLE PRECISION, dest_unit TEXT) -> DOUBLE PRECISION

returns the spectral value expr converted to dest_unit. expr has to be in either energy, wavelength, or frequency, and dest_unit must be a VOUnit giving another spectral unit (e.g., MHz, keV, nm, or Angstrom). This is intended to let users express spectral constraints in their preferred unit independently of the choice of unit in the database. Examples:: gavo_specconv(obscore.em_min, "keV") > 300 gavo_specconv(obscore.em_max, "MHz") > 30 gavo_specconv(spectral_start, "Angstrom") > 4000 There is a variant of gavo_specconv accepting expr's unit in a third argument.

gavo_specconv(expr NUMERIC, expr_unit TEXT, dest_unit TEXT) -> NUMERIC

returns expr assumed to be in expr_unit expressed in dest_unit. This is a variant of the two-argument gavo_specconv for when the unit of expr is not known to the ADQL translator, either because it because it is a literal or because it does not look like a spectral unit. Examples:: gavo_specconv(656, 'nm', 'J') BETWEEN spectral_start AND spectral_end gavo_specconv(arccos(phi)*incidence, 'Hz', 'eV') Clearly, overriding known units is likely to yield bad results; the translator therefore warns if an existing unit is overridden with a different unit.

gavo_vocmatch(vocname TEXT, term TEXT, matchagainst TEXT) -> INTEGER

returns 1 if matchagainst is term or narrower in the IVOA vocabulary vocname, 0 otherwise. This is intended for semantic querying. For instance, gavo_vocmatch('datalink/core', 'calibration', semantics) would be 1 if semantics is any of calibration, bias, dark, or flat. For RDF-flavoured vocabularies (strict trees), term will expand to the entire branch rooted in term. For SKOS-flavoured vocabularies (where narrower is not transitive), only directly narrower terms will be included. Both the term and the vocabulary name must be string literals (i.e., constants). matchagainst can be any string-valued expression.

ivo_epoch_prop(ra DOUBLE PRECISION, dec DOUBLE PRECISION, parallax DOUBLE PRECISION, pmra DOUBLE PRECISION, pmdec DOUBLE PRECISION, radial_velocity DOUBLE PRECISION, ref_epoch DOUBLE PRECISION, out_epoch DOUBLE PRECISION) -> DOUBLE PRECISION[6]

Returns a 6-vector of (ra, dec, parallax, pmra, pmdec, rv) at out_epoch for these quantities at ref_epoch. Essentially, it will apply the proper motion under the assumption of linear motion. Despite the name of the positional parameters, this is not restricted to equatorial systems, as long as positions and proper motions are expressed in the same reference frames. Units on input and output are degrees for ra and dec, mas for parallax, mas/yr for pmra and pmdec, and km/s for the radial velocity. ref_epoch and out_epoch are given in Julian years. parallax, pmra, pmdec, and radial_velocity may be None and will enter the computations as 0 then, except in the case of parallax, which will be some small value. When abs(parallax) is smaller or equal to that small value, parallax and radial velocity will be NULL on output. In daily use, you probably want to use the ivo_epoch_prop_pos functions.

ivo_epoch_prop_pos(ra DOUBLE PRECISION, dec DOUBLE PRECISION, parallax DOUBLE PRECISION, pmra DOUBLE PRECISION, pmdec DOUBLE PRECISION, radial_velocity DOUBLE PRECISION, ref_epoch DOUBLE PRECISION, out_epoch DOUBLE PRECISION) -> POINT

Returns a POINT giving the position at out_epoch for an object with the six parameters at ref_epoch. Essentially, it will apply the proper motion under the assumption of linear motion. Despite the name of the positional parameters, this is not restricted to equatorial systems, as long as positions and proper motions are expressed in the same reference frames. Units on input are degrees for ra and dec, mas for parallax, mas/yr for pmra and pmdec, and km/s for the radial velocity. ref_epoch and out_epoch are given in Julian years. parallax, pmra, pmdec, and radial_velocity may be None and will enter the computations as 0 then, except in the case of parallax, which will be some small value.

ivo_epoch_prop_pos(ra DOUBLE PRECISION, dec DOUBLE PRECISION, pmra DOUBLE PRECISION, pmdec DOUBLE PRECISION, ref_epoch DOUBLE PRECISION, out_epoch DOUBLE PRECISION) -> POINT

A variant of ivo_epoch_prop_pos that behave as if parallax and radial_velocity were both passed as NULL.

ivo_geom_transform(from_sys TEXT, to_sys TEXT, geo GEOMETRY) -> GEOMETRY

The function transforms ADQL geometries between various reference systems. geo can be a POINT, a CIRCLE, or a POLYGON, and the function will return a geometry of the same type. In the current implementation, from_sys and to_sys must be literal strings (i.e., they cannot be computed through expressions or be taken from database columns). All transforms are just simple rotations, which is only a rough approximation to the actual relationships between reference systems (in particular between FK4 and ICRS-based ones). Note that, in particular, the epoch is not changed (i.e., no proper motions are applied). We currently support the following reference frames: ICRS, FK5 (which is treated as ICRS), FK4 (for B1950. without epoch-dependent corrections), GALACTIC. Reference frame names are case-sensitive.

ivo_hashlist_has(hashlist TEXT, item TEXT) -> INTEGER

The function takes two strings; the first is a list of words not containing the hash sign (#), concatenated by hash signs, the second is a word not containing the hash sign. It returns 1 if, compared case-insensitively, the second argument is in the list of words coded in the first argument. The behaviour in case the the second argument contains a hash sign is unspecified.

ivo_hasword(haystack TEXT, needle TEXT) -> INTEGER

gavo_hasword returns 1 if needle shows up in haystack, 0 otherwise. This is for "google-like"-searches in text-like fields. In word, you can actually employ a fairly complex query language; see https://www.postgresql.org/docs/current/textsearch.html for details.

ivo_healpix_center(hpxOrder INTEGER, hpxIndex BIGINT) -> POINT

returns a POINT corresponding to the center of the healpix with the given index at the given order.

ivo_healpix_index(order INTEGER, ra DOUBLE PRECISION, dec DOUBLE PRECISION) -> BIGINT

Returns the index of the (nest) healpix with order containing the spherical point (ra, dec). An alternative, 2-argument form ivo_healpix_index(order INTEGER, p POINT) -> BIGINT is also available.

ivo_histogram(val REAL, lower REAL, upper REAL, nbins INTEGER) -> INTEGER[]

The aggregate function returns a histogram of val with nbins+2 elements. Assuming 0-based arrays, result[0] contains the number of underflows (i.e., val<lower), result[nbins+1] the number of overflows. Elements 1..nbins are the counts in nbins bins of width (upper-lower)/nbins. Clients will have to convert back to physical units using some external communication, there currently is no (meta-) data as lower and upper in the TAP response.

ivo_interval_has(val NUMERIC, iv INTERVAL) -> INTEGER

The function returns 1 if the interval iv contains val, 0 otherwise. The lower limit is always included in iv, behaviour on the upper limit is column-specific.

ivo_interval_overlaps(l1 NUMERIC, h1 NUMERIC, l2 NUMERIC, h2 NUMERIC) -> INTEGER

The function returns 1 if the interval [l1...h1] overlaps with the interval [l2...h2]. For the purposes of this function, the case l1=h2 or l2=h1 is treated as overlap. The function returns 0 for non-overlapping intervals.

ivo_nocasematch(value TEXT, pattern TEXT) -> INTEGER

ivo_nocasematch returns 1 if pattern matches value, 0 otherwise. pattern is defined as for the SQL LIKE operator, but the match is performed case-insensitively. This function in effect provides a surrogate for the ILIKE SQL operator that is missing from ADQL. On this site, this is actually implemented using python's and SQL's LOWER, so for everything except ASCII, your mileage will vary.

ivo_normal_random(mu REAL, sigma REAL) -> REAL

The function returns a random number drawn from a normal distribution with mean mu and width sigma. Implementation note: Right now, the Gaussian is approximated by summing up and scaling ten calls to random. This, hence, is not very precise or fast. It might work for some use cases, and we will provide a better implementation if this proves inadequate.

ivo_simbadpoint(identifier TEXT) -> POINT

gavo_simbadpoint queries simbad for an identifier and returns the corresponding point. Note that identifier can only be a literal, i.e., as simple string rather than a column name. This is because our database cannot query simbad, and we probably wouldn't want to fire off millions of simbad queries anyway; use simbad's own TAP service for this kind of application.

ivo_string_agg(expression TEXT, delimiter TEXT) -> TEXT

An aggregate function returning all values of expression within a GROUP contcatenated with delimiter

ivo_to_jd(d TIMESTAMP) -> DOUBLE PRECISION

The function converts a postgres timestamp to julian date. This is naive; no corrections for timezones, let alone time scales or the like are done; you can thus not expect this to be good to second-precision unless you are careful in the construction of the timestamp.

ivo_to_mjd(d TIMESTAMP) -> DOUBLE PRECISION

The function converts a postgres timestamp to modified julian date. This is naive; no corrections for timezones, let alone time scales or the like are done; you can thus not expect this to be good to second-precision unless you are careful in the construction of the timestamp.

BOX

POINT

CIRCLE

POLYGON

REGION

CENTROID

COORD1

COORD2

DISTANCE

CONTAINS

INTERSECTS

AREA

COALESCE

LOWER

ILIKE

UPPER

OFFSET

CAST

IN_UNIT

WITH

TABLESAMPLE

Written after a table reference, TABLESAMPLE(10) will make the database only use 10% of the rows; these are `somewhat random' in that the system will use random blocks. This should be good enough when just testing queries (and much better than using TOP n).

MOC

A geometry function creating MOCs. It either takes a string argument with an ASCII MOC ('4/13 17-18 8/3002'), or an order and another geometry.

VECTORMATH

You can compute with vectors here. See https://wiki.ivoa.net/twiki/bin/view/IVOA/ADQLVectorMath for an overview of the functions and operators available.

CASE

The SQL92 CASE expression

UNION

EXCEPT

INTERSECT

text/tab-separated-valuestsvtext/plaintxttext/csvcsv_baretext/csv;header=presentcsvapplication/jsonjsonapplication/geo+jsongeojsonapplication/x-votable+xmlvotableapplication/x-votable+xml;serialization=BINARY2votable/b2votableb2application/x-votable+xml;serialization=TABLEDATAtext/xmlvotable/tdvotabletdapplication/x-votable+xml;serialization=TABLEDATA;version=1.1text/xmlvotabletd1.1application/x-votable+xml;version=1.1text/xmlvotable1.1application/x-votable+xml;serialization=TABLEDATA;version=1.2text/xmlvotabletd1.2application/x-votable+xml;serialization=TABLEDATA;version=1.6vodmlapplication/x-votable+xml;version=1.6vodmlbtext/htmlhtmlapplication/fitsfits17280020200001600000010000000http://dc.g-vo.org/__system__/tap/run/capabilitieshttps://dc.g-vo.org/__system__/tap/run/capabilitieshttp://dc.g-vo.org/__system__/tap/run/availabilityhttps://dc.g-vo.org/__system__/tap/run/availabilityhttp://dc.g-vo.org/__system__/tap/run/tableMetadatahttps://dc.g-vo.org/__system__/tap/run/tableMetadatahttp://dc.g-vo.org/__system__/tap/run/exampleshttps://dc.g-vo.org/__system__/tap/run/examplesivoaDefinition and support code for the ObsCore data model and table.ivoa.obs_radioAn IVOA-defined metadata table for radio measurements, with extra metadata for interferometric measurements ("visibilities") as well as single-dish observations. You will almost always want to join this table to ivoa.obscore (do a natural join).ivo://ivoa.net/std/obsradio#table-1.0obs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexedprimarys_resolution_minAngular resolution, longest baseline and max frequency dependentarcsecpos.angResolution;stat.minChar.SpatialAxis.Resolution.Bounds.Limits.LoLimfloatnullables_resolution_maxAngular resolution, longest baseline and min frequency dependentarcsecpos.angResolution;stat.maxChar.SpatialAxis.Resolution.Bounds.Limits.HiLimfloatnullables_fov_minField of view diameter, min value, max frequency dependentdegphys.angSize;instr.fov;stat.minChar.SpatialAxis.Coverage.Bounds.Extent.LowLimfloatnullables_fov_maxField of view diameter, max value, min frequency dependentdegphys.angSize;instr.fov;stat.maxChar.SpatialAxis.Coverage.Bounds.Extent.HiLimfloatnullables_maximum_angular_scaleMaximum scale in dataset, shortest baseline and frequency dependentarcsecphys.angSize;stat.maxChar.SpatialAxis.Resolution.Scale.Limits.HiLimfloatnullablef_resolutionAbsolute spectral resolution in frequencykHzem.freq;stat.maxChar.SpectralAxis.Coverage.BoundsLimits.HiLimfloatnullablet_exp_minMinimum integration time per samplestime.duration;obs.exposure;stat.minChar.TimeAxis.Sampling.ExtentLoLimfloatnullablet_exp_maxMaximum integration time per samplestime.duration;obs.exposure;stat.maxChar.TimeAxis.Sampling.ExtentHiLimfloatnullablet_exp_meanAverage integration time per samplestime.duration;obs.exposure;stat.meanChar.TimeAxis.Sampling.ExtentHiLimfloatnullableuv_distance_minMinimal distance in uv planemstat.fourier;pos;stat.minChar.UVAxis.Coverage.Bounds.Limits.LoLimfloatnullableuv_distance_maxMaximal distance in uv planemstat.fourier;pos;stat.maxChar.UVAxis.Coverage.Bounds.Limits.LoLimfloatnullableuv_distribution_eccEccentricity of uv distributionstat.fourier;posChar.UVAxis.Coverage.Bounds.Eccentricityfloatnullableuv_distribution_fillFilling factor of uv distributionstat.fourier;pos;arith.ratioChar.UVAxis.Coverage.Bounds.FillingFactorfloatnullableinstrument_ant_numberNumber of antennas in arraymeta.number;instr.paramProvenance.ObsConfig.Instrument.Array.AntNumberfloatnullableinstrument_ant_min_distMinimum distance between antennas in arrayminstr.baseline;stat.minProvenance.ObsConfig.Instrument.Array.MinDistfloatnullableinstrument_ant_max_distMaximum distance between antennas in arrayminstr.baseline;stat.maxProvenance.ObsConfig.Instrument.Array.MaxDistfloatnullableinstrument_ant_diameterDiameter of telecope or antennas in arrayminstr.paramProvenance.ObsConfig.Instrument.Array.Diameterfloatnullableinstrument_feedNumber of feedsinstr.paramProvenance.ObsConfig.Instrument.Feedfloatnullablescan_modeScan mode (on-off, raster map, on-the-fly map,...)instr.paramProvenance.Observation.sky_scan_modefloatnullabletracking_modeTargeted, alt-azimuth, wobble, ...)instr.paramProvenance.Observation.tracking_modefloatnullableivoa.obscoreobs_publisher_didobs_publisher_didivoa.obscoreThe IVOA-defined obscore table, containing generic metadata for datasets within this data centre.ivo://ivoa.net/std/obscore#table-1.1118582767dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecubeimagespectrumtimeseriescharindexednullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel12.02.02.031.00123shortindexedobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collection1BIGB1m-Spiegelteleskop (Hamburg)AG-Teleskop (Bonn)AG-Teleskop (Hamburg)APO Q2237 runBGDSBGDS DR2 time seriesBamberg Southern Sky Patrol (Argentina)Bamberg Southern Sky Patrol (New Zealand)Bamberg Southern Sky Patrol (South Africa)Boyden-deCALIFACARMENES DR1CARMENES DR1 timeseriesCARSDASCHDFBS spectraDFBS-platesDoppel-Reflektor (Hamburg)ESO telescopes (La Silla)FerosFornax cluster center mosaicGLENDAMAGreat Schmidt Camera (Potsdam)Grosser Refraktor (Hamburg)Grosser Schmidt-Spiegel (Hamburg)HDAPHamburg-ESO SurveyHamburger Schmidt-Spiegel (Calar Alto)K2C9 VSTKleiner Schmidt-Spiegel II (Hamburg)LAMOST6 LRSLAMOST6 MRSLippert-Astrograph (Hamburg)LoTSS DR2Maidanak LensesMetcalf Telescope (South Africa)MiNDSTEpMuenster Flare SurveyPLTSPPAKM31Potsdam Kapteyn SeriesRASSROME/REA time seriesRoBoTTRoss B Camera (South Africa)Ross Camera (Potsdam)Schmidtsches Spiegelteleskop (Hamburg)Small Schmidt Camera (Potsdam)TMAPTMAWTartu Old ObservatoryVLBA LH sourcesZeiss Objective (South Africa)Zeiss Triplet (Potsdam)flashherosmlqsomlqso slitppakm31 cubeszcosmoscharindexednullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharindexednullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.size19.09.097.017226641.0longnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classAsteroidBlazarClGCluster of StarsCometDouble or multiple starGalaxyGravLensHIIHII (ionized) regionLensingEvMoonNULLPlanetary NebulaQSORegionStarVariable StarXagnblazarfieldfsgalk2starplanetradio-grvcandistarsurvey fieldunknown (&sg)unknown (--)unknown (3_ccand&sg)unknown (3_cunknown)unknown (agb_cand)unknown (agb_known)unknown (agn_gal)unknown (agn_point)unknown (b)unknown (bllac)unknown (by)unknown (c)unknown (ccandidate)unknown (css_var)unknown (ctts/rot)unknown (d)unknown (dd)unknown (dsctr)unknown (dscut)unknown (dss_gccand)unknown (dss_pncand)unknown (dual_agn)unknown (dwagb_cand)unknown (dwqsocand)unknown (e)unknown (ea)unknown (eb)unknown (eb/ke)unknown (ec)unknown (edgal_cand)unknown (ell/rs)unknown (emb)unknown (emg)unknown (emos)unknown (er)unknown (esd)unknown (ew)unknown (ewqsocand)unknown (exor)unknown (exor:)unknown (f)unknown (firstg)unknown (firsts)unknown (fs_rv)unknown (gcknown&sg)unknown (gcknown)unknown (gdor)unknown (hii)unknown (ins)unknown (insb)unknown (k)unknown (l)unknown (l:)unknown (laqso)unknown (m)unknown (m31_pn)unknown (m31obj)unknown (m31target)unknown (m33_ccand)unknown (m33_pn)unknown (m33known_c)unknown (m35star)unknown (m67star)unknown (misc)unknown (mpcand)unknown (mqsocand)unknown (mwsc_star)unknown (na)unknown (nedqso)unknown (null)unknown (nvss)unknown (othper)unknown (p)unknown (photowd)unknown (pne)unknown (qso)unknown (qso_rev)unknown (qsocand)unknown (radio)unknown (rgcand)unknown (rrab)unknown (rrc)unknown (rrlyare)unknown (rrlycand)unknown (rv)unknown (s)unknown (sdssqso)unknown (sg)unknown (sn ia)unknown (sn)unknown (sqsocand)unknown (sr:)unknown (stars)unknown (supergaint)unknown (tts/rot+uv)unknown (ungcluster)unknown (uv)unknown (uv:)unknown (uvn)unknown (uxor)unknown (var)unknown (var:)unknown (var_per)unknown (vari)unknown (varwise)unknown (w)unknown (wds)unknown (wise_var)unknown (wise_vari)unknown (wn)unknown (wqsocand)unknown (wsqsocand)unknown (wtts/rot)unknown (x)unknown (xd)unknown (xmm)unknown (yso)charnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1020.1413209.025341.7143600.982073doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9161-63.4054-18.958256.480589.9880.982073doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameter1.7119e-050.0001111110.0005555560.001650.39290.982067floatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharindexednullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.value5.14641e-060.00027781.0762515450.00354295floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime-6146.555450.156458.35814959214.20.620126doubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime-6146.5562865762658738.163023.50.620108doubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent0107206960934800.00296283floatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.value1001001001003e+080.481214floatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit1.23881e-173.184e-074.8e-078.6e-071.837720.996148floatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit1.23881e-153.6e-076.99e-071.12e-062.492820.996148floatindexednullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refval-15502563.5264.644636.44738030.345989floatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.name2m Liverpool robotic telescope (Canary Islands, Spain)AO PotsdamApache Point ObservatoryBonn; GermanyBoyden Observatory; Bloemfontein; South AfricaBoyden Station, SAByurakan Astrophysical Observatory BAOCAS, NAOCFHTCalar AltoCalar Alto 3.5m telescopeCalar Alto Observatory; SpainESOESO La SillaFermiHamburg-Bergedorf; GermanyHamburger Sternwarte; ESO La SillaHarvard-Smithsonian Center for AstrophysicsIAATLOFARLa Silla ESO 1.5m telescopeLa Silla; ChileLandessternwarte Heidelberg-Königstuhl, Max-Planck-Institut für Astronomie HeidelbergLas Cumbres Observatory Telescope NetworkMaidanak ObservatoryMount John Observatory; Lake Tekapo; New ZealandObservatorio de Fisica Cosmica; San Miguel; ArgentinaPalomar ObservatoryPotsdam-TelegrafenbergROSATRoBoTTTartu; Estonia (MPC code 075)Universitätssternwarte Bochum near Cerro ArmazonesVLTVery Large TelescopeVery Long Baseline Array, operated by The National Radio Astronomy Observatorycharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.name1 in Cook Lens #832 Series renamed from ac-a10-inch Metcalf Triplet11-inch Draper Refractor12-inch Metcalf Doublet122-cm Schmidt13-inch Boyden Refractor16-inch Metcalf Doublet (Refigured after 3500)1m ESO Schmidt1m-Spiegelteleskop200 inch Hale Telescope24-33 in Jewett Schmidt24-inch Bruce Doublet24-inch Clark Reflector2m Liverpool robotic telescope3.5m APO32-36 inch BakerSchmidt 10 1/2 inch round Armagh-Dunsink-Harvard4-inch Cooke (1-327)4-inch Cooke Lens4-inch Voightlander Lens40cm GPO7.5-inch Cooke/Clark Refractor at Maria Mitchell Observatory8-inch Bache Doublet8-inch Brashear Lens8-inch Draper Doublet8-inch Ross LundinADH SchmidtAG-AstrographAZT 22Asiago Observatory 92/67 cm SchmidtAstrograph (four 10-cm Tessar f/6 cameras)Astrograph (six 10-cm Tessar f/6 cameras)Astrograph (ten 10-cm Tessar f/6 cameras)Byurakan 1m SchmidtCARMENESCFHT 3.6mCalar Alto (493), 1.23m in Cassegrain focus w/correctorCalar Alto (493), 2.2m in Cassegrain focus w/correctorCalar Alto (493), 3.5m in primary focus w/2-lens correctorCalar Alto (493), 3.5m in primary focus w/3-lens correctorCalar Alto (493), SchmidtDK-1.54Doppel-ReflektorESO 1-metre Schmidt telescopeESO La Silla, 2.2m MPG telescopeESO/MPG 2.2mFEROSFORSFermi LATFlash/HerosGrand Prisme Objectif telescopeGreat Refractor - POT080Great Refractor - POT080Great Schmidt CameraGrosser RefraktorGrosser Schmidt-SpiegelHamburger Schmidt-SpiegelHeidelberg Koenigstuhl (24), 72cm Walz ReflektorHeidelberg Koenigstuhl (24), Bruce AstrographHeidelberg Koenigstuhl (24), Wolf's DoppelastrographI TessarKleiner Schmidt-Spiegel IILAMOSTLippert-AstrographLowel 40 inch reflectorMax Wolf's residence in Heidelberg, Maerzgasse, Wolf's DoppelastrographMetcalf 10" (250/1240/167)Original Schmidt-SpiegelPPMAS/PPAK at 3.5m Calar AltoPOT015 Zeiss Triplet 15PetzvalPositivesPotsdam Multi-aperture Spectrophotometer (PMAS) with the PPaK fiber-bundlePotsdam Multi-aperture Spectrophotometer (PMAS) with the PPaK fiber-bundleROSAT HRIROSAT PSPCBROSAT PSPCCRobotic Bochum Twin Telescope (RoBoTT)Ross CameraRoss-B 3"Sinistro camerasSmall Schmidt CameraTMAWTPDPVIMOSVLBAVSTYSO Double AstrographZeissZeiss + Apo-Tessar Zeiss ObjectiveZeiss TripletZeiss Triplet 15 cm Potsdam-TelegrafenbergZeiss-Triplet POT015 - 15charnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins111.01.01.0382430.9981014intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins211.01.01.0382430.9981014intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBins11.013.0181.03070.61775124intnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBins11.01.03900.06861960.8303535intnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBins11.01.01.010.0003706701intnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriod5.14641e-060.2654461.7925415450.00354892floatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablepreviewURL of a preview (low-resolution, quick-to-retrieve representation) of the data.meta.ref.url;meta.previewcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullabletap_schema GAVO Data Center's Table Access Protocol (TAP) service with table metadata.tap_schema.columnsColumns in tables available for ADQL querying.table_nameFully qualified table namecharindexedprimarycolumn_nameColumn namecharindexedprimarydescriptionBrief description of columnunicodeCharnullableunitUnit in VO standard formatcharnullableucdUCD of column if anycharnullableutypeUtype of column if anycharnullabledatatypeADQL datatypecharnullablearraysizeArraysize in VOTable notationcharnullablextypeVOTable extended type information (for special interpretation of data content, e.g., timestamps or points)charnullable"size"Legacy length (ignore if you can).intnullableprincipalIs column principal?intindexedIs there an index on this column?intstdIs this a standard column?intsourcerdId of the originating rd (local information)charnullablecolumn_index1-based index of the column in database order.shortnullabletap_schema.tablestable_nametable_nametap_schema.tablesTables available for ADQL querying.schema_nameFully qualified schema namecharnullabletable_nameFully qualified table namecharindexedprimarytable_typeOne of: table, viewcharnullabledescriptionBrief description of the tableunicodeCharnullableutypeutype if the table corresponds to a data modelcharnullabletable_indexSuggested position this table should take in a sorted list of tables from this data centerintnullablesourcerdId of the originating rd (local information)charnullablenrowsThe approximate size of the table in rowslongnullabletap_schema.schemasschema_nameschema_nametap_schema.groupsColumns that are part of groups within tables available for ADQL querying.table_nameFully qualified table namecharnullablecolumn_nameName of a column belonging to the groupcharnullablecolumn_utypeutype the column within the groupcharnullablegroup_nameName of the groupcharnullablegroup_utypeutype of the groupcharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.tablestable_nametable_nametap_schema.key_columnsColumns participating in foreign key relationships between tables available for ADQL querying.key_idKey identifier from TAP_SCHEMA.keyscharnullablefrom_columnKey column name in the from tablecharnullabletarget_columnKey column in the target tablecharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.keyskey_idkey_idtap_schema.keysForeign key relationships between tables available for ADQL querying.key_idUnique key identifiercharindexedprimaryfrom_tableFully qualified table namecharnullabletarget_tableFully qualified table namecharnullabledescriptionDescription of this keyunicodeCharnullableutypeUtype of this keycharnullablesourcerdId of the originating rd (local information)charnullabletap_schema.tablesfrom_tabletable_nametap_schema.tablestarget_tabletable_nametap_schema.schemasSchemas containing tables available for ADQL querying.schema_nameFully qualified schema namecharindexedprimarydescriptionBrief description of the schemaunicodeCharnullableutypeutype if schema corresponds to a data modelcharnullableschema_indexSuggested position this schema should take in a sorted list of schemas from this data center.intnullableauger3 The Pierre Auger Open Data is the public release of 10% of the Pierre Auger Observatory cosmic-ray data published in recent scientific papers and at International conferences. The Pierre Auger Observatory, located on a vast, high-altitude plain in the Province of Mendoza in Argentina, is the world's largest cosmic ray observatory and measures the extensive air-showers produced by cosmic rays above ~1e17 eV. Here, we include data from the two surface detector (SD) setups, SD750 and SD1500, as well as the flourescence detectors (FD). For both of these, we also host the full json event descriptors. In addition there is a table of highly inclined events and the scaler readouts. See also the portal page https://opendata.auger.org.auger3.ev_inclinedHighly inclined (60 to 80°) Auger public events detected by the surface detectors in all configurations.2355idEvent identification number in the format YYDDDSSSSSXX, where XX is the order of the event at the current second. Time is expressed here in UTC+12h., i.e., the day starting at noonmeta.id;meta.maincharnullablesdidEvent number from data acquisitionmeta.id7449801918233.999999999820897250.048238896.4497393301.0intsd_gpsnanotimeThe GPS time of the event within its GPS secondnstime.epoch3120003.37206e+075.00409e+089.71666e+089.99795e+081doublenullablesd_thetaZenith angle of the eventdegpos.az.zd6060.467.778.980.11floatnullableerr_sd_thetaUncertainty in zenith angle of the eventdegstat.error;pos.az.zd0.10.10.20.30.51floatnullablesd_phiAzimuth angle of the eventdegpos.az.azi-180-170.438-4.4169.7179.81floatnullableerr_sd_phiUncertainty in azimuth angle of the eventdegstat.error;pos.az.azi0.10.10.20.40.61floatnullablesd_lGalactic longitude of the eventdegpos.galactic.lon0.212.462224347359.91doublenullablesd_bGalactic latitude of the eventdegpos.galactic.lat-87.8-69.7-1073.73888.91doublenullablesd_raRA of the eventdegpos.eq.ra09.762176.6349.838359.91doubleindexednullablesd_decDeclination of the eventdegpos.eq.dec-83.9-76.1-13.836.644.21doubleindexednullablesd_xx-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.x-34567.9-29902.2-3125.624579.930430.41floatnullableerr_sd_xUncertainty in x-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.x0.89.06251.5141.852249.81floatnullablesd_yy-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.y-27405.1-23855.95186.930032.5348361floatnullableerr_sd_yUncertainty in y-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.y18.82450.8142.4229.91floatnullablesd_zz-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.z-167.5-123.338-27.473.3105.11floatnullableerr_sd_zUncertainty in z-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.z0floatnullablesd_eastingEastward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lon4426944473494741375017885076381doublenullablesd_northingNorthward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lat6.07178e+066.07534e+066.10436e+066.12924e+066.13405e+061doublenullablesd_altitudeAltitude of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.alt1232.51276.661372.61473.31505.11floatnullablegpstimeAquisition time on the GPS timescalestime.epoch7.66802e+088.20765e+081.04218e+091.21135e+091.2198e+091doubleindexednullablesd_exposureIntegrated exposure of the reconstructed event. For the SD1500 array the energy-threshold for full-efficiency is 2.5e18 eV (4e18 eV) for vertical (inclined) events. For the SD750 array the energy-threshold for full-efficiency is 1e17 eV.stime.duration;obs.exposure4.5166.255935.021726.391769.121floatnullablesd_geochi2χ² value of the geometric fitstat.fit.chi20.031.02245.1850.86642515.611floatnullablesd_nbstatNumber of triggered stations used in reconstructionmeta.number57.013.028.0531.0shortnullablesd_geondfNumber of degrees of freedom in the geometric fitstat.fit.dof241025501floatnullablesd_n19Energy estimator, N19, of a shower with a zenith angle > 60 deginstr.param0.70.81.14.512.21floatnullableerr_sd_n19Uncertainty in energy estimator, N19, of a shower with a zenith angle > 60 degstat.error;instr.param0.10.10.10.30.51floatnullablesd_n68N19 that a shower would have produced had it arrived at 68 deginstr.param0.80.81.14.512.41floatnullableerr_sd_n68Uncertainty in n19 that a shower would have produced had it arrived at 68 degstat.error;instr.param0.10.10.10.30.51floatnullableauger3.ev_sd1500Auger public events detected by the surface detectors in the SD1500 configuration.24319idEvent identification number in the format YYDDDSSSSSXX, where XX is the order of the event at the current second. Time is expressed here in UTC+12h., i.e., the day starting at noonmeta.id;meta.maincharnullablesdidEvent number from data acquisitionmeta.id6222401845721.020056550.047572661.79999999497369801.0intsd_gpsnanotimeThe GPS time of the event within its GPS secondnstime.epoch170003.10475e+074.96948e+089.695e+089.9984e+080.935524doublenullablesd_thetaZenith angle of the eventdegpos.az.zd0.358.92537.9558.515600.935524floatnullableerr_sd_thetaUncertainty in zenith angle of the eventdegstat.error;pos.az.zd0.090.210.441.16.210.935524floatnullablesd_phiAzimuth angle of the eventdegpos.az.azi010.925179.91348.1359.960.935524floatnullableerr_sd_phiUncertainty in azimuth angle of the eventdegstat.error;pos.az.azi0.080.250.784.775191.140.935524floatnullablesd_lGalactic longitude of the eventdegpos.galactic.lon07.21260.62352.99359.990.935524doublenullablesd_bGalactic latitude of the eventdegpos.galactic.lat-89.81-74.855-16.0555.8287.210.935524doublenullablesd_rapos.eq.ra;meta.main0.0110.91179.17349.755359.990.935524floatindexednullablesd_decpos.eq.dec;meta.main-89.41-77.32-29.3815.1424.790.935524floatindexednullablesd_xx-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.x-36201.9-29439.6-2433.8624994.930296.20.935524floatnullableerr_sd_xUncertainty in x-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.x4.1514.19543.68107.84363.280.935524floatnullablesd_yy-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.y-28075.1-23434.85357.9530354.435038.70.935524floatnullableerr_sd_yUncertainty in y-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.y3.6315.2942.31107.865745.440.935524floatnullablesd_zz-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.z-169.87-123.82-30.1475.07112.880.935524floatnullableerr_sd_zUncertainty in z-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.z0floatnullablesd_eastingEastward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lon4410704478264748105022035075030.935524doublenullablesd_northingNorthward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lat6.07111e+066.07576e+066.10454e+066.12957e+066.13426e+060.935524doublenullablesd_altitudeAltitude of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.alt1345.751354.481394.141548.141605.490.935524floatnullablegpstimeAquisition time on the GPS timescalestime.epoch7.57207e+088.18138e+081.03112e+091.20771e+091.21979e+091doubleindexednullablesd_exposureIntegrated exposure of the reconstructed event. For the SD1500 array the energy-threshold for full-efficiency is 2.5e18 eV (4e18 eV) for vertical (inclined) events. For the SD750 array the energy-threshold for full-efficiency is 1e17 eV.stime.duration;obs.exposure0.2157202.5323088.085854.546040.840.887824floatnullablesd_geochi2χ² value of the geometric fitstat.fit.chi2001.3433.131123.880.935524floatnullablesd_nbstatNumber of triggered stations used in reconstructionmeta.number33.05.011.0280.9355237shortnullablesd_s1000Expected signal at 1000 m from the core, S(1000), used as estimator of the energy of detected with the 1500 m array'VEM'stat.fit;instr.experiment2.136.89516.0568.21689.790.935524floatnullableerr_sd_s1000Uncertainty in expected signal at 1000 m from the core, S(1000), used as estimator of the energy of detected with the 1500 m array'VEM'stat.error;stat.fit;instr.experiment0.540.91.543.7118.490.935524floatnullablesd_gcorrGeomagnetic correction to S(1000)%instr.offset;arith.ratio0.9720.9780.9950.99910.935524floatnullablesd_wcorrWeather correction to S(1000)%instr.offset;arith.ratio0.9310.9570.9991.0541.1320.935524floatnullablesd_geondfNumber of degrees of freedom in the geometric fitstat.fit.dof0017240.935524floatnullablefulldataURL of the complete, JSON-formatted record or this event. See https://opendata.auger.org/data.php for an explanation of what you find there.meta.ref.url;meta.datasetcharnullablefd_total_energyTotal energy of the primary particle initiating the eventEeVem.energy0.6310.656671.329511.116860.6390.131173floatnullableerr_fd_total_energyUncertainty in total energy of the primary particle initiating the eventEeVstat.error;em.energy0.0430.0490.0970.874315.1980.131173floatnullablefd_cal_energyCalorimetric energy of the primary particle initiating the eventEeVem.energy0.5260.5481.139.6548953.1940.131173floatnullableerr_fd_cal_energyUncertainty in calorimetric energy of the primary particle initiating the eventEeVstat.error;em.energy0.0340.0390.0810.758314.5770.131173floatnullablefd_x_maxPosition of the maximum of the energy deposition in the atmosphereg/cm**2pos.earth.altitude511.23639.171728.835858.6391064.950.131173floatnullableerr_fd_x_maxUncertainty in position of the maximum of the energy deposition in the atmosphereg/cm**2stat.error;pos.earth.altitude4.398.196715.61533.576656.290.131173floatnullablefd_height_x_maxHeight of x_max above the sea levelmpos.earth.altitude1946.763074.065062.718232.96113520.131173floatnullablefd_dist_x_maxDistance of x_max to FD eyempos.spherical.r5326.87798.7312826.224813.8400280.131173floatnullablefd_de_dx_maxMaximum energy depositPeV/(g/cm**2)phys.energy.density;stat.max0.860.971.9716.202784.420.131173floatnullableerr_fd_de_dx_maxUncertainty in maximum energy depositPeV/(g/cm**2)stat.error;phys.energy.density;stat.max0.020.030.060.372.080.131173floatnullablesd_energyEnergyEeVphys.energy0.4331.46253.39115.2035144.1150.935524floatnullableerr_sd_energyUncertainty in energyEeVstat.error;phys.energy0.110.2120.3590.853.9830.935524floatnullablefd_cherenkov_fractionFraction of detected light from Cherenkov emissionphys.energy;arith.ratio0.020.050.10.20.370.131173floatnullablefd_min_view_angleLight emission angle from the shower towards the FD eyedegpos.emergenceAng16.1721.600141.6397.2565121.590.131173floatnullablefd_usp_lUniversal shower profile shape parameter Lg/cm**2stat.fit192.11215.667227.685242.92260.50.131173floatnullableerr_fd_usp_lUncertainty in universal shower profile shape parameter Lg/cm**2stat.error;stat.fit2.716.21679.1511.223313.810.131173floatnullablefd_usp_rUniversal shower profile shape parameter Rstat.fit0.150.220.260.290.390.131173floatnullableerr_fd_usp_rUncertainty in universal shower profile shape parameter Rstat.error;stat.fit0.020.040.050.060.060.131173floatnullablefd_hottest_station_idid of the SD station with the highest recorded signalmeta.id;instr.obsty71195.0751.01715.3318500.13117316shortnullablefd_dist_sdp_stationDistance of the hottest station to the plane that includes the shower axis and the eye position (SDP)mpos.spherical.r0.0115.84279.84755.9261479.350.131173floatnullablefd_dist_axis_stationDistance of hottest station to the reconstructed shower axis in the shower planempos.cylindrical.r8.77116.421501.705919.7551479.670.131173floatnullablesd_betaβ slope parameter of the fitted LDFstat.fit.param-2.55-2.4-2.15-1.63-1.470.935524floatnullablesd_gammaγ slope parameter of the fitted LDFstat.fit.param-0.06-0.020.020.110.220.935524floatnullablesd_chi2χ² value of the LDF fitstat.fit.chi200.142.3916.535519.730.935524floatnullablesd_ndfNumber of degrees of freedom in the LDF fitstat.fit.dof0028250.935524floatnullablesd_s38Signal produced at 1000 m by a shower with a zenith angle of 38 deg in the 1500 m array'VEM'instr.param2.277.40516.7471.735635.40.935524floatnullableeye_usedThree smallints, 1 if the Eye was used for the spectrum analysis, the energy calibration analysis, and the X_max analysis, respectivelymeta.codeshortnullablefd_gpsnanotimeThe GPS time of the event within its GPS secondnstime.epoch3102043.37894e+075.04658e+089.67246e+089.98851e+080.131173doublenullablefd_thetaZenith angle of the eventdegpos.az.zd11.9720.943539.22560.01375.360.131173floatnullableerr_fd_thetaUncertainty in zenith angle of the eventdegstat.error;pos.az.zd0.080.210.481.021.730.131173floatnullablefd_phiAzimuth angle of the eventdegpos.az.azi0.3110.2636171.945349.496359.960.131173floatnullableerr_fd_phiUncertainty in azimuth angle of the eventdegstat.error;pos.az.azi0.190.440.81.764.20.131173floatnullablefd_lGalactic longitude of the eventdegpos.galactic.lon0.026.3301260.415352.68359.850.131173doublenullablefd_bGalactic latitude of the eventdegpos.galactic.lat-89.01-74-17.1457.912985.110.131173doublenullablefd_raRA of the eventdegpos.eq.ra0.068.8767198.605348.443359.980.131173doublenullablefd_decDeclination of the eventdegpos.eq.dec-89.19-75.8832-25.60512.046634.810.131173doublenullablefd_xx-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.x-36912.6-31334.5-5409.3923835.930142.10.131173floatnullableerr_fd_xUncertainty in x-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.x11.5522.393451.3179.48989.140.131173floatnullablefd_yy-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.y-29825.9-247655309.6732319.137267.20.131173floatnullableerr_fd_yUncertainty in y-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.y10.6821.8550.085174.2261229.530.131173floatnullablefd_zz-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.z-172.28-102.79-40.6880.2474104.140.131173floatnullableerr_fd_zUncertainty in z-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.z0floatnullablefd_eastingEastward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lon4403644459314717825010565073280.131173doublenullablefd_northingNorthward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lat6.06937e+066.07443e+066.1045e+066.13152e+066.1365e+060.131173doublenullablefd_altitudeAltitude of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.alt1346.151358.051394.741561.091597.170.131173floatnullablesd_r_curvatureRadius of curvature of the showermphys.size.radius06022.439922.1720295.6980440.935524floatnullableerr_sd_r_curvatureUncertainty in radius of curvature of the showermstat.error;phys.size.radius00954.95265.461135600.935524floatnullablemulti_eye1 if this is a multi-eye eventmeta.code00.00.00.011.0shortauger3.ev_sd750Auger public events detected by the surface detectors in the SD750 configuration.54481idEvent identification number in the format YYDDDSSSSSXX, where XX is the order of the event at the current second. Time is expressed here in UTC+12h., i.e., the day starting at noonmeta.id;meta.maincharnullablesdidEvent number from data acquisitionmeta.id1700090025771034.037534540.049044498.0497446101.0intsd_gpsnanotimeThe GPS time of the event within its GPS secondnstime.epoch-1348543.01673e+074.99196e+089.6942e+089.99856e+081doublenullablesd_thetaZenith angle of the eventdegpos.az.zd0.376.5927.4639.3401floatnullableerr_sd_thetaUncertainty in zenith angle of the eventdegstat.error;pos.az.zd0floatnullablesd_phiAzimuth angle of the eventdegpos.az.azi010.654181.19348.732359.991floatnullableerr_sd_phiUncertainty in azimuth angle of the eventdegstat.error;pos.az.azi0floatnullablesd_lGalactic longitude of the eventdegpos.galactic.lon-179.97-154.08-52.2691.658179.941doublenullablesd_bGalactic latitude of the eventdegpos.galactic.lat-89.75-76.336-15.8246.97666.841doublenullablesd_raRA of the eventdegpos.eq.ra0.0111.13179.42349.166359.991doubleindexednullablesd_decDeclination of the eventdegpos.eq.dec-75.12-67.3-32.26-0.644.871doubleindexednullablesd_xx-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.x-30173.1-29393.1-26072.4-23783.4-23210.31floatnullableerr_sd_xUncertainty in x-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.x07.1929.385.0883941.551floatnullablesd_yy-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.y12393.312732.114763.116877.6172651floatnullableerr_sd_yUncertainty in y-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.y07.4429.3785.3823613.41floatnullablesd_zz-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.z78.9781.7892.74104.5107.461floatnullableerr_sd_zUncertainty in z-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.z0floatnullablesd_eastingEastward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lon4470644478444511624534504540221doublenullablesd_northingNorthward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lat6.11152e+066.11186e+066.11389e+066.116e+066.11639e+061doublenullablesd_altitudeAltitude of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.alt1478.971481.781492.741504.51507.461floatnullablegpstimeAquisition time on the GPS timescalestime.epoch1.07261e+091.0775e+091.14422e+091.21595e+091.21984e+091doubleindexednullablesd_exposureIntegrated exposure of the reconstructed event. For the SD1500 array the energy-threshold for full-efficiency is 2.5e18 eV (4e18 eV) for vertical (inclined) events. For the SD750 array the energy-threshold for full-efficiency is 1e17 eV.stime.duration;obs.exposure0.00350.3338255.2154510.163410.48140.999908floatnullablesd_geochi2χ² value of the geometric fitstat.fit.chi2001.2949.1363492.241floatnullablesd_nbstatNumber of triggered stations used in reconstructionmeta.number33.06.011.0491.0shortnullablesd_s450Expected signal at 450 m from the core, S(450), used as estimator of the energy of shower detected with the 750 m array'VEM'stat.fit;instr.experiment6.087.4512.2140.7964598.611floatnullableerr_sd_s450Uncertainty in expected signal at 450 m from the core, S(450), used as estimator of the energy of shower detected with the 750 m array'VEM'stat.error;stat.fit;instr.experiment01.151.683.442515721floatnullablesd_s35Signal produced at 450 m by a shower with a zenith angle of 35 deg in the 750 m array'VEM'instr.param5.347.6310.2734.95663751.090.999963floatnullablefulldataURL of the complete, JSON-formatted record or this event. See https://opendata.auger.org/data.php for an explanation of what you find there.meta.ref.url;meta.datasetcharnullablefd_total_energyTotal energy of the primary particle initiating the eventEeVem.energy0.0720.109760.30.808882.2570.00361594floatnullableerr_fd_total_energyUncertainty in total energy of the primary particle initiating the eventEeVstat.error;em.energy0.0050.0090.0220.0590.1420.00361594floatnullablefd_cal_energyCalorimetric energy of the primary particle initiating the eventEeVem.energy0.0560.086880.2450.67841.940.00361594floatnullableerr_fd_cal_energyUncertainty in calorimetric energy of the primary particle initiating the eventEeVstat.error;em.energy0.0040.0070.0170.048120.1190.00361594floatnullablefd_x_maxPosition of the maximum of the energy deposition in the atmosphereg/cm**2pos.earth.altitude509.73570.483676.88846962.730.00361594floatnullableerr_fd_x_maxUncertainty in position of the maximum of the energy deposition in the atmosphereg/cm**2stat.error;pos.earth.altitude6.548.799215.9735.397639.830.00361594floatnullablefd_height_x_maxHeight of x_max above the sea levelmpos.earth.altitude1974.982480.734442.265851.237398.330.00361594floatnullablefd_dist_x_maxDistance of x_max to FD eyempos.spherical.r2970.583588.325663.8810052.111398.40.00361594floatnullablefd_de_dx_maxMaximum energy depositPeV/(g/cm**2)phys.energy.density;stat.max0.10.160.441.25363.130.00361594floatnullableerr_fd_de_dx_maxUncertainty in maximum energy depositPeV/(g/cm**2)stat.error;phys.energy.density;stat.max00.010.010.030.060.00361594floatnullablesd_energyEnergyEeVphys.energy0.0710.1010.1370.46650.5431floatnullableerr_sd_energyUncertainty in energyEeVstat.error;phys.energy0floatnullablefd_cherenkov_fractionFraction of detected light from Cherenkov emissionphys.energy;arith.ratio0.040.050.080.150.170.00361594floatnullablefd_min_view_angleLight emission angle from the shower towards the FD eyedegpos.emergenceAng16.7820.435238.2562.926483.180.00361594floatnullablefd_usp_lUniversal shower profile shape parameter Lg/cm**2stat.fit192.67211.255221.97231.524246.310.00361594floatnullableerr_fd_usp_lUncertainty in universal shower profile shape parameter Lg/cm**2stat.error;stat.fit5.736.91489.4611.473212.810.00361594floatnullablefd_usp_rUniversal shower profile shape parameter Rstat.fit0.220.240.260.270.310.00361594floatnullableerr_fd_usp_rUncertainty in universal shower profile shape parameter Rstat.error;stat.fit0.030.040.050.060.060.00361594floatnullablefd_hottest_station_idid of the SD station with the highest recorded signalmeta.id;instr.obsty1223.881767.01839.1218440.0036159395shortnullablefd_dist_sdp_stationDistance of the hottest station to the plane that includes the shower axis and the eye position (SDP)mpos.spherical.r0.848.6232160.12370.1355350.00361594floatnullablefd_dist_axis_stationDistance of hottest station to the reconstructed shower axis in the shower planempos.cylindrical.r37.3150.5796277.7423.69611.670.00361594floatnullablesd_betaβ slope parameter of the fitted LDFstat.fit.param-3.35-3.17-2.99-2.78-2.321floatnullablesd_gammaγ slope parameter of the fitted LDFstat.fit.param-0.39-0.34-0.31-0.28-0.191floatnullablesd_chi2χ² value of the LDF fitstat.fit.chi20.822.887.6532.216183.021floatnullablesd_ndfNumber of degrees of freedom in the LDF fitstat.fit.dof00414911floatnullablesd_s38Signal produced at 1000 m by a shower with a zenith angle of 38 deg in the 1500 m array'VEM'instr.param19.4220.719341.07561.430762.733.671e-05floatnullableeye_usedThree smallints, 1 if the Eye was used for the spectrum analysis, the energy calibration analysis, and the X_max analysis, respectivelymeta.codeshortnullablefd_gpsnanotimeThe GPS time of the event within its GPS secondnstime.epoch7.87511e+065.35249e+074.86304e+089.63612e+089.9687e+080.00361594doublenullablefd_thetaZenith angle of the eventdegpos.az.zd2.57.27826.8639.178440.850.00361594floatnullableerr_fd_thetaUncertainty in zenith angle of the eventdegstat.error;pos.az.zd0.140.20.410.99121.430.00361594floatnullablefd_phiAzimuth angle of the eventdegpos.az.azi2.7421.9684173.74344.453358.910.00361594floatnullableerr_fd_phiUncertainty in azimuth angle of the eventdegstat.error;pos.az.azi0.330.45761.125.367218.720.00361594floatnullablefd_lGalactic longitude of the eventdegpos.galactic.lon0.613.0408265.94352.656359.60.00361594doublenullablefd_bGalactic latitude of the eventdegpos.galactic.lat-87.25-80.638-21.8545.39261.870.00361594doublenullablefd_raRA of the eventdegpos.eq.ra1.027.4912236.07350.86359.250.00361594doublenullablefd_decDeclination of the eventdegpos.eq.dec-72.58-67.6248-31.56-1.32923.650.00361594doublenullablefd_xx-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.x-29763.8-29418-26805.1-24214.1-23516.70.00361594floatnullableerr_fd_xUncertainty in x-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.x7.9212.852825.9362.167290.330.00361594floatnullablefd_yy-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.y12430.612809.114607.416746.717169.90.00361594floatnullableerr_fd_yUncertainty in y-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.y4.176.996418.753.263276.610.00361594floatnullablefd_zz-coordinate of the shower core projected at ground level (site coordinates system)mpos.cartesian.z80.7784.051297.43106.7106.70.00361594floatnullableerr_fd_zUncertainty in z-coordinate of the shower core projected at ground level (site coordinates system)mstat.error;pos.cartesian.z0floatnullablefd_eastingEastward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lon4474744478204504344530244537170.00361594doublenullablefd_northingNorthward coordinate of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.lat6.11156e+066.11194e+066.11373e+066.11587e+066.11629e+060.00361594doublenullablefd_altitudeAltitude of the shower core projected at ground level (UTM coordinates system)mpos.bodyrc.alt1541.611544.991570.41592.611592.620.00361594floatnullableauger3.scaler For every Auger station during every second, the scalers record the number of times that the amplitude of the signal is larger than 3 ADC counts, corresponding to an energy deposit of about 15 MeV, and smaller than 21 ADC counts, corresponding to an energy deposit of about 100 MeV. This table allows one to study the temporal behavior of the number of counts, which is modulated by terrestrial and extraterrestrial phenomena.463915inc_timeUnix time in seconds (seconds since 1st Jan 1970, without leap seconds)stime.epoch11122159501126822428.01353658950.01594611972.016073842501.0intindexedrate_corrCorrected scaler ratecount/(m**2.s)phot.flux172.855178.543183.214198.026204.471floatnullablearray_fractionFraction of array in operation%instr;arith.ratio9094.899.499.91001floatnullablerate_uncorraverage detector scaler rate, uncorrectedcount/sphot.flux1691.171781.611870.242024.62115.11floatnullablepressureBarometric pressure at observatoryhPaphys.pressure;obs.atmos838.601849.107856.734864.647872.6671floatnullablebgds From the Bochum Galactic Disk Survey, time series have been obtained in the r and i bands on an (up to) nightly basis. Depending on the field, the time series contain up to more than 300 nights over more than 7 years. Each measurement represents the averaged flux over 10 minutes of observation (from 9 averaged 10s images). The Bochum Galactic Disk Survey is an ongoing project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has been recorded since mid-2010 in Sloan r and i simultaneously with the Robotic Bochum Twin Telescope (RoBoTT) at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of about 2x10^7 stars over more than seven years. Additionally, intermittent measurements in Johnson UVB and Sloan z have been recorded as well.bgds.data The Bochum Galactic Disk Survey is a project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has been recorded from September 2010 to September 2019 with the RoBoTT Telecsope at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of more than 2x10^7 stars. The second and final data release contains follow-up observations from January 2017 to September 2019 in Sloan r and i and intermittent measurements in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII.accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure5501958751.3doubleindexednullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharindexednullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharindexednullableexposureExposure time (per frame)stime.duration;obs.exposurefloatnullableairmassAirmass at mean epochobs.airMassfloatnullablemoondistMoon distance at mean epochdegobs.paramfloatnullablepub_didDataset identifier assigned by the publishermeta.id;meta.maincharnullablebgds.phot_all All mean photometry of bgds in one table. It may be simpler to write queries against the split-band tables phot_band. Measurements in different fields and bands have not been merged, as that procedure is too error-prone in crowded milky way regions.band_nameThe band the mean photometry is given for.meta.id;instr.filtercharnullableobs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharnullableraICRS right ascension for this object.pos.eq.ra;meta.maindoublenullabledecICRS declination for this object.pos.eq.dec;meta.maindoublenullablemean_magMean magnitude in band given in phot_band.magphot.mag;stat.meanfloatnullableerr_magError in mean magnitude in this bandmagstat.error;phot.magfloatnullableampDifference between brightest and weakest observation.magphot.mag;arith.difffloatnullablefluxMean flux in this band; this is computed from the mean magnitude based on Landolt standard stars.mJyphot.flux;stat.meanfloatnullableerr_fluxError in mean flux in this bandmJystat.error;phot.fluxfloatnullablenobsNumber of observations in this light curvemeta.number;obsshortbgds2 From the Bochum Galactic Disk Survey, time series have been obtained in the r and i bands on an (up to) nightly basis. Depending on the field, the time series contain up to more than 300 nights over 9 years. Each measurement in r and i represents the averaged flux over 10 minutes of observation (from 9 averaged 10s images). Additionally, intermittent measurements in Johnson UVB, Sloan z and the narrowbands OIII, NB, Halpha and SII have been recorded as well. The Bochum Galactic Disk Survey is a project to monitor the stellar content of the Galactic disk in a 6 degree wide stripe centered on the Galactic plane. The data has been recorded from September 2010 to September 2019 in Sloan r and i simultaneously with the Robotic Bochum Twin Telescope (RoBoTT) at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It contains measurements of about 2x10^7 stars over nine years. The source images are available from ivo://org.gavo.dc/bgds/q/sia.bgds2.lc_allA union of all BGDS2 light curves. Note that the magnitudes here are in different bands.band_nameThe band the median photometry is given for.meta.id;instr.filtercharnullablemed_magMedian magnitude in the band given in the band_name columnmagphot.mag;em.opt6.8390612.165215.34316.243716.4771floatnullableerr_magError in med_magmagstat.error;phot.mag;em.opt0.005033940.01988610.1358670.2389472.439221floatnullablefluxError in fluxmJystat.error;phot.flux;em.opt0.9315961.154882.6474849.42286674.241floatnullablemagsAn array containing the magnitudes for band_name and the times in mjdmagphot.mag;em.optfloatnullablemag_errsErrors in magsmagstat.error;phot.mag;em.optfloatnullableobs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.011.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min554505545055693.256559.158309.21doublenullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max5545357142.15824658739.1587411doublenullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean55451.556303.457390.957880.158389.41doublenullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start6.65e-076.65e-076.65e-076.65e-076.65e-071floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop8.39e-078.39e-078.39e-078.39e-078.39e-071floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value7.44e-077.44e-077.44e-077.44e-077.44e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00150.00150.00150.00150.00151floatnullablebgds2.phot_all Extracted sources from the Bochum Galactic Disk Survey. We provide median photometry in U, B, V, z, r, and i broadbands as well as the narrow bands OIII, NB, Halpha and SII for particular fields. Note that sources in different bands are not matched. Also, sources sitting in the regions imaged in multiple fields have not been matched even within one band. BGDS light curves are available in i and r for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII in a separate SSAP service and via TAP. For median photometry matched to Gaia DR3 objects, see the bgds2.matched table and the matchedphot service. band_nameThe band the median photometry is given for.meta.id;instr.filtercharnullableobs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullableampDifference between brightest and weakest observation.magphot.mag;em.opt.U;arith.diff00.015640.185370.65400714.61floatnullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in the band given by filtermagphot.mag5.4228910.482213.764114.864919.43321floatnullableerr_magError in med_magmagstat.error;phot.mag0.068970.108090.180010.34473913.58561floatnullablefluxMedian flux in the band given by the filter column; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux0.031952.155375.92536121.70612849.41floatnullableerr_fluxError in median flux in the Johnson U bandmJystat.error;phot.flux0.258620.4367911.0573213.32698899.231floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortgdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullablebgds2.lc_b BGDS DR2 lightcurves in the Johnson B band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.4600000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Johnson B.magphot.mag;em.opt.b;stat.median7.5726713.014116.560317.705718.25051floatnullableerr_magError in median magnitude in Johnson Bmagstat.error;phot.mag;em.opt.b0.008054140.03568650.1314340.2649572.491731floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Johnson B band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.b;stat.median0.2137380.3530231.0138526.5733990.481floatnullableerr_fluxError in median flux in the Johnson B bandmJystat.error;phot.flux;em.opt.b0.02530310.06242710.1317180.9109893682.91floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Johnson B magnitude for the times in mjdmagphot.mag;em.opt.bfloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min561995620056848.157477.258210.21doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max56818.1569085721557575.3582711doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean56621.656849.457047.257514.858236.41doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start3.7e-073.7e-073.7e-073.7e-073.7e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop5.5e-075.5e-075.5e-075.5e-075.5e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value4.41e-074.41e-074.41e-074.41e-074.41e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00140.00140.00140.00140.00141floatnullablebgds2.lc_ha BGDS DR2 lightcurves in the Astrodon Halpha band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.81567obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Astrodon Halpha.magphot.mag;em.line.halpha;stat.median6.0004811.266314.165815.112515.30451floatnullableerr_magError in median magnitude in Astrodon Halphamagstat.error;phot.mag;em.line.halpha0.01429240.03880680.1548930.3469241.147511floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Astrodon Halpha band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.line.halpha;stat.median2.742963.273657.82918113.11514448.91floatnullableerr_fluxError in median flux in the Astrodon Halpha bandmJystat.error;phot.flux;em.line.halpha0.4439940.5682721.177226.04307685.5881floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Astrodon Halpha magnitude for the times in mjdmagphot.mag;em.line.halphafloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min57230.257230.257620.158205.258228.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max57235.257265.25762658270582701doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean57232.757245.857622.758236.958257.51doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start6.53e-076.53e-076.53e-076.53e-076.53e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop6.56e-076.56e-076.56e-076.56e-076.56e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value6.6e-076.6e-076.6e-076.6e-076.6e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00160.00160.00160.00160.00161floatnullablebgds2.lc_i BGDS DR2 lightcurves in the SDSS i' band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.16000000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in SDSS i'.magphot.mag;em.opt.I;stat.median6.8390612.165215.34316.243716.4771floatnullableerr_magError in median magnitude in SDSS i'magstat.error;phot.mag;em.opt.I0.005033940.01988610.1358670.2389472.439221floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the SDSS i' band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.I;stat.median0.9315961.154882.6474849.42286674.241floatnullableerr_fluxError in median flux in the SDSS i' bandmJystat.error;phot.flux;em.opt.I0.06565380.148480.3617541.118893746.161floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.011.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the SDSS i' magnitude for the times in mjdmagphot.mag;em.opt.Ifloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min554505545055693.256559.158309.21doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max5545357142.15824658739.1587411doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean55451.556303.457390.957880.158389.41doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start6.65e-076.65e-076.65e-076.65e-076.65e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop8.39e-078.39e-078.39e-078.39e-078.39e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value7.44e-077.44e-077.44e-077.44e-077.44e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00150.00150.00150.00150.00151floatnullablebgds2.lc_nb BGDS DR2 lightcurves in the Astrodon NB band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.88663obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Astrodon NB.magphot.mag;em.line;stat.median6.0253711.437114.515215.40415.58591floatnullableerr_magError in median magnitude in Astrodon NBmagstat.error;phot.mag;em.line0.01632940.02577410.1490090.2533110.9634131floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Astrodon NB band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.line;stat.median2.116762.502725.6747996.645314121.41floatnullableerr_fluxError in median flux in the Astrodon NB bandmJystat.error;phot.flux;em.line0.2704680.3804290.8305692.391818773.791floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Astrodon NB magnitude for the times in mjdmagphot.mag;em.linefloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min57220.257220.257620.158205.258231.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max57230.257265.25764358271582711doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean57225.257239.457628.758236.8582521doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start6.42e-076.42e-076.42e-076.42e-076.42e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop6.48e-076.48e-076.48e-076.48e-076.48e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value6.45e-076.45e-076.45e-076.45e-076.45e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00130.00130.00130.00130.00131floatnullablebgds2.lc_oiii BGDS DR2 lightcurves in the Astrodon OIII band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.19937obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Astrodon OIII.magphot.mag;em.line.oiii;stat.median6.7774211.005614.379815.185815.33411floatnullableerr_magError in median magnitude in Astrodon OIIImagstat.error;phot.mag;em.line.oiii0.01868690.0213960.1401480.3007030.9565451floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Astrodon OIII band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.line.oiii;stat.median2.669183.059916.42841143.8137064.141floatnullableerr_fluxError in median flux in the Astrodon OIII bandmJystat.error;phot.flux;em.line.oiii0.2773880.4170130.8616523.439325390.621floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Astrodon OIII magnitude for the times in mjdmagphot.mag;em.line.oiiifloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min58205.258205.258205.258207.258226.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max58238.1582685827158271582711doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean58224.958235.558238.758241.358250.81doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start4.97e-074.97e-074.97e-074.97e-074.97e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop5.04e-075.04e-075.04e-075.04e-075.04e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value5e-075e-075e-075e-075e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00120.00120.00120.00120.00121floatnullablebgds2.lc_r BGDS DR2 lightcurves in the SDSS r' band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.21000000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in SDSS r'.magphot.mag;em.opt.r;stat.median8.1200712.922116.306717.31817.53811floatnullableerr_magError in median magnitude in SDSS r'magstat.error;phot.mag;em.opt.r0.006234560.01703590.1247460.2297794.652031floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the SDSS r' band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.r;stat.median0.3505940.4293681.0898424.61472051.161floatnullableerr_fluxError in median flux in the SDSS r' bandmJystat.error;phot.flux;em.opt.r0.02199810.0563920.1319960.4456323147.591floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.011.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the SDSS r' magnitude for the times in mjdmagphot.mag;em.opt.rfloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min5568255684.355911.356560.158175.41doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max5621957142.15824358750.158751.11doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean55853.356378.657148.957762.158260.51doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start5.42e-075.42e-075.42e-075.42e-075.42e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop6.99e-076.99e-076.99e-076.99e-076.99e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value6.12e-076.12e-076.12e-076.12e-076.12e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00130.00130.00130.00130.00131floatnullablebgds2.lc_sii BGDS DR2 lightcurves in the Astrodon SII band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.80329obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Astrodon SII.magphot.mag;em.line;stat.median6.0922711.227414.212315.127915.29531floatnullableerr_magError in median magnitude in Astrodon SIImagstat.error;phot.mag;em.line0.01294740.03457290.1414980.2446480.8972181floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Astrodon SII band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.line;stat.median2.766453.227597.50087117.23213277.61floatnullableerr_fluxError in median flux in the Astrodon SII bandmJystat.error;phot.flux;em.line0.4153630.5422351.060983.939316142.071floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Astrodon SII magnitude for the times in mjdmagphot.mag;em.linefloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min57220.257220.257620.158204.258227.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max57235.257267.25762658270582701doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean57228.957241.457622.758236.558252.11doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start6.69e-076.69e-076.69e-076.69e-076.69e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop6.75e-076.75e-076.75e-076.75e-076.75e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value6.71e-076.71e-076.71e-076.71e-076.71e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00140.00140.00140.00140.00141floatnullablebgds2.lc_u BGDS DR2 lightcurves in the Johnson U band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.392958obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Johnson U.magphot.mag;em.opt.U;stat.median5.4094710.517113.81714.787515.20551floatnullableerr_magError in median magnitude in Johnson Umagstat.error;phot.mag;em.opt.U0.0119430.04242280.143450.2702061.830011floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Johnson U band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.U;stat.median1.568832.305685.63654117.74413001.81floatnullableerr_fluxError in median flux in the Johnson U bandmJystat.error;phot.flux;em.opt.U0.2037330.3956220.7981064.991712510.281floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Johnson U magnitude for the times in mjdmagphot.mag;em.opt.Ufloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min56762.256762.257084.157471.258216.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max56766.157051.257218.157660.4582701doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean56764.456878.157126.457507.358242.61doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start3e-073e-073e-073e-073e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop3.9e-073.9e-073.9e-073.9e-073.9e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value3.46e-073.46e-073.46e-073.46e-073.46e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00170.00170.00170.00170.00171floatnullablebgds2.lc_v BGDS DR2 lightcurves in the Johnson V band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.9300000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in Johnson V.magphot.mag;em.opt.V;stat.median8.2692613.00216.50417.903518.33651floatnullableerr_magError in median magnitude in Johnson Vmagstat.error;phot.mag;em.opt.V0.00762240.03593650.1206130.2543662.10471floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Johnson V band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.V;stat.median0.1775520.2645420.96010324.16191888.91floatnullableerr_fluxError in median flux in the Johnson V bandmJystat.error;phot.flux;em.opt.V0.01762650.04556080.1123160.8671041204.31floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the Johnson V magnitude for the times in mjdmagphot.mag;em.opt.Vfloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min561995619956848.157475.2575611doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max56818.35690857203.257574.1582701doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean56621.656852.357031.557489.9582101doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start4.8e-074.8e-074.8e-074.8e-074.8e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop7.3e-077.3e-077.3e-077.3e-077.3e-071floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value5.5e-075.5e-075.5e-075.5e-075.5e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00150.00150.00150.00150.00151floatnullablebgds2.lc_z BGDS DR2 lightcurves in the SDSS z' band. Lightcurves are available in i' and r' for all fields and partially in U, B, V, z, OIII, NB, Halpha and SII if they have enough observations.6900000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimarygdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablefieldSurvey field observed.meta.id;obs.fieldcharnullablemed_magMedian magnitude in SDSS z'.magphot.mag;em.opt.I;stat.median6.2997911.435614.394115.511616.19861floatnullableerr_magError in median magnitude in SDSS z'magstat.error;phot.mag;em.opt.I0.00655170.04416080.1310690.2460571.9781floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the SDSS z' band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.I;stat.median1.181872.225356.2282795.013610767.31floatnullableerr_fluxError in median flux in the SDSS z' bandmJystat.error;phot.flux;em.opt.I0.1620720.3712050.7870734.326778935.731floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortvar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.001.0shortnullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the SDSS z' magnitude for the times in mjdmagphot.mag;em.opt.Ifloatnullablemag_errsAn array containing per-epoch errors for the mags arraymagstat.error;phot.magfloatnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min56762.256762.256920.157275.158224.11doubleindexednullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max56765.157055.15726757575.2582701doubleindexednullabletime_avgMean epoch of the observationsdtime.epoch;stat.mean56763.656852.157144.857500.458243.11doubleindexednullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharindexednullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start7.78e-077.78e-077.78e-077.78e-077.78e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop1.12e-061.12e-061.12e-061.12e-061.12e-061floatindexednullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value8.96e-078.96e-078.96e-078.96e-078.96e-071floatnullablessa_apertureAngular diameter of aperture. The aperture is elliptical and adaptively scaled for each source using the Kron radius (1980ApJS...43..305K), as implemented in SourceExtractor (1996A&AS..117..393B). The mean FWHM of all sources for each filter is given.degphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00160.00160.00160.00160.00161floatnullablebgds2.phot_b BGDS median photometry in the Johnson B band. This is available for all objects found in the fields observed. Median photometry in the i' and r' bands is given in the lc_(band) tables together with the lightcurves.3300000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main106.132109.369152.004267.724270.871doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9381-63.9872-41.6931-12.0563-7.337971doubleindexednullablemed_mag_bMedian magnitude in Johnson B.magphot.mag;em.opt.b;stat.median8.4077412.929816.512517.796620.89321floatnullableerr_mag_bError in median magnitude in Johnson Bmagstat.error;phot.mag;em.opt.b0.042840.073970.163330.325478.379931floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt.b;arith.diff00.009260.144610.5753411.30451floatnullablefluxMedian flux in the Johnson B band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.b;stat.median0.018740.325681.060828.72471860.761floatnullableerr_fluxError in median flux in the Johnson B bandmJystat.error;phot.flux;em.opt.b0.016440.064150.16942.19471034.391floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortfieldSurvey field observed.meta.id;obs.fieldcharnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296383942332371203.0281317559313674e+185.355030203234772e+186.057357171200772e+1860709988806672263680.9999362longnullablebgds2.phot_u BGDS median photometry in the Johnson U band. This is available for all objects found in the fields observed. Median photometry in the i' and r' bands is given in the lc_(band) tables together with the lightcurves.380671obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doubleindexednullablemed_mag_uMedian magnitude in Johnson U.magphot.mag;em.opt.U;stat.median5.4228910.482213.764114.864919.43321floatnullableerr_mag_uError in median magnitude in Johnson Umagstat.error;phot.mag;em.opt.U0.068970.108090.180010.34473913.58561floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt.U;arith.diff00.015640.185370.65400714.61floatnullablefluxMedian flux in the Johnson U band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.U;stat.median0.031952.155375.92536121.70612849.41floatnullableerr_fluxError in median flux in the Johnson U bandmJystat.error;phot.flux;em.opt.U0.258620.4367911.0573213.32698899.231floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortfieldSurvey field observed.meta.id;obs.fieldcharnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullablebgds2.phot_v BGDS median photometry in the Johnson V band. This is available for all objects found in the fields observed. Median photometry in the i' and r' bands is given in the lc_(band) tables together with the lightcurves.6300000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main106.131109.594157.633268.233270.8691doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9381-64.4271-41.9364-13.2473-7.337851doubleindexednullablemed_mag_vMedian magnitude in Johnson V.magphot.mag;em.opt.V;stat.median8.0420912.92516.540118.002321.15891floatnullableerr_mag_vError in median magnitude in Johnson Vmagstat.error;phot.mag;em.opt.V0.032060.066040.158390.350295.854041floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt.V;arith.diff00.010520.157660.636638.421771floatnullablefluxMedian flux in the Johnson V band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.V;stat.median0.013690.242250.9309325.94172346.821floatnullableerr_fluxError in median flux in the Johnson V bandmJystat.error;phot.flux;em.opt.V0.014650.048640.143731.84851035.121floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortfieldSurvey field observed.meta.id;obs.fieldcharnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296383255137619203.0311013916592205e+185.350285123372937e+186.057376618814555e+1860709985370698288640.99997145longnullablebgds2.phot_z BGDS median photometry in the SDSS z' band. This is available for all objects found in the fields observed. Median photometry in the i' and r' bands is given in the lc_(band) tables together with the lightcurves.4800000obs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.046108.123215.574279.523281.6481doubleindexednullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9381-64.5261-34.4226-3.508710.542751doubleindexednullablemed_mag_zMedian magnitude in SDSS z'.magphot.mag;em.opt.I;stat.median6.311.422814.377515.59621.28541floatnullableerr_mag_zError in median magnitude in SDSS z'magstat.error;phot.mag;em.opt.I0.043930.078760.155870.307858.320031floatnullableampDifference between brightest and weakest observation.magphot.mag;em.opt.I;arith.diff00.013280.171360.5956311.22371floatnullablefluxMedian flux in the SDSS z' band; this is computed from the median magnitude based on Landolt standard stars.mJyphot.flux;em.opt.I;stat.median0.010912.064356.3298596.165410766.21floatnullableerr_fluxError in median flux in the SDSS z' bandmJystat.error;phot.flux;em.opt.I0.207570.379260.963587.803196547.551floatnullablenobsNumber of observations of this objectmeta.number;obs22.03.04.041.0shortfieldSurvey field observed.meta.id;obs.fieldcharnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296383255137619203.0322947096782925e+185.333156398675384e+186.053192289866939e+1860709987432282785280.99991024longnullablebgds2.matched Median photometry in U, B, V, z, r, and i broadbands as well as the narrow bands OIII, NB, Halpha and SII for particular objects; all measurements have been matched to the nearest Gaia DR3 object. For the raw measurements, see the bgds2.phot_all table and the medphot service. 22000000raICRS RA of the object, obtained as the median of all RA measurements of all r and i measurements. If there are no r and i positions, this is the median of the positions from all filters.degpos.eq.ra;meta.maindoubleindexednullabledecICRS Declination of the object, obtained as the median of all declination measurements of all r and i measurements. If there are no r and i positions, this is the median of the positions from all filters.degpos.eq.dec;meta.maindoubleindexednullablegdr3_idGaia DR3 source_id of this object.meta.id;meta.main29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longindexednullablei_med_magMedian magnitude in SDSS i'magphot.mag;em.opt.Ifloatnullableerr_i_med_magUncertainty in i_med_magmagstat.error;phot.mag;em.opt.Ifloatnullablei_fluxMedian flux in SDSS i'mJyphot.flux;em.opt.Ifloatnullableerr_i_fluxUncertainty in i_fluxmJystat.error;phot.flux;em.opt.Ifloatnullabler_med_magMedian magnitude in SDSS r'magphot.mag;em.opt.rfloatnullableerr_r_med_magUncertainty in r_med_magmagstat.error;phot.mag;em.opt.rfloatnullabler_fluxMedian flux in SDSS r'mJyphot.flux;em.opt.rfloatnullableerr_r_fluxUncertainty in r_fluxmJystat.error;phot.flux;em.opt.rfloatnullableha_med_magMedian magnitude in Astrodon Halphamagphot.mag;em.line.halphafloatnullableerr_ha_med_magUncertainty in ha_med_magmagstat.error;phot.mag;em.line.halphafloatnullableha_fluxMedian flux in Astrodon HalphamJyphot.flux;em.line.halphafloatnullableerr_ha_fluxUncertainty in ha_fluxmJystat.error;phot.flux;em.line.halphafloatnullablenb_med_magMedian magnitude in Astrodon NBmagphot.mag;em.linefloatnullableerr_nb_med_magUncertainty in nb_med_magmagstat.error;phot.mag;em.linefloatnullablenb_fluxMedian flux in Astrodon NBmJyphot.flux;em.linefloatnullableerr_nb_fluxUncertainty in nb_fluxmJystat.error;phot.flux;em.linefloatnullableoiii_med_magMedian magnitude in Astrodon OIIImagphot.mag;em.line.oiiifloatnullableerr_oiii_med_magUncertainty in oiii_med_magmagstat.error;phot.mag;em.line.oiiifloatnullableoiii_fluxMedian flux in Astrodon OIIImJyphot.flux;em.line.oiiifloatnullableerr_oiii_fluxUncertainty in oiii_fluxmJystat.error;phot.flux;em.line.oiiifloatnullablesii_med_magMedian magnitude in Astrodon SIImagphot.mag;em.linefloatnullableerr_sii_med_magUncertainty in sii_med_magmagstat.error;phot.mag;em.linefloatnullablesii_fluxMedian flux in Astrodon SIImJyphot.flux;em.linefloatnullableerr_sii_fluxUncertainty in sii_fluxmJystat.error;phot.flux;em.linefloatnullableb_med_magMedian magnitude in Johnson Bmagphot.mag;em.opt.bfloatnullableerr_b_med_magUncertainty in b_med_magmagstat.error;phot.mag;em.opt.bfloatnullableb_fluxMedian flux in Johnson BmJyphot.flux;em.opt.bfloatnullableerr_b_fluxUncertainty in b_fluxmJystat.error;phot.flux;em.opt.bfloatnullableu_med_magMedian magnitude in Johnson Umagphot.mag;em.opt.Ufloatnullableerr_u_med_magUncertainty in u_med_magmagstat.error;phot.mag;em.opt.Ufloatnullableu_fluxMedian flux in Johnson UmJyphot.flux;em.opt.Ufloatnullableerr_u_fluxUncertainty in u_fluxmJystat.error;phot.flux;em.opt.Ufloatnullablev_med_magMedian magnitude in Johnson Vmagphot.mag;em.opt.Vfloatnullableerr_v_med_magUncertainty in v_med_magmagstat.error;phot.mag;em.opt.Vfloatnullablev_fluxMedian flux in Johnson VmJyphot.flux;em.opt.Vfloatnullableerr_v_fluxUncertainty in v_fluxmJystat.error;phot.flux;em.opt.Vfloatnullablez_med_magMedian magnitude in SDSS z'magphot.mag;em.opt.Ifloatnullableerr_z_med_magUncertainty in z_med_magmagstat.error;phot.mag;em.opt.Ifloatnullablez_fluxMedian flux in SDSS z'mJyphot.flux;em.opt.Ifloatnullableerr_z_fluxUncertainty in z_fluxmJystat.error;phot.flux;em.opt.Ifloatnullablevar1 if at least one of the r or i light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.011.0shortnullablesptSpectral type estimated via UBV photometry, the reddening path (from 1956ApJ...124..367H), and the fiducial colours per spectral type (from Tab. 1-2 in 1970A&A.....4..234F). This is only given where UBV photometry is available and the reddening path as a unique intersection with the spectral type.src.sptypecharnullablebgds2.ssa_time_series This table contains metadata about the photometric time series from BGDS in IVOA SSA format. The actual data is available through a datalink service or in the lc_all table.57085431accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typecharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharnullablessa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcecharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxs**-1stat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxs**-1stat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.Calibrationcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.Calibrationcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullableobs_idMain identifier of this observation (a single object may have multiple observations in different bands and fields)meta.id;meta.maincharnullabletime_minFirst timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.min554505545055693.256559.158309.21doublenullabletime_maxLast timestamp in time series (MJD Topocentric UTC)dtime.epoch;stat.max5545357142.15824658739.1587411doublenullableampDifference between brightest and weakest observation.magphot.mag;em.opt;arith.diff00.015640.185370.65400714.61floatnullablemed_magMedian magnitude in the band given in the band_name columnmagphot.mag;em.opt6.8390612.165215.34316.243716.4771floatnullablefieldSurvey field observed.meta.id;obs.fieldcharnullableraICRS right ascension for this object as mean of the positions obtained from source extraction.pos.eq.ra;meta.main100.047103.78152.056280.33283.6751doublenullabledecICRS declination for this object as mean of the positions obtained from the source extraction.pos.eq.dec;meta.main-65.9373-64.2493-34.0598-4.278910.605271doublenullablemjdsAn array containing the time values of the time seriesdtime.epochdoublenullablemagsAn array containing the magnitudes for band_name and the times in mjdmagphot.mag;em.optfloatnullablemag_errsErrors in magsmagstat.error;phot.mag;em.optfloatnullablegdr3_idGaia DR3 source_id of this object.meta.id.cross29296384285929734403.0276701637698514e+185.334893060128903e+186.053414365808342e+1860709987389031877120.99951667longnullablevar1 if the light curves was classified as variable. 0 otherwise. The variability analysis is done only for r and i.meta.code;src.var00.00.00.011.0shortnullablecalifadr3 The Calar Alto Legacy Integral Field Area (CALIFA) survey provides spatially resolved spectroscopic information for 667 galaxies, mainly within the local universe (0.005 < z < 0.03). CALIFA data was obtained using the PPAK integral field unit (IFU), with a hexagonal field-of-view of 1.3 square arcmin, with a 100% covering factor by adopting a three-pointing dithering scheme. has been taken in two setups: V500 (6 Å bin size, 646 galaxies) and V1200 (2.3 Å bin size, 484 galaxies). A final product ("COMBO") combining both data sets, covering 3700-7500 Å at 6 Å bin size, is made availble for 484 galaxies. CALIFA is a legacy survey, intended for the community. This is the (final) Data Release 3. This is the VO/TAP publication with a simple web interface on top. See http://califa.caha.es/ for the upstream site.califadr3.cubes Metadata for the CALIFA data cubes as delivered by the project.1574accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecalifaidCALIFA internal object keymeta.id;meta.mainshortobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent0107206960934800.00296283floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime-6146.555450.156458.35814959214.20.620126doublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime-6146.5562865762658738.163023.50.620108doublenullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit1.23881e-173.184e-074.8e-078.6e-071.837720.996148floatnullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit1.23881e-153.6e-076.99e-071.12e-062.492820.996148floatnullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refval-15502563.5264.644636.44738030.345989floatnullables_raRight ascension of galaxy center, J2000, from NEDdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1020.1413209.025341.7143600.982073doublenullables_decDeclination of galaxy center, J2000, from NEDdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9161-63.4054-18.958256.480589.9880.982073doublenullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBins11.01.03900.06861960.8303535intnullableobs_ext_meanMean atmospheric extinction in V band over all pointings.magobs.atmos.extinction;em.opt.V;stat.meanfloatnullableobs_ext_maxMaximal atmospheric extinction in V band band among all pointings.magobs.atmos.extinction;em.opt.V;stat.maxfloatnullableobs_ext_rmsRMS atmospheric extinction in V band band over all pointingsmagstat.error;obs.atmos.extinction;em.opt.Vfloatnullableflag_obs_extQuality flag for atmospheric extinction in V band (determined as the most severe over mean, max, and rmsmeta.code.qual;obs.atmos.extinction;em.opt.Vshortnullableobs_am_meanMean airmass (secz) over all pointings.magobs.airMass;stat.meanfloatnullableobs_am_maxMaximal airmass (secz) band among all pointings.magobs.airMass;stat.maxfloatnullableobs_am_rmsRMS airmass (secz) band over all pointingsmagstat.error;obs.airMassfloatnullableflag_obs_amQuality flag for airmass (secz) (determined as the most severe over mean, max, and rmsmeta.code.qual;obs.airMassshortnullablered_disp_meanMean spectral dispersion FWHM over all pointings.0.1nminstr.dispersion;stat.meanfloatnullablered_disp_maxMaximal spectral dispersion FWHM band among all pointings.0.1nminstr.dispersion;stat.maxfloatnullablered_disp_rmsRMS spectral dispersion FWHM band over all pointings0.1nmstat.error;instr.dispersionfloatnullableflag_red_dispQuality flag for spectral dispersion FWHM (determined as the most severe over mean, max, and rmsmeta.code.qual;instr.dispersionshortnullablered_cdisp_meanMean cross-dispersion FWHM over all pointings.pixelinstr.dispersion;stat.meanfloatnullablered_cdisp_maxMaximal cross-dispersion FWHM band among all pointings.pixelinstr.dispersion;stat.maxfloatnullablered_cdisp_rmsRMS cross-dispersion FWHM band over all pointingspixelstat.error;instr.dispersionfloatnullableflag_red_cdispQuality flag for cross-dispersion FWHM (determined as the most severe over mean, max, and rmsmeta.code.qual;instr.dispersionshortnullablered_resskyline_minFlux residual of a bright skyline (at 557.7 nm for V500, 435.8 nm for V1200), minimum over all pointingscountstat.fit.residual;spect.line;stat.minfloatnullablered_resskyline_maxFlux residual of a bright skyline (at 557.7 nm for V500, 435.8 nm for V1200), maximum over all pointingscountstat.fit.residual;spect.line;stat.maxfloatnullablered_rmsresskyline_maxRMS flux residual over all fibers of a bright skyline (at 557.7 nm for V500, 435.8 nm for V1200), maximum over all pointingscountstat.fit.residual;spect.line;stat.maxfloatnullableflag_red_skylinesFlag denoting problems with the sky substractionmeta.code.qualshortnullablered_meanstraylight_maxMaximum of mean straylight intensity over all pointingscountinstr.background;stat.meanfloatnullablered_maxstraylight_maxMaximum of maximum straylight intensity over all pointingscountinstr.background;stat.maxfloatnullablered_rmsstraylight_maxMaximum of RMS straylight intensity over all pointingscountinstr.backgroundfloatnullableflag_red_straylightFlag for critical straylight.meta.code.qualshortnullableobs_skymag_meanMean V band sky surface brightness over all pointings.mag/arcsec**2phot.mag.sb;instr.skyLevel;em.opt.V;stat.meanfloatnullableobs_skymag_rmsRMS of V band sky surface brightness over all pointings.mag/arcsec**2stat.error;phot.mag.sb;instr.skyLevel;em.opt.Vfloatnullableflag_obs_skymagFlag for critical sky surface brightness.meta.code.qualshortnullablered_limsb3-sigma limiting surface brightness in B band in mag.mag/arcsec**2phot.mag.sb;em.opt.B;stat.minfloatnullablered_limsbflux3-sigma limiting surface brightness in B band as flux.1e3J.cm**-2.s**-1.m**-1.arcsec**-2floatnullableflag_red_limsbFlag for critical limiting surface brightness sensitivity.meta.code.qualshortnullablered_frac_bigerrFraction of bad pixels (error larger than five times the value) in this cube.instr.det.noise;arith.ratiofloatnullableflag_red_errspecFlag indicating excessive bad pixels.meta.code.qualshortnullablecal_qflux_gAverage flux ratio relative to SDSS g mean over all pointingsphot.flux;em.opt.V;arith.ratiofloatnullablecal_qflux_rAverage flux ratio relative to SDSS r mean over all pointingsphot.flux;em.opt.R;arith.ratiofloatnullablecal_qflux_rmsAverage flux ratio relative to SDSS g and r RMS over all pointingsstat.error;em.opt;arith.ratiofloatnullableflag_cal_specphotoFlag for problems with spectro-photometric calibration.meta.code.qualshortnullablecal_rmsvelmeanRMS of radial velocity residuals of estimates based on 3 or 4 spectral subranges wrt the estimates from the full spectrum.km/sstat.error;instr.calibfloatnullableflag_cal_wlFlag for critical wavelength calibration stability.meta.code.qualshortnullableflag_cal_imgqualFlag for visually evident problems in this cubemeta.code.qualshortnullableflag_cal_specqualFlag for visually evident problems in a 30''-aperture spectrum generated from this cubemeta.code.qualshortnullablecal_flatsdssFlag for visually evident problems in the `SDSS flat' (see source paper); NULL here means: no SDSS flat applied.meta.code.qualshortnullableflag_cal_registrationFlag for visually evident problems in the registration of the synthetic broad-band image with SDSS and related procedures.meta.code.qualshortnullableflag_cal_v1200v500Set if a visual check for the 30''-aperture integrated spectra in V500, V1200, and COMB showed problems.meta.code.qualshortnullableobs_seeing_meanMean FWHM seeing over all pointingsarcsecinstr.obsty.seeing;stat.meanfloatnullableobs_seeing_rmsRMS of FWHM seeing over all pointingsarcsecstat.error;instr.obsty.seeingfloatnullablecal_snr1hlrSignal to noise ratio at the half-light ratio.stat.snrfloatnullablenotesNotesmeta.notecharnullablesetupInstrument setup (V500, V1200, or COMBO)meta.code;instrcharnullablecalifadr3.fluxposv1200 Data cubes of positions and fluxes in the optical for a sample of galaxies, obtained by the CALIFA project in the v1200 setup. Note that due to the dithering scheme, the points here do not actually correspond to raw measurements but instead represent a reduction of several measurements.lambdaWavelength0.1nm36503684.34229.64791.748401floatnullablefluxFlux1e-18J/(s.m**2.nm)-2523.15-0.04757530.01935910.234861962.991floatnullableerrorError in Flux1e-22J/(s.cm**2.nm)-0.8455530.006616720.01635650.1621256.26841e+081floatnullableraj2000Right ascension of spectrum, ICRSdegpos.eq.ra;meta.main0.3186888.65888180.715352.624359.9141doublenullabledej2000Declination of spectrum, ICRSdegpos.eq.dec;meta.main-22.5588-9.0578823.778862.506884.06381doublenullablecalifadr3.fluxposv500 Data cubes of positions and fluxes in the optical for a sample of galaxies, obtained by the CALIFA project in the v500 setup. Note that due to the dithering scheme, the points here do not actually correspond to raw measurements but instead represent a reduction of several measurements.lambdaWavelength0.1nm370138315579735775011floatnullablefluxFlux1e-18J/(s.m**2.nm)-1650.7-0.00728230.01718670.2395081713.911floatnullableerrorError in Flux1e-22J/(s.cm**2.nm)00.00240480.005762960.03227941.26876e+111floatnullableraj2000Right ascension of spectrum, ICRSdegpos.eq.ra;meta.main0.3186888.65888180.715352.624359.9141doublenullabledej2000Declination of spectrum, ICRSdegpos.eq.dec;meta.main-22.5588-9.0578823.778862.506884.06381doublenullablecalifadr3.fluxv1200Flux and errors versus position for CALIFA setup v1200. Positions are pixel indices into the CALIFA cubes. The associate positions are in califadr.spectra; use "JOIN califadr3.spectra USING (califaid, xindex, yindex)" to join that table (or use the fluxpos tables).2147483647lambdaWavelength0.1nm36503684.34229.64791.748401floatindexednullablefluxFlux1e-18J/(s.m**2.nm)-2523.15-0.04757530.01935910.234861962.991floatnullableerrorError in Flux1e-22J/(s.cm**2.nm)-0.8455530.006616720.01635650.1621256.26841e+081floatnullablecalifaidCALIFA id number of the target.meta.id120.0699.03037.090091.0shortindexedxindexX index in the CALIFA grid; V1200 indices are pixel+1000.pos.cartesian.x019.01056.02067.020771.0shortindexedyindexY index in the CALIFA grid; V1200 indexes are pixel+1000pos.cartesian.y015.01052.02064.020721.0shortindexedcalifadr3.spectracalifaidcalifaidxindexxindexyindexyindexcalifadr3.fluxv500Flux and errors versus position for CALIFA setup v500. Positions are pixel indices into the CALIFA cubes. The associate positions are in califadr.spectra; use "JOIN califadr3.spectra USING (califaid, xindex, yindex)" to join that table (or use the fluxpos tables).2147483647lambdaWavelength0.1nm370138315579735775011floatindexednullablefluxFlux1e-18J/(s.m**2.nm)-1650.7-0.00728230.01718670.2395081713.911floatnullableerrorError in Flux1e-22J/(s.cm**2.nm)00.00240480.005762960.03227941.26876e+111floatnullablecalifaidCALIFA id number of the target.meta.id120.0699.03037.090091.0shortindexedxindexX index in the CALIFA grid; V1200 indices are pixel+1000.pos.cartesian.x019.01056.02067.020771.0shortindexedyindexY index in the CALIFA grid; V1200 indexes are pixel+1000pos.cartesian.y015.01052.02064.020721.0shortindexedcalifadr3.spectracalifaidcalifaidxindexxindexyindexyindexcalifadr3.objects Object data for DR3 sample. The photometric and derived quantities are from growth curve analysis of the SDSS images for galaxies from the mother sample (califaid<1000), from SDSS DR7/12 photometry otherwise.667target_nameObject a targeted observation targetedmeta.id;srcobscore:Target.NamecharnullablecalifaidCALIFA internal object keymeta.id;meta.main120.98728.05009.1690091.0shortraj2000Right ascension of the galaxy center, J2000 (from NED)degpos.eq.ra;meta.main0.332418.66344179.404351.839359.9031doublenullabledej2000Right ascension of the galaxy center, J2000 (from NED)degpos.eq.dec;meta.main-22.5492-9.2436523.957962.276184.05261doublenullableredshiftRedshift, from growth curve analysis photometry for mother sample galaxies, from SDSS DR7/12 petrosian photometry otherwise.src.redshift0.00190.00470.01590.03110.08021floatnullablesdss_zRedshift taken from SDSS DR7src.redshift000.014950.02940350.080410.998501floatnullablemaj_axisApparent isophotal major axis from SDSSarcsecphys.angSize;src-3960.8724.133150.9871.24180.50971floatnullablemstarStellar masslog(solMass)phys.mass7.00048.7751710.60611.69111.9591floatnullablemstar_min3 sigma lower limit of Stellar masslog(solMass)phys.mass;stat.min6.82458.679810.49111.552111.8541floatnullablemstar_max3 sigma upper limit of Stellar masslog(solMass)phys.mass;stat.max7.19768.8771310.72311.81312.1691floatnullablechi2χ² of best fitstat.fit.chi20.00229490.03071731.057716.823381.2691floatnullablevmax_nocorrSurvey volume for this galaxy from apparent isophotal diameter and measured redshift (cf. 2014A&A...569A...1W)Mpc**3stat.weight3990178233600001.4777e+061.51e+060.812594floatnullablevmax_denscorrV_max additionally corrected for cosmic variance (cf. 2014A&A...569A...1W)Mpc**3stat.weight5710207462385001.62e+061.82e+060.812594floatnullablemaguMagnitude in the u band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.U12.797513.673415.239417.072323.93691floatnullableerr_maguError in m_ustat.error;phot.mag;em.opt.U12.797513.673415.239417.072323.93691floatnullableu_extExtinction in the u bandphys.absorption;em.opt.U0.037650.0579440.156290.8500411.038090.187406floatnullableabs_u_min3 sigma lower limit of the absolute magnitude in uphot.mag;em.opt.U;stat.min-22.345-21.0308-19.342-15.973-12.4861floatnullableabs_u_max3 sigma upper limit of the absolute magnitude in uphot.mag;em.opt.U;stat.max-21.856-20.7888-19.175-15.832-12.1351floatnullablemaggMagnitude in the g band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.V11.221412.156113.808215.439221.75971floatnullableerr_maggError in m_gstat.error;phot.mag;em.opt.V11.221412.156113.808215.439221.75971floatnullableg_extExtinction in the g bandphys.absorption;em.opt.V00.04054720.114920.6254510.763820.187406floatnullableabs_g_min3 sigma lower limit of the absolute magnitude in gphot.mag;em.opt.V;stat.min-23.538-22.5307-20.689-17.3015-13.371floatnullableabs_g_max3 sigma upper limit of the absolute magnitude in gphot.mag;em.opt.V;stat.max-23.391-22.4436-20.621-17.2049-13.2341floatnullablemagrMagnitude in the r band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.R10.530411.388313.100314.789921.01591floatnullableerr_magrError in m_rstat.error;phot.mag;em.opt.R10.530411.388313.100314.789921.01591floatnullabler_extExtinction in the r bandphys.absorption;em.opt.R0.02010.03091880.084420.4556881150.187406floatnullableabs_r_min3 sigma lower limit of the absolute magnitude in rphot.mag;em.opt.R;stat.min-24.113-23.2408-21.289-17.721-13.5921floatnullableabs_r_max3 sigma upper limit of the absolute magnitude in rphot.mag;em.opt.R;stat.max-34.95-23.2156-21.258-17.6889-13.5241floatnullablemagiMagnitude in the i band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.I10.033611.002112.697414.564420.79871floatnullableerr_magiError in m_istat.error;phot.mag;em.opt.I10.033611.002112.697414.564420.79871floatnullablei_extExtinction in the i bandphys.absorption;em.opt.I0.015240.02344880.064020.3439730.420070.187406floatnullableabs_i_min3 sigma lower limit of the absolute magnitude in iphot.mag;em.opt.I;stat.min-24.557-23.7231-21.681-18.0145-13.8571floatnullableabs_i_max3 sigma upper limit of the absolute magnitude in iphot.mag;em.opt.I;stat.max-34.95-23.672-21.616-17.9516-13.691floatnullablemagzMagnitude in the z band. This is from a growth curve analysis of the SDSS imagery for galaxies in the mother sample (id<1000). Otherwiese, it is the SDSS DR7/12 petrosian magnitude.phot.mag;em.opt.I9.9363610.678412.464114.450820.61791floatnullableerr_magzError in m_zstat.error;phot.mag;em.opt.I9.9363610.678412.464114.450820.61791floatnullablez_extExtinction in the z bandphys.absorption;em.opt.I0.01080.01662320.045390.2438790.297840.187406floatnullableabs_z_min3 sigma lower limit of the absolute magnitude in zphot.mag;em.opt.I;stat.min-24.982-24.1293-22.035-18.2764-14.1111floatnullableabs_z_max3 sigma upper limit of the absolute magnitude in zphot.mag;em.opt.I;stat.max-24.732-24.0371-21.923-18.1659-13.881floatnullablehubtypMorphological type from CALIFA's own visual classification (see 2014A&A...569A...1W for details). (M) indicates definite merging going on, (m) indicates likely merging, (i) indicates signs of interaction.src.morph.typecharminhubtypEarliest morphological type in CALIFA's estimationsrc.morph.typecharmaxhubtypLatest morphological type in CALIFA's estimationsrc.morph.typecharbarBar strength, A -- strong bar, AB -- intermediate, B -- weak bar; with minimum and maximum estimates.meta.code;src.morphcharnullableflag_release_combCube in setup COMB available?meta.code;meta.dataset00.01.01.011.0shortflag_release_v1200Cube in setup V1200 available?meta.code;meta.dataset00.01.01.011.0shortflag_release_v500Cube in setup V500 available?meta.code;meta.dataset00.01.01.011.0shortaxis_ratiob/a axis ratio of a moment-based anaylsis of the SDSS DR7 images (cf. 2014A&A...569A...1W).phys.angSize;arith.ratio0.115160.1831410.560990.9345.091floatnullableposition_anglePosition angle wrt north.degpos.posAng-66.5715-21.496190.3536193.14380.4320.997001floatnullableel_hlrPetrosian half-light radius in r bandarcsecphys.angSize;src0.415394.6140516.23633.279866.9241floatnullablemodmag_rModel magnitude in r bandmagphot.mag;meta.modelled11.901512.461313.730816.604720.82250.187406floatnullablecalifadr3.cubescalifaidcalifaidcalifadr3.spectra Metadata for individual spectra. Note that the spectra result from reducing a complex dithering scheme and are not independent from one another.5100000accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size5000050000.050000.050000.0500001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshift0.00187870.005106670.01527670.0293720.07407871floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio at 500 nm (V500 spectra) or 400 nm (V1200 spectra)stat.snrssa:Derived.SNR-22026.2-0.9841241.268716.38375527.40.991863floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00030.00030.00030.00030.00031floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value55357.955393.456480.957121.957378.21doubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent180024002700360096001floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value5.95e-085.95e-081.876e-071.9e-071.9e-071floatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extent1.19e-071.19e-073.752e-073.8e-073.8e-071floatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start3.65e-073.65e-073.701e-073.749e-073.749e-071floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop4.84e-074.84e-077.501e-077.501e-077.501e-071floatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Length17011701.01877.01901.019011.0intnullableraj2000Right ascension of spectrum, ICRSdegpos.eq.ra;meta.main0.3186888.65888180.715352.624359.9141doubleindexednullabledej2000Declination of spectrum, ICRSdegpos.eq.dec;meta.main-22.5588-9.0578823.778862.506884.06381doubleindexednullablecalifaidCALIFA id number of the target.meta.id120.0699.03037.090091.0shortindexedprimaryxindexX index in the CALIFA grid; V1200 indices are pixel+1000.pos.cartesian.x019.01056.02067.020771.0shortindexedprimaryyindexY index in the CALIFA grid; V1200 indexes are pixel+1000pos.cartesian.y015.01052.02064.020721.0shortindexedprimarycns5 The Fifth Catalogue of Nearby Stars (CNS5) aims to provide the most volume-complete sample of stars in the solar neighbourhood. The CNS5 is compiled based on trigonometric parallaxes from Gaia EDR3 and Hipparcos, and supplemented with astrometric data from Spitzer and ground-based surveys carried out in the infrared. The CNS5 catalogue is statistically complete down to 19.7 mag in G-band and 11.8 mag in W1-band absolute magnitudes, corresponding to a spectral type of L8. Continuous updates of observational data for nearby stars from all sources were collected and evaluated. For all known stars in the 25 pc sphere around the Sun, the best values of positions in space, velocities, and magnitudes in different filters are presented.cns5.main The Fifth Catalogue of Nearby Stars (CNS5) aims to provide the most volume-complete sample of stars in the solar neighbourhood. The CNS5 is compiled based on trigonometric parallaxes from Gaia EDR3 and Hipparcos, and supplemented with astrometric data from Spitzer and ground-based surveys carried out in the infrared. The CNS5 catalogue is statistically complete down to 19.7 mag in G-band and 11.8 mag in W1-band absolute magnitudes, corresponding to a spectral type of L8. Continuous updates of observational data for nearby stars from all sources were collected and evaluated. For all known stars in the 25 pc sphere around the Sun, the best values of positions in space, velocities, and magnitudes in different filters are presented.5909cns5_idCNS5 designationmeta.id;meta.mainlonggj_idGliese-Jahreiss numbermeta.id.crosscharnullablecomponent_idSuffix for a component of binary or multiple systemmeta.code.multipcharnullablen_componentsTotal number of components in the systemmeta.numbershortnullableprimary_flagTrue for the primary of a multiple systemmeta.codeshortnullablegj_system_primaryGliese-Jahriess number of the primary component of the systemmeta.id.crosscharnullablegaia_edr3_idSource identifier in Gaia EDR3meta.id.crosslongnullablehip_idHipparcos identifiermeta.id.crossintnullableraRight ascensiondegpos.eq.ra;meta.maindoubleindexednullabledecDeclinationdegpos.eq.dec;meta.maindoubleindexednullableepochReference epoch for coordinatesyrtime.epochdoublenullablecoordinates_bibcodeSource of the positionmeta.bib;pos.eqcharnullableparallaxAbsolute trigonometric parallaxmaspos.parallax.trigdoublenullableparallax_errorError in parallaxmasstat.error;pos.parallax.trigfloatnullableparallax_bibcodeSource of the parallaxmeta.bib;pos.parallax.trigcharnullablepmraProper motion in right ascensionmas/yrpos.pm;pos.eq.radoublenullablepmra_errorError in pmramas/yrstat.error;pos.pm;pos.eq.radoublenullablepmdecProper motion in declinationmas/yrpos.pm;pos.eq.decdoublenullablepmdec_errorError of pmdecmas/yrstat.error;pos.pm;pos.eq.decdoublenullablepm_bibcodeSource of the proper motionmeta.bib;pos.pmcharnullablervSpectroscopic radial velocitykm/sphys.veloc;pos.barycenterdoublenullablerv_errorError in rvkm/sstat.error;phys.veloc;pos.barycenterdoublenullablerv_bibcodeSource of the radial velocitymeta.bib;phys.veloc;pos.barycentercharnullableg_magG band mean magnitude (corrected)magphot.mag;em.optfloatnullableg_mag_errorError in g_magmagstat.error;phot.mag;em.optdoublenullablebp_magGaia eDR3 integrated BP mean magnitudemagphot.mag;em.opt.bfloatnullablebp_mag_errorError in bp_magmagstat.error;phot.mag;em.opt.bdoublenullablerp_magGaia eDR3 integrated RP mean magnitudemagphot.mag;em.opt.rfloatnullablerp_mag_errorError in rp_magmagstat.error;phot.mag;em.opt.rdoublenullableg_mag_from_hipHipparcos Hp magnitude converted to the G bandmagphot.mag;em.optdoublenullableg_mag_from_hip_errorError in g_mag_from_hipmagstat.error;phot.mag;em.optdoublenullableg_rp_from_hipG - RP colour computed from Hipparcos V and Imagphot.color;em.opt.r;em.optdoublenullableg_rp_from_hip_errorError in g_rp_from_hipmagstat.error;phot.color;em.opt.r;em.optdoublenullableg_mag_resultingResulting (e.g., deblended) G band magnitudemagphot.mag;em.optfloatnullableg_mag_resulting_errorError in g_mag_resultingmagstat.error;phot.mag;em.optdoublenullableg_rp_resultingResulting (e.g., deblended) G - RP colourmagphot.color;em.opt.r;em.optdoublenullableg_rp_resulting_errorError in g_rp_resultingmagstat.error;phot.color;em.opt.r;em.optdoublenullableg_rp_resulting_flag0 – G-RP is deblended; 1 – G-RP is uncorrected vs. eDR3; 2 – G-RP is converted from Hipparcosmeta.code;phot.magshortnullablej_mag2MASS J band magnitudemagphot.mag;em.ir.jfloatnullablej_mag_errorError in j_magmagstat.error;phot.mag;em.ir.jfloatnullableh_mag2MASS H band magnitudemagphot.mag;em.ir.hfloatnullableh_mag_errorError in h_magmagstat.error;phot.mag;em.ir.hfloatnullablek_mag2MASS Ks band magnitudemagphot.mag;em.ir.kfloatnullablek_mag_errorError in k_magmagstat.error;phot.mag;em.ir.kfloatnullablejhk_mag_bibcodeSource of NIR magnitudesmeta.bib;phot.mag;em.ircharnullablew1_magWISE W1 band magnitudemagphot.mag;em.ir.3-4umfloatnullablew1_mag_errorError in w1_magmagstat.error;phot.mag;em.ir.3-4umfloatnullablew2_magWISE W2 band magnitudemagphot.mag;em.ir.4-8umfloatnullablew2_mag_errorError in w2_magmagstat.error;phot.mag;em.ir.4-8umfloatnullablew3_magWISE W3 band magnitudemagphot.mag;em.ir.8-15umfloatnullablew3_mag_errorError in w3_magmagstat.error;phot.mag;em.ir.8-15umfloatnullablew4_magWISE W4 band magnitudemagphot.mag;em.ir.15-30umfloatnullablew4_mag_errorError in w4_magmagstat.error;phot.mag;em.ir.15-30umfloatnullablewise_mag_bibcodeSource of MIR magnitudesmeta.bib;phot.mag;em.ircharnullablegaia This schema contains data re-published from the official Gaia mirrors (such as ivo://uni-heidelberg.de/gaia/tap) either to support combining its data with local tables (the various Xlite tables) or to make the data more accessible to VO clients (e.g., epoch fluxes). Other Gaia-related data is found in, among others, the gdr3mock, gdr3spec, gedr3auto, gedr3dist, gedr3mock, and gedr3spur schemas.gaia.dr2_ts_ssa This table contains about 1.5 Million photometric timeseries for roughly 0.5 Million objects. Photometry is available in the Gaia G, BP, and RP bands for epochs between 2014-07-25 and 2016-05-25. The spectra are available in VOTable format with the timeseries annotation proposed in the Nadvornik et al IVOA note.1700000accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typecharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharnullablessa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcecharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxs**-1stat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxs**-1stat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.Calibrationcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.Calibrationcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullabletime_minFirst timestamp in time series (MJD Barycentric TCB)dtime.epoch;stat.mindoubleindexednullabletime_maxLast timestamp in time series (MJD Barycentric TCB)dtime.epoch;stat.maxdoubleindexednullablegaia.dr2epochflux A table of the light curves released with Gaia DR2 (about half a million in total). In each Gaia band (G, BP, RP), we give epochs, fluxes and their errors in arrays. We do not include the quality flags (DR2: “may be safely ignored for many general purpose applications”). You can access them through the associated datalink service if you select source_id. You will usually join this table with gaia.dr2light. We have also removed all entries with NaN observation times; hence, the array lengths in the different bands can be significantly different, and the indices in transit_ids do not always correspond to the indices in the time series. Furthermore, we only give fluxes and their errors here rather than magnitudes. Fluxes can be turned into magnitude using:: mag = -2.5 log10(flux)+zero point, where the zero points assumed for Gaia DR2 are 25.6884±0.0018 in G, 25.3514±0.0014 in BP, and 24.7619±0.0019 in RP (VEGAMAG).550737source_idUnique source identifier. Note that this *cannot* be matched against the DR1 source_id.meta.id;meta.mainlongindexedprimarytransit_idTransit unique identifier. For a given object, a transit comprises the different Gaia observations (SM, AF, BP, RP and RVS) obtained for each focal plane crossing. NOTE: Where invalid observations have been removed, transit_id *cannot* be joined with times and fluxes.meta.versionlongnullableg_transit_timeThe field-of-view transit averaged observation times for the G-band observations. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullableg_transit_fluxG-band fluxes for the transit, for combination with g_transit_time_mjd. Here, this is a combination of individual SM-AF CCD fluxess**-1phot.flux;em.opt.Vfloatnullableg_transit_flux_errorThe error in G-band flux.s**-1stat.error;phot.flux;em.opt.Vfloatnullablerp_obs_timeThe observation time of the RP CCD transit. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullablerp_fluxRP-band integrated fluxes, for combination with rp_obs_times**-1phot.flux;em.opt.Rfloatnullablerp_flux_errorThe error in RP-band flux.s**-1stat.error;phot.flux;em.opt.Rfloatnullablebp_obs_timeThe observation time of the BP CCD transit. This is given for barycentric TCB in JD-2,455,197.5.dtime.epochdoublenullablebp_fluxBP-band integrated fluxes, for combination with bp_obs_times**-1phot.flux;em.opt.Bfloatnullablebp_flux_errorThe error in BP-band flux.s**-1stat.error;phot.flux;em.opt.Bfloatnullablesolution_idA DPAC id for the toolchain used to produce these particular time series. It is given to facilitate comparison with ESAC data products.meta.versionlonggaia.dr2lightsource_idsource_idgaia.dr2light This is a “light” version of the full Gaia DR2 gaia_source table, containing the original astrometric and photmetric columns with just enough additional information to let careful researchers notice when data is becomes uncertain and the full error model should be consulted. The full DR2 is available from numerous places in the VO (in particular from the TAP services ivo://uni-heidelberg.de/gaia/tap and ivo://esavo/gaia/tap). This table also includes a column containing the Renormalized Unit Weight Error RUWE (GAIA-C3-TN-LU-LL-124-01), a robust measure for the consistency of the solution. On this TAP service, there is the table gdr2dist.main containing distances computed by Bailer-Jones et al (:bibcode:`2018AJ....156...58B`). If in doubt, use these instead of the parallaxes provided here.1600000000source_idUnique source identifier. Note that this *cannot* be matched against the DR1 source_id.meta.id;meta.mainlongindexedprimaryraBarycentric Right Ascension in ICRS at ref_epochdegpos.eq.ra;meta.maindoubleindexednullabledecBarycentric Declination in ICRS at ref_epochdegpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullablepmraProper motion in right ascension of the source in ICRS at ref_epoch. This is the projection of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatindexednullablepmdecProper motion in declination at ref_epoch.mas/yrpos.pm;pos.eq.decfloatindexednullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch ref_epoch. If looking for a distance, consider joining with gdr2dist.main and using the distances from there.maspos.parallaxfloatindexednullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale.magphot.mag;em.opt;stat.meanfloatindexednullablephot_g_mean_fluxG-band mean flux as electrons per second.s**-1phot.flux;em.opt;stat.meandoublenullablephot_g_mean_flux_errorError on phot_g_mean_fluxs**-1stat.error;phot.flux;em.opt;stat.meanfloatnullablephot_rp_mean_fluxMean flux in the integrated RP band.s**-1phot.flux;em.opt.Rdoublenullablephot_rp_mean_flux_errorError in the mean flux in the integrated RP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Rfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Rfloatindexednullablephot_bp_mean_fluxMean flux in the integrated BP band.s**-1phot.flux;em.opt.Bdoublenullablephot_bp_mean_flux_errorError in the mean flux in the integrated BP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Bfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Bfloatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. The radial velocity provided is the median value of the radial velocity measurements at all epochs. Warning: in the vicinity of bright stars, DR2 RVs can be grossly wrong. See arXiv:1901.10460 for details.km/sspect.dopplerVelocfloatnullableradial_velocity_errorThe radial velocity error is the error on the median to which a constant noise floor of 0.11 km/s has been added in quadrature to take into account the calibration contribution.km/sstat.error;spect.dopplerVelocfloatnullableastrometric_gof_alGoodness-of-fit statistic of the astrometric solution for the source in the along-scan direction (you probably want to use RUWE instead of this).stat.fit.goodnessfloatnullableastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.codefloatnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.codelongruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weightfloatnullablegaia.dr3lite This is gaia_source from the Gaia Data Release 3, stripped to just enough columns to enable basic science (but therefore a bit faster and simpler to deal with than the full gaia_source table). Note that on this server, there is also The gedr3dist.main, which gives distances computed by Bailer-Jones et al. Use these in preference to working with the raw parallaxes. This server also carries the gedr3mock schema containing a simulation of gaia_source based on a state-of-the-art galaxy model, computed by Rybizki et al. The full DR3 is available from numerous places in the VO (in particular from the TAP services ivo://uni-heidelberg.de/gaia/tap and ivo://esavo/gaia/tap).1811709771source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longindexedprimaryraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.main1.63271e-0644.3559260.257327.9323601doubleindexednullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.main-89.8559-69.306-25.65858.828789.80891doubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.ra0.003892330.026180.36931612.747299.96761floatnullabledec_errorStandard error of decmasstat.error;pos.eq.dec0.004471330.0252670.34071910.084999.94791floatnullablepmraProper motion in right ascension of the source in ICRS at J2016.0. This is the tangent plane projection (i.e., multiplied by cos(δ)) of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.ra-2290.75-10.761-2.510985.690194002.650.810079floatindexednullablepmdecProper motion in declination at J2016.0.mas/yrpos.pm;pos.eq.dec-5817.8-11.9807-3.107555.227451707.70.810079floatindexednullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.ra0.004197780.03003810.3524571.764463.427460.810079floatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.dec0.005543070.02828050.3147091.553273.442090.810079floatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch J2016.0. If looking for a distance, consider joining with gedr3dist.main and using the distances from there.maspos.parallax-187.029-1.324720.3063952.29237269.0570.810079floatindexednullableparallax_errorStandard error of parallaxmasstat.error;pos.parallax0.007283380.0304280.3430891.506425.575540.810079floatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.mean1.7732815.506819.722921.033322.75070.996994floatindexednullablephot_g_mean_flux_over_errorIntegrated mean G flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt;stat.mean1.0823740.8126240.3572759.6921526.20.996994floatnullablephot_rp_mean_flux_over_errorIntegrated mean RP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.R0.05457844.5115535.5538808.8234.28292e+070.85822floatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.R1.9687414.540418.604320.259924.64070.85822floatindexednullablephot_bp_mean_flux_over_errorIntegrated mean BP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.B0.05579282.6186215.1807468.8943.7971e+070.851071floatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.B2.39815.891120.294321.856525.31610.851071floatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodness0.05097181.059221.309752.559711726.670.850372floatnullableastrometric_excess_noiseThis is the excess noise of the source, measuring the disagreement, expressed as an angle, between the observations of a source and the best-fitting standard astrometric model (using five astrometric parameters). A value of 0 signifies a well-behaved source, a positive value signifies that the residuals are larger than expected.masstat.fit.goodness000.2528616.90813842.4691floatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. For stars brighter than about 12 mag, this is the median of all single-epoch measurements. For fainter stars, RV estimation is from a co-added spectrum.km/sspect.dopplerVeloc.opt;em.opt.I-861.114-102.485-3.6544796.6219859.690.0186703floatnullableradial_velocity_errorError in radial_velocity; this is the error of the median for bright stars. For faint stars, it is derived from the cross-correlation function.km/sstat.error;spect.dopplerVeloc0.1130010.2643623.2835211.2939.99630.0186703floatnullablepseudocolourEffective wavenumber of the source estimated in the final astrometric processing. The pseudocolour is the astrometrically estimated effective wavenumber of the photon flux distribution in the astrometric (G) band, estimated from the chromatic displacements of image centroids. The field is empty when chromaticity was instead taken into account using the photometrically determined ν_eff given in the field nu_eff_used_in_astrometry.um**-1em.wavenumber;phot.color-2.223770.9691671.354041.720255.086220.486942floatnullablepseudocolour_errorStandard error of the pseudocolour.um**-1stat.error;em.wavenumber;phot.color0.001352550.02575120.1098140.3241780.9766360.486942floatnullablevisibility_periods_usedNumber of visibility periods (groups of observations at least 4 days apart) used in the astrometric solution. A small value (less than 10) indicates that the calculated parallax could be more vulnerable to error not reflected in the formal uncertainties.meta.number;obs15.016.028.0331.0shortastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.code33.031.095.0951.0shortnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.code054342273.3905836836.01757319938.899999918117097401.0longindexedruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weight0.2247530.9243341.022951.6219993.41370.810079floatnullablegaia.edr3lite This is a “light” version of the full Gaia DR3 gaia_source table. It is just a view copying gaia.dr3lite, which should preferentially be used in new queries. This table is being kept around in order to keep legacy queries from breaking unnecessarily. However, it is actually DR3 data rather than eDR3. The minute differences did not seem to warrant keeping two copies of the relatively massive data around.1811709771source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongnullableraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.maindoubleindexednullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullablepmraProper motion in right ascension of the source in ICRS at J2016.0. This is the tangent plane projection (i.e., multiplied by cos(δ)) of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatindexednullablepmdecProper motion in declination at J2016.0.mas/yrpos.pm;pos.eq.decfloatindexednullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch J2016.0. If looking for a distance, consider joining with gedr3dist.main and using the distances from there.maspos.parallaxfloatindexednullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.meanfloatindexednullablephot_g_mean_flux_over_errorIntegrated mean G flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt;stat.meanfloatnullablephot_rp_mean_flux_over_errorIntegrated mean RP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Rfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.Rfloatindexednullablephot_bp_mean_flux_over_errorIntegrated mean BP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Bfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.Bfloatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableastrometric_excess_noiseThis is the excess noise of the source, measuring the disagreement, expressed as an angle, between the observations of a source and the best-fitting standard astrometric model (using five astrometric parameters). A value of 0 signifies a well-behaved source, a positive value signifies that the residuals are larger than expected.masstat.fit.goodnessfloatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. For stars brighter than about 12 mag, this is the median of all single-epoch measurements. For fainter stars, RV estimation is from a co-added spectrum.km/sspect.dopplerVeloc.opt;em.opt.Ifloatnullableradial_velocity_errorError in radial_velocity; this is the error of the median for bright stars. For faint stars, it is derived from the cross-correlation function.km/sstat.error;spect.dopplerVelocfloatnullablepseudocolourEffective wavenumber of the source estimated in the final astrometric processing. The pseudocolour is the astrometrically estimated effective wavenumber of the photon flux distribution in the astrometric (G) band, estimated from the chromatic displacements of image centroids. The field is empty when chromaticity was instead taken into account using the photometrically determined ν_eff given in the field nu_eff_used_in_astrometry.um**-1em.wavenumber;phot.colorfloatnullablepseudocolour_errorStandard error of the pseudocolour.um**-1stat.error;em.wavenumber;phot.colorfloatnullablevisibility_periods_usedNumber of visibility periods (groups of observations at least 4 days apart) used in the astrometric solution. A small value (less than 10) indicates that the calculated parallax could be more vulnerable to error not reflected in the formal uncertainties.meta.number;obsshortastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.codeshortnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.codelongindexedruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weightfloatnullablegdr2ap We estimated the stellar astrophysical parameters of 120 million stars over the entire sky that have Gaia parallax and photometry from Gaia DR2, 2MASS, and AllWISE. We provide estimates of log age, log mass, log temperature, log luminosity, log surface gravity, distance modulus, dust extinction (A0), and average grain size (R0) along the lines of sight. In contrast with other catalogs, we do not use a Galactic model as prior but weakly informative ones. Our estimate and uncertainties are quantiles, so they are invariant under monotonic transformations (e.g., log, exp). This means that one can use our median estimate to obtain the median distance or temperature, for instance, and likewise for the uncertainties.gdr2ap.main We estimated the stellar astrophysical parameters of 120 million stars over the entire sky that have Gaia parallax and photometry from Gaia DR2, 2MASS, and AllWISE. We provide estimates of log age, log mass, log temperature, log luminosity, log surface gravity, distance modulus, dust extinction (A0), and average grain size (R0) along the lines of sight. In contrast with other catalogs, we do not use a Galactic model as prior but weakly informative ones. Our estimate and uncertainties are quantiles, so they are invariant under monotonic transformations (e.g., log, exp). This means that one can use our median estimate to obtain the median distance or temperature, for instance, and likewise for the uncertainties.130000000source_idUnique source identifier. Note that this *cannot* be matched against the DR1 source_id.meta.id;meta.mainlongindexedprimarya0_bestmultivariate maximum posterior estimate for the dust exctinction A₀ towards this source.magphys.absorptionfloatnullablea0_p50median of the distribution of dust exctinction A₀ towards this source.magphys.absorption;stat.medianfloatindexednullablea0_distDistribution (min, p16, p25, p50, p75, p84, max) of the dust exctinction A₀ towards this source. In ADQL, write a0_dist[1] for the minimum, a0_dist[2] for the 16th percentile, and so on.magstat;phys.absorptionfloatnullabler0_bestmultivariate maximum posterior estimate for the average dust grain size extinction parameter.phys.absorptionfloatnullabler0_p50median of the distribution of average dust grain size extinction parameter.phys.absorption;stat.medianfloatindexednullabler0_distDistribution (min, p16, p25, p50, p75, p84, max) of the average dust grain size extinction parameter. In ADQL, write r0_dist[1] for the minimum, r0_dist[2] for the 16th percentile, and so on.stat;phys.absorptionfloatnullableloga_bestmultivariate maximum posterior estimate for the log10 of the age.log(yr)time.agefloatnullableloga_p50median of the distribution of log10 of the age.log(yr)time.age;stat.medianfloatnullableloga_distDistribution (min, p16, p25, p50, p75, p84, max) of the log10 of the age. In ADQL, write loga_dist[1] for the minimum, loga_dist[2] for the 16th percentile, and so on.log(yr)stat;time.agefloatnullablelogl_bestmultivariate maximum posterior estimate for the log10 of the luminosity.log(solLum)phys.luminosityfloatnullablelogl_p50median of the distribution of log10 of the luminosity.log(solLum)phys.luminosity;stat.medianfloatindexednullablelogl_distDistribution (min, p16, p25, p50, p75, p84, max) of the log10 of the luminosity. In ADQL, write logl_dist[1] for the minimum, logl_dist[2] for the 16th percentile, and so on.log(solLum)stat;phys.luminosityfloatnullablelogm_bestmultivariate maximum posterior estimate for the log10 of the mass.log(solMass)phys.massfloatnullablelogm_p50median of the distribution of log10 of the mass.log(solMass)phys.mass;stat.medianfloatnullablelogm_distDistribution (min, p16, p25, p50, p75, p84, max) of the log10 of the mass. In ADQL, write logm_dist[1] for the minimum, logm_dist[2] for the 16th percentile, and so on.log(solMass)stat;phys.massfloatnullablelogt_bestmultivariate maximum posterior estimate for the log10 of the effective temperature.log(K)phys.temperaturefloatnullablelogt_p50median of the distribution of log10 of the effective temperature.log(K)phys.temperature;stat.medianfloatindexednullablelogt_distDistribution (min, p16, p25, p50, p75, p84, max) of the log10 of the effective temperature. In ADQL, write logt_dist[1] for the minimum, logt_dist[2] for the 16th percentile, and so on.log(K)stat;phys.temperaturefloatnullablelogg_bestmultivariate maximum posterior estimate for the log10 of the surface gravity.log(cm/s**2)phys.gravityfloatnullablelogg_p50median of the distribution of log10 of the surface gravity.log(cm/s**2)phys.gravity;stat.medianfloatnullablelogg_distDistribution (min, p16, p25, p50, p75, p84, max) of the log10 of the surface gravity. In ADQL, write logg_dist[1] for the minimum, logg_dist[2] for the 16th percentile, and so on.log(cm/s**2)stat;phys.gravityfloatnullablea_bp_bestmultivariate maximum posterior estimate for the attenuation in the Gaia BP band towards this source..magphys.absorption;em.opt.Bfloatnullablea_bp_p50median of the distribution of attenuation in the Gaia BP band towards this source..magphys.absorption;em.opt.B;stat.medianfloatnullablea_bp_distDistribution (min, p16, p25, p50, p75, p84, max) of the attenuation in the Gaia BP band towards this source.. In ADQL, write a_bp_dist[1] for the minimum, a_bp_dist[2] for the 16th percentile, and so on.magstat;phys.absorption;em.opt.Bfloatnullablea_g_bestmultivariate maximum posterior estimate for the attenuation in the Gaia G band towards this source..magphys.absorption;em.optfloatnullablea_g_p50median of the distribution of attenuation in the Gaia G band towards this source..magphys.absorption;em.opt;stat.medianfloatnullablea_g_distDistribution (min, p16, p25, p50, p75, p84, max) of the attenuation in the Gaia G band towards this source.. In ADQL, write a_g_dist[1] for the minimum, a_g_dist[2] for the 16th percentile, and so on.magstat;phys.absorption;em.optfloatnullablea_rp_bestmultivariate maximum posterior estimate for the attenuation in the Gaia RP band towards this source..magphys.absorptionfloatnullablea_rp_p50median of the distribution of attenuation in the Gaia RP band towards this source..magphys.absorption;stat.medianfloatnullablea_rp_distDistribution (min, p16, p25, p50, p75, p84, max) of the attenuation in the Gaia RP band towards this source.. In ADQL, write a_rp_dist[1] for the minimum, a_rp_dist[2] for the 16th percentile, and so on.magstat;phys.absorptionfloatnullablemag_bpRecalibrated Gaia BP magnitude.magphot.mag;em.opt.Bfloatnullableerr_bpRecalibrated error from original Gaia BP magnitude.magstat.error;phot.mag;em.opt.Bfloatnullablebp_bestmultivariate maximum posterior estimate for the Gaia BP magnitude.magphot.mag;em.opt.Bfloatnullablebp_p50median of the distribution of Gaia BP magnitude.magphot.mag;em.opt.B;stat.medianfloatnullablebp_distDistribution (min, p16, p25, p50, p75, p84, max) of the Gaia BP magnitude. In ADQL, write bp_dist[1] for the minimum, bp_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.opt.Bfloatnullablemag_gRecalibrated Gaia G magnitude.magphot.mag;em.optfloatnullableerr_gRecalibrated error from original Gaia G magnitude.magstat.error;phot.mag;em.optfloatnullableg_bestmultivariate maximum posterior estimate for the Gaia G magnitude.magphot.mag;em.optfloatnullableg_p50median of the distribution of Gaia G magnitude.magphot.mag;em.opt;stat.medianfloatnullableg_distDistribution (min, p16, p25, p50, p75, p84, max) of the Gaia G magnitude. In ADQL, write g_dist[1] for the minimum, g_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.optfloatnullablemag_rpRecalibrated Gaia RP magnitude.magphot.mag;em.opt.Rfloatnullableerr_rpRecalibrated error from original Gaia RP magnitude.magstat.error;phot.mag;em.opt.Rfloatnullablerp_bestmultivariate maximum posterior estimate for the Gaia RP magnitude.magphot.mag;em.opt.Rfloatnullablerp_p50median of the distribution of Gaia RP magnitude.magphot.mag;em.opt.R;stat.medianfloatnullablerp_distDistribution (min, p16, p25, p50, p75, p84, max) of the Gaia RP magnitude. In ADQL, write rp_dist[1] for the minimum, rp_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.opt.Rfloatnullablemag_jRecalibrated 2MASS J magnitude.magphot.mag;em.IR.Jfloatnullableerr_jRecalibrated error from original 2MASS J magnitude.magstat.error;phot.mag;em.IR.Jfloatnullablej_bestmultivariate maximum posterior estimate for the 2MASS J magnitude.magphot.mag;em.IR.Jfloatnullablej_p50median of the distribution of 2MASS J magnitude.magphot.mag;em.IR.J;stat.medianfloatnullablej_distDistribution (min, p16, p25, p50, p75, p84, max) of the 2MASS J magnitude. In ADQL, write j_dist[1] for the minimum, j_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.IR.Jfloatnullablemag_hRecalibrated 2MASS H magnitude.magphot.mag;em.IR.Hfloatnullableerr_hRecalibrated error from original 2MASS H magnitude.magstat.error;phot.mag;em.IR.Hfloatnullableh_bestmultivariate maximum posterior estimate for the 2MASS H magnitude.magphot.mag;em.IR.Hfloatnullableh_p50median of the distribution of 2MASS H magnitude.magphot.mag;em.IR.H;stat.medianfloatnullableh_distDistribution (min, p16, p25, p50, p75, p84, max) of the 2MASS H magnitude. In ADQL, write h_dist[1] for the minimum, h_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.IR.Hfloatnullablemag_ksRecalibrated 2MASS Ks magnitude.magphot.mag;em.IR.Kfloatnullableerr_ksRecalibrated error from original 2MASS Ks magnitude.magstat.error;phot.mag;em.IR.Kfloatnullableks_bestmultivariate maximum posterior estimate for the 2MASS Ks magnitude.magphot.mag;em.IR.Kfloatnullableks_p50median of the distribution of 2MASS Ks magnitude.magphot.mag;em.IR.K;stat.medianfloatnullableks_distDistribution (min, p16, p25, p50, p75, p84, max) of the 2MASS Ks magnitude. In ADQL, write ks_dist[1] for the minimum, ks_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.IR.Kfloatnullablemag_w1Recalibrated WISE W1 magnitude.magphot.mag;em.IR.3-4umfloatnullableerr_w1Recalibrated error from original WISE W1 magnitude.magstat.error;phot.mag;em.IR.3-4umfloatnullablew1_bestmultivariate maximum posterior estimate for the WISE W1 magnitude.magphot.mag;em.IR.3-4umfloatnullablew1_p50median of the distribution of WISE W1 magnitude.magphot.mag;em.IR.3-4um;stat.medianfloatnullablew1_distDistribution (min, p16, p25, p50, p75, p84, max) of the WISE W1 magnitude. In ADQL, write w1_dist[1] for the minimum, w1_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.IR.3-4umfloatnullablemag_w2Recalibrated WISE W2 magnitude.magphot.mag;em.IR.4-8umfloatnullableerr_w2Recalibrated error from original WISE W2 magnitude.magstat.error;phot.mag;em.IR.4-8umfloatnullablew2_bestmultivariate maximum posterior estimate for the WISE W2 magnitude.magphot.mag;em.IR.4-8umfloatnullablew2_p50median of the distribution of WISE W2 magnitude.magphot.mag;em.IR.4-8um;stat.medianfloatnullablew2_distDistribution (min, p16, p25, p50, p75, p84, max) of the WISE W2 magnitude. In ADQL, write w2_dist[1] for the minimum, w2_dist[2] for the 16th percentile, and so on.magstat;phot.mag;em.IR.4-8umfloatnullabledmod_bestmultivariate maximum posterior estimate for the distance modulus.magphot.mag.distModfloatnullabledmod_p50median of the distribution of distance modulus.magphot.mag.distMod;stat.medianfloatnullabledmod_distDistribution (min, p16, p25, p50, p75, p84, max) of the distance modulus. In ADQL, write dmod_dist[1] for the minimum, dmod_dist[2] for the 16th percentile, and so on.magstat;phot.mag.distModfloatnullablelnlike_bestmultivariate maximum posterior estimate for the log likelihood of the solution (paper Eq. 1).stat.paramfloatnullablelnlike_p50median of the distribution of log likelihood of the solution (paper Eq. 1).stat.param;stat.medianfloatnullablelnlike_distDistribution (min, p16, p25, p50, p75, p84, max) of the log likelihood of the solution (paper Eq. 1). In ADQL, write lnlike_dist[1] for the minimum, lnlike_dist[2] for the 16th percentile, and so on.stat;stat.paramfloatnullablelnp_bestmultivariate maximum posterior estimate for the log posterior of the solution (paper Eq. 2).stat.probabilityfloatnullablelnp_p50median of the distribution of log posterior of the solution (paper Eq. 2).stat.probability;stat.medianfloatnullablelnp_distDistribution (min, p16, p25, p50, p75, p84, max) of the log posterior of the solution (paper Eq. 2). In ADQL, write lnp_dist[1] for the minimum, lnp_dist[2] for the 16th percentile, and so on.stat;stat.probabilityfloatnullablelog10jitter_bestmultivariate maximum posterior estimate for the log photometric likelihood jitter common to all bands.log(mag)stat.paramfloatnullablelog10jitter_p50median of the distribution of log photometric likelihood jitter common to all bands.log(mag)stat.param;stat.medianfloatnullablelog10jitter_distDistribution (min, p16, p25, p50, p75, p84, max) of the log photometric likelihood jitter common to all bands. In ADQL, write log10jitter_dist[1] for the minimum, log10jitter_dist[2] for the 16th percentile, and so on.log(mag)stat;stat.paramfloatnullableparallaxRecalibrated parallax.maspos.parallaxfloatnullableerr_parallaxError in recalibrated parallax.masstat.error;pos.parallaxfloatnullablegdr3spec This is a re-publication the Gaia DR3 RP/BP spectra in the IVOA Spectral Data Model. It presents the continous spectra in sampled form, using a Monte Carlo scheme to decorrelate errors, elaborated in this resource's reference URL. The underlying tables are also available for querying through TAP, which opens some powerful methods for mass-analysing the data.gdr3spec.spectraThis table contains the sampled spectra, their errors (as the standard deviation of the samples between the different realisations), and the Gaia DR3 source_id. Join this table on source_id with gaia.dr3lite to obtain information on the sources.219196404source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longindexedprimaryfluxmean BP + RP combined spectrum fluxW.m**-2.nm**-1phot.flux;em.optfloatnullableflux_errormean BP + RP combined spectrum flux errorW.m**-2.nm**-1stat.error;phot.flux;em.optfloatnullablegdr3spec.ssametaSSA Metadata for the Monte Carlo-sampled Gaia DR3 XP spectra219196404phot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.mean1.7732815.506819.722921.033322.75070.996994floatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.B2.39815.891120.294321.856525.31610.851071floatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.R1.9687414.540418.604320.259924.64070.85822floatnullablesource_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longnullableraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.main1.63271e-0644.3559260.257327.9323601doublenullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.main-89.8559-69.306-25.65858.828789.80891doublenullablepreviewURL of a preview for the datasetmeta.ref.url;meta.previewcharnullableaccrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharnullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.Formatapplication/x-votable+xmlcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoublenullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.Unitnmcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.UnitW.m**-2.nm**-1charssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionGaia DR3 XPcharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationABSOLUTEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperturedoublenullablegdr3spec.withposThis table contains the data from gdr3spec.spectra plus position and photometry from gaia.dr3lite. It is a view, and there is generally no advantage to using it instead of manually performing the join.219196404source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longnullableraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.main1.63271e-0644.3559260.257327.9323601doublenullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.main-89.8559-69.306-25.65858.828789.80891doublenullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.ra0.003892330.026180.36931612.747299.96761floatnullabledec_errorStandard error of decmasstat.error;pos.eq.dec0.004471330.0252670.34071910.084999.94791floatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.mean1.7732815.506819.722921.033322.75070.996994floatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.B2.39815.891120.294321.856525.31610.851071floatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.R1.9687414.540418.604320.259924.64070.85822floatnullablefluxmean BP + RP combined spectrum fluxW.m**-2.nm**-1phot.flux;em.optfloatnullableflux_errormean BP + RP combined spectrum flux errorW.m**-2.nm**-1stat.error;phot.flux;em.optfloatnullablegedr3dist We estimate the distance from the Sun to sources in Gaia eDR3 that have parallaxes. We provide two types of distance estimate, together with their corresponding asymmetric uncertainties, using Bayesian posterior density functions that we sample for each source. Our prior is based on a detailed model of the 3D spatial, colour, and magnitude distribution of stars in our Galaxy that includes a 3D map of interstellar extinction. The first type of distance estimate is purely geometric, in that it only makes use of the Gaia parallax and parallax uncertainty. This uses a direction-dependent distance prior derived from our Galaxy model. The second type of distance estimate is photogeometric: in addition to parallax it also uses the source's G-band magnitude and BP-RP colour. This type of estimate uses the geometric prior together with a direction-dependent and colour-dependent prior on the absolute magnitude of the star. Our distance estimate and uncertainties are quantiles, so are invariant under logarithmic transformations. This means that our median estimate of the distance can be used to give the median estimate of the distance modulus, and likewise for the uncertainties. For applications that cannot be satisfied through TAP, you can download a `full table dump`_. .. _full table dump: /gedr3dist/q/download/formgedr3dist.litewithdistThis table joins the DR3 "lite" table (consisting only of the columns necessary for the most basic science) with the estimated geometric and photogeometric distances. Note that this is an inner join, i.e., DR3 objects without distance estimates will not show up here. Note: Due to current limitations of the postgres query planner, this table cannot usefully be used in positional joins ("crossmatches"). See the `Tricking the query planner`_ example. .. _tricking the query planner: http://dc.g-vo.org/tap/examples#Trickingthequeryplanner1470000000source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongnullableraBarycentric Right Ascension in ICRS at epoch J2016.0degpos.eq.ra;meta.maindoubleindexednullabledecBarycentric Declination in ICRS at epoch J2016.0degpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullablepmraProper motion in right ascension of the source in ICRS at J2016.0. This is the tangent plane projection (i.e., multiplied by cos(δ)) of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatindexednullablepmdecProper motion in declination at J2016.0.mas/yrpos.pm;pos.eq.decfloatindexednullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch J2016.0. If looking for a distance, consider joining with gedr3dist.main and using the distances from there.maspos.parallaxfloatindexednullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.meanfloatindexednullablephot_g_mean_flux_over_errorIntegrated mean G flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt;stat.meanfloatnullablephot_rp_mean_flux_over_errorIntegrated mean RP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Rfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.Rfloatindexednullablephot_bp_mean_flux_over_errorIntegrated mean BP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Bfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.Bfloatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableastrometric_excess_noiseThis is the excess noise of the source, measuring the disagreement, expressed as an angle, between the observations of a source and the best-fitting standard astrometric model (using five astrometric parameters). A value of 0 signifies a well-behaved source, a positive value signifies that the residuals are larger than expected.masstat.fit.goodnessfloatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. For stars brighter than about 12 mag, this is the median of all single-epoch measurements. For fainter stars, RV estimation is from a co-added spectrum.km/sspect.dopplerVeloc.opt;em.opt.Ifloatnullableradial_velocity_errorError in radial_velocity; this is the error of the median for bright stars. For faint stars, it is derived from the cross-correlation function.km/sstat.error;spect.dopplerVelocfloatnullablepseudocolourEffective wavenumber of the source estimated in the final astrometric processing. The pseudocolour is the astrometrically estimated effective wavenumber of the photon flux distribution in the astrometric (G) band, estimated from the chromatic displacements of image centroids. The field is empty when chromaticity was instead taken into account using the photometrically determined ν_eff given in the field nu_eff_used_in_astrometry.um**-1em.wavenumber;phot.colorfloatnullablepseudocolour_errorStandard error of the pseudocolour.um**-1stat.error;em.wavenumber;phot.colorfloatnullablevisibility_periods_usedNumber of visibility periods (groups of observations at least 4 days apart) used in the astrometric solution. A small value (less than 10) indicates that the calculated parallax could be more vulnerable to error not reflected in the formal uncertainties.meta.number;obsshortastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.codeshortnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.codelongindexedruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weightfloatnullabler_med_geoThe median of the geometric distance posterior. The geometric distance estimate.pcpos.distancefloatindexednullabler_lo_geoThe 16th percentile of the geometric distance posterior. The lower 1-sigma-like bound on the confidence interval.pcpos.distance;stat.minfloatnullabler_hi_geoThe 84th percentile of the geometric distance posterior. The upper 1-sigma-like bound on the confidence interval.pcpos.distance;stat.maxfloatnullabler_med_photogeoThe median of the photogeometric distance posterior. The photogeometric distance estimate.pcpos.distancefloatindexednullabler_lo_photogeoThe 16th percentile of the photogeometric distance posterior. The lower 1-sigma-like bound on the confidence interval.pcpos.distance;stat.minfloatnullabler_hi_photogeoThe 84th percentile of the photogeometric distance posterior. The upper 1-sigma-like bound on the confidence interval.pcpos.distance;stat.maxfloatnullableflagAdditional information on the solution. Do not use for filtering (see table note in the reference URL).meta.codecharnullablegedr3dist.main We estimate the distance from the Sun to sources in Gaia eDR3 that have parallaxes. We provide two types of distance estimate, together with their corresponding asymmetric uncertainties, using Bayesian posterior density functions that we sample for each source. Our prior is based on a detailed model of the 3D spatial, colour, and magnitude distribution of stars in our Galaxy that includes a 3D map of interstellar extinction. The first type of distance estimate is purely geometric, in that it only makes use of the Gaia parallax and parallax uncertainty. This uses a direction-dependent distance prior derived from our Galaxy model. The second type of distance estimate is photogeometric: in addition to parallax it also uses the source's G-band magnitude and BP-RP colour. This type of estimate uses the geometric prior together with a direction-dependent and colour-dependent prior on the absolute magnitude of the star. Our distance estimate and uncertainties are quantiles, so are invariant under logarithmic transformations. This means that our median estimate of the distance can be used to give the median estimate of the distance modulus, and likewise for the uncertainties. For applications that cannot be satisfied through TAP, you can download a `full table dump`_. .. _full table dump: /gedr3dist/q/download/form1470000000source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longindexedprimaryr_med_geoThe median of the geometric distance posterior. The geometric distance estimate.pcpos.distance2.54595640.7684096.157643.5662691.51floatindexednullabler_lo_geoThe 16th percentile of the geometric distance posterior. The lower 1-sigma-like bound on the confidence interval.pcpos.distance;stat.min2.54571514.5692483.125224.3247253.61floatnullabler_hi_geoThe 84th percentile of the geometric distance posterior. The upper 1-sigma-like bound on the confidence interval.pcpos.distance;stat.max2.54621757.9756397.3811446.489501.51floatnullabler_med_photogeoThe median of the photogeometric distance posterior. The photogeometric distance estimate.pcpos.distance2.54585674.0164329.7510465.559393.70.917561floatindexednullabler_lo_photogeoThe 16th percentile of the photogeometric distance posterior. The lower 1-sigma-like bound on the confidence interval.pcpos.distance;stat.min2.54569600.533344.348572.346482.30.917561floatnullabler_hi_photogeoThe 84th percentile of the photogeometric distance posterior. The upper 1-sigma-like bound on the confidence interval.pcpos.distance;stat.max2.54611748.4765707.5213015.2858530.917561floatnullableflagAdditional information on the solution. Do not use for filtering (see table note in the reference URL).meta.codecharnullablegedr3mock This catalogue is a simulation of the Gaia EDR3 stellar content using Galaxia (a tool to sample stars from a Besancon-like Milky Way model), 3d dust extinction maps and the latest PARSEC Isochrones. It is mimicking the Gaia DR2 data model and an apparent magnitude limit of G=20,7. Extinctions and photometry in different bands have also been included in a supplementary table as well as uncertainty estimates using scaled GDR2 errors. Additional magnitude limit per HEALpix maps are provided, based on the mode in the magnitude distribution of Gaia DR2 data.gedr3mock.generated_dataThis contains the data actually generated. Users probably want to use the gdr2mock.main table that (fairly well) follows the Gaia DR2 data model.1600000000teffeffective TemperatureK668.743464.335557.167058.742133531floatfehlog of metallicity in solar units ('dex')-3.85583-0.835298-0.06409740.4228291.384841floata0monochramatic Extinction at lambda=547.7nmmag00.1009861.238624.8685722.21581floatlumStellar luminositysolLum-4.46797-1.639190.05167021.783755.882351floatlGalactic longitudedeg7.01627e-071.68645197.614357.8843601doublebGalactic latitudedeg-89.9153-32.1305-2.3438623.416789.90741doublesmassinitial mass in solar massessolMass0.09000280.4285950.9083381.7286757.94461floatageAge of the starGyr5.048436.29511e+087.78739e+091.16998e+101.35e+101floatloggSurface gravity of starlog(cm/(s**2))-3.351282.389414.380764.826888.527171floatphot_g_mean_magapparent G mag including extinctionmag0.53617315.149919.48820.643820.71floatindexedphot_bp_mean_magapparent BP mag including extinctionmag0.50138615.748920.301321.913430.24681floatindexedphot_rp_mean_magapparent RP mag including extinctionmag0.57550314.434318.625119.801821.01631floatindexedphot_rvs_mean_magapparent RVS mag including extinctionmag0.073060914.110118.221919.476121.10291floatpopidPopulation ID according to the Besancon model. Including SMC/LMC = 10 and stellar clusters = 1101.06.09.0111.0shortmactactual (present) mass in solar massessolMass0.090.4284130.9047381.725148.23021floatphot_g_mean_mag_errorerror in Gmag0.0001171590.0004017250.00316970.007837340.03687061floata_gExtinction in Gmag00.07635151.024093.6856912.83881floata_bpExtinction in BPmag00.102341.295034.8623319.41441floata_rpExtinction in RPmag00.0621790.7899122.9863211.3391floata_rvsExtinction in RVSmag00.05277860.6475882.5433211.57781floatparallaxparallax in masmas0.002025750.07771660.2068031.44307344.5271floatindexedradial_velocityRadial velocity in km/skm/s-1020.02-164.951-2.29996192.4181017.541floatpm_raProper motion in projection of right ascensionmas/yr-1256.07-9.64812-2.362474.699875662.041floatpm_decProper motion in declinationmas/yr-2030.75-11.0463-2.945894.943971708.881floatparallax_errorparallax uncertainty in masmas0.01005820.03382770.3108270.776591.516271floatradial_velocity_errorRadial velocity uncertainty in km/skm/s0.1076213.977247.8922810.863914.85561floatphot_g_n_obsNumber of photometric observations (trained from DR2 scaled to DR3 time)95157.0311.0658.031941.0shortvisibility_periods_usedNumber of observations effectively used for the astrometric solutions (trained from DR2 scaled to DR3)913.017.026.0341.0shortsource_idHealpix number using Nside = 4096 with the nested scheme on equatorial coordinates times 2^35. The last digits of the source_id are reserved for a running number that serves as a unique identifier per HEALPix cell. This is formed in accordance with Gaia's source_id definition, but of course mock objects have no relation to any Gaia objects that may have an identical source_id.meta.id;meta.main31610959298575.0547592736530234e+174.253777047802872e+186.68145365260706e+1869175284091657912321.0longindexedprimaryraBarycentric Right Ascension in ICRS at ref_epochdegpos.eq.ra;meta.main2.07962e-0557.9741263.95322.9733601doubleindexednullabledecBarycentric Declination in ICRS at ref_epochdegpos.eq.dec;meta.main-89.9929-69.0995-27.64358.222489.93971doubleindexednullableindex_parsec[GeDR3mock only] Foreign key into the photometry/extinction table, .meta.id.cross1018201267176030.0101187030.0135185017.02172430361.0intindexedrandom_indexRandom index that can be used to deterministically select subsets2547207854.76786746291.01526251106.6215734573151.0intindexedd11y[GeDR3mock only] Probability that this source can be detected by Gaia, estimated according to interpolated Table 1 in 2019A&A...621A..86B, in percent (this is below 100 for fainter sources of close pairs).stat.likelihood;obs00.01.094.0990.04337956shortgedr3mock.maglim_5 This table gives empirical magnitude limits for G and BP bands derived from Gaia DR2 with G < 20.7 mag for HEALPixels of 5 (scale roughly ~2 degrees). For each band we have 4 different variants: (1) no additional condition, (2) parallax available, (3) BP-RP available, (4) parallax and BP-RP available. For BP mag limits we also require that BP is available. The magnitude limits are approximated by the mode of the magnitude distribution in a specific HEALpix. Since this mode estimator is prone to Poisson noise in low density areas we report the magnitude limits in two flavours: (a) directly the mode estimator (b) the same as the mode estimator, except that in healpixel with a stellar density below 1e5 sources per square degree the limit is arbitrarily set to 20.7 mag. These magnitude limits were created using the `gdr2_completeness package`_ and users are encouraged to create custom-made magnitude limits with specific conditions, e.g. RVS sample with good parallaxes. .. _gdr2_completeness package: https://github.com/jan-rybizki/gdr2_completeness12288hpxLevel 5 HEALPix for which the magnitude limit applies.pos.healpix0368.616143.511918.39122871.0intindexedmaglim_gThe mode of the G magnitude distribution in the respective HEALPixmaginstr.sensitivity18.920.320.620.620.61floatnullablestarcount_gThe number of stars in the respective HEALPix bin with G<20.7meta.number63877081.6127026.5812037.70999999930123261.0intmaglim_g_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity18.920.620.720.720.71floatnullablemaglim_g_parallaxThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity18.519.820.520.620.61floatnullablestarcount_g_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number46416537.2225895.5720948.729999999921492621.0intmaglim_g_parallax_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity18.520.320.720.720.71floatnullablemaglim_g_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity17.820.320.620.620.61floatnullablestarcount_g_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number56956897.2226570.0701180.159999999916897071.0intmaglim_g_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.820.520.720.720.71floatnullablemaglim_g_parallax_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity17.519.820.520.620.61floatnullablestarcount_g_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number42016469.6125653.0649752.779999998716032231.0intmaglim_g_parallax_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.520.220.720.720.71floatnullablemaglim_bpThe mode of the BP magnitude distribution in the respective HEALPixmaginstr.sensitivity18.220.320.720.720.71floatnullablestarcount_bpThe number of stars in the respective HEALPix bin with G<20.7meta.number56956897.2226570.5702063.439999999417186121.0intmaglim_bp_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity18.220.420.720.720.71floatnullablemaglim_bp_parallaxThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity1820.220.720.720.71floatnullablestarcount_bp_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number42016469.6125654.0649988.719999998816232291.0intmaglim_bp_parallax_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity1820.420.720.720.71floatnullablemaglim_bp_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity1820.320.720.720.71floatnullablestarcount_bp_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number56956897.2226570.0701180.159999999916897071.0intmaglim_bp_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity1820.420.720.720.71floatnullablemaglim_bp_parallax_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity1820.220.720.720.71floatnullablestarcount_bp_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number42016469.6125653.0649752.779999998716032231.0intmaglim_bp_parallax_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity1820.420.720.720.71floatnullablegedr3mock.maglim_6 This table gives empirical magnitude limits for G and BP bands derived from Gaia DR2 with G < 20.7 mag for HEALPixels of 6 (scale roughly ~1 degrees). For each band we have 4 different variants: (1) no additional condition, (2) parallax available, (3) BP-RP available, (4) parallax and BP-RP available. For BP mag limits we also require that BP is available. The magnitude limits are approximated by the mode of the magnitude distribution in a specific HEALpix. Since this mode estimator is prone to Poisson noise in low density areas we report the magnitude limits in two flavours: (a) directly the mode estimator (b) the same as the mode estimator, except that in healpixel with a stellar density below 1e5 sources per square degree the limit is arbitrarily set to 20.7 mag. These magnitude limits were created using the `gdr2_completeness package`_ and users are encouraged to create custom-made magnitude limits with specific conditions, e.g. RVS sample with good parallaxes. .. _gdr2_completeness package: https://github.com/jan-rybizki/gdr2_completeness49152hpxLevel 6 HEALPix for which the magnitude limit applies.pos.healpix01474.5324575.547676.47491511.0intindexedmaglim_gThe mode of the G magnitude distribution in the respective HEALPixmaginstr.sensitivity18.920.120.620.620.61floatnullablestarcount_gThe number of stars in the respective HEALPix bin with G<20.7meta.number15211770.06720.5204874.520000000028212691.0intmaglim_g_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity18.920.620.720.720.71floatnullablemaglim_g_parallaxThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity17.619.720.420.620.61floatnullablestarcount_g_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number10621632.06458.5180328.760000000245892111.0intmaglim_g_parallax_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.620.320.720.720.71floatnullablemaglim_g_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity16.92020.520.620.61floatnullablestarcount_g_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number6041723.06611.5176661.474522101.0intmaglim_g_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity16.920.520.720.720.71floatnullablemaglim_g_parallax_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity16.619.720.420.620.61floatnullablestarcount_g_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number5071612.06391.0162698.930000000024258961.0intmaglim_g_parallax_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity16.620.320.720.720.71floatnullablemaglim_bpThe mode of the BP magnitude distribution in the respective HEALPixmaginstr.sensitivity17.920.220.720.720.71floatnullablestarcount_bpThe number of stars in the respective HEALPix bin with G<20.7meta.number6041723.06611.5176742.824616601.0intmaglim_bp_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.920.420.720.720.71floatnullablemaglim_bp_parallaxThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity17.820.120.720.720.71floatnullablestarcount_bp_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number5071613.06391.5162776.354322961.0intmaglim_bp_parallax_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.820.420.720.720.71floatnullablemaglim_bp_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity17.920.220.720.720.71floatnullablestarcount_bp_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number6041723.06611.5176661.474522101.0intmaglim_bp_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.920.420.720.720.71floatnullablemaglim_bp_parallax_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity17.820.120.720.720.71floatnullablestarcount_bp_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number5071612.06391.0162698.930000000024258961.0intmaglim_bp_parallax_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.820.420.720.720.71floatnullablegedr3mock.maglim_7 This table gives empirical magnitude limits for G and BP bands derived from Gaia DR2 with G < 20.7 mag for HEALPixels of 7 (scale roughly ~0.5 degrees). For each band we have 4 different variants: (1) no additional condition, (2) parallax available, (3) BP-RP available, (4) parallax and BP-RP available. For BP mag limits we also require that BP is available. The magnitude limits are approximated by the mode of the magnitude distribution in a specific HEALpix. Since this mode estimator is prone to Poisson noise in low density areas we report the magnitude limits in two flavours: (a) directly the mode estimator (b) the same as the mode estimator, except that in healpixel with a stellar density below 1e5 sources per square degree the limit is arbitrarily set to 20.7 mag. These magnitude limits were created using the `gdr2_completeness package`_ and users are encouraged to create custom-made magnitude limits with specific conditions, e.g. RVS sample with good parallaxes. .. _gdr2_completeness package: https://github.com/jan-rybizki/gdr2_completeness196608hpxLevel 7 HEALPix for which the magnitude limit applies.pos.healpix05898.2198303.5190708.791966071.0intindexedmaglim_gThe mode of the G magnitude distribution in the respective HEALPixmaginstr.sensitivity16.819.720.520.620.71floatnullablestarcount_gThe number of stars in the respective HEALPix bin with G<20.7meta.number240440.01678.551103.790000000012382671.0intmaglim_g_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.720.620.720.720.71floatnullablemaglim_g_parallaxThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity15.119.420.420.620.71floatnullablestarcount_g_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number194405.01612.045006.790000000011720271.0intmaglim_g_parallax_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity16.620.320.720.720.71floatnullablemaglim_g_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity16.519.720.520.620.71floatnullablestarcount_g_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number59428.01651.044354.3700000000241213431.0intmaglim_g_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity16.520.520.720.720.71floatnullablemaglim_g_parallax_colorThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity15.119.320.320.620.71floatnullablestarcount_g_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number54400.01596.040766.5800000000161145341.0intmaglim_g_parallax_color_density_thresholdThe mode of the G magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity16.520.320.720.720.71floatnullablemaglim_bpThe mode of the BP magnitude distribution in the respective HEALPixmaginstr.sensitivity17.42020.720.720.71floatnullablestarcount_bpThe number of stars in the respective HEALPix bin with G<20.7meta.number59428.01651.044379.5800000000161248461.0intmaglim_bp_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.420.420.720.720.71floatnullablemaglim_bp_parallaxThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurementmaginstr.sensitivity16.519.920.620.720.71floatnullablestarcount_bp_parallaxThe number of stars in the respective HEALPix bin with G<20.7 and parallax measurementmeta.number54400.01596.040792.160000000031170901.0intmaglim_bp_parallax_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.320.420.720.720.71floatnullablemaglim_bp_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurementmaginstr.sensitivity17.42020.720.720.71floatnullablestarcount_bp_colorThe number of stars in the respective HEALPix bin with G<20.7 and BP and RP measurementmeta.number59428.01651.044354.3700000000241213431.0intmaglim_bp_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.420.420.720.720.71floatnullablemaglim_bp_parallax_colorThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurementmaginstr.sensitivity16.519.920.620.720.71floatnullablestarcount_bp_parallax_colorThe number of stars in the respective HEALPix bin with G<20.7 and parallax and BP and RP measurementmeta.number54400.01596.040766.5800000000161145341.0intmaglim_bp_parallax_color_density_thresholdThe mode of the BP magnitude distribution in the respective HEALPix when also requiring a parallax and BP and RP measurement. In HEALPixes with less than 1e5 stars per square degree the limit is set to 20.7 mag. This should reduce the noise of the mode estimator due to Poisson noise in low density areas.maginstr.sensitivity17.320.420.720.720.71floatnullablegedr3mock.mainA synthetic Milky Way catalog mimicking Gaia EDR3 in stellar content and data model.source_idHealpix number using Nside = 4096 with the nested scheme on equatorial coordinates times 2^35. The last digits of the source_id are reserved for a running number that serves as a unique identifier per HEALPix cell. This is formed in accordance with Gaia's source_id definition, but of course mock objects have no relation to any Gaia objects that may have an identical source_id.meta.id;meta.main31610959298575.0547592736530234e+174.253777047802872e+186.68145365260706e+1869175284091657912321.0longraBarycentric Right Ascension in ICRS at ref_epochdegpos.eq.ra;meta.maindoubleindexednullabledecBarycentric Declination in ICRS at ref_epochdegpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullablepmraProper motion in right ascension of the source in ICRS at ref_epoch. This is the projection of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatnullablepmdecProper motion in declination at ref_epoch.mas/yrpos.pm;pos.eq.decfloatnullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch ref_epoch. If looking for a distance, consider joining with gdr2dist.main and using the distances from there.maspos.parallaxfloatindexednullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale.magphot.mag;em.opt;stat.meanfloatindexednullablephot_g_mean_fluxG-band mean flux as electrons per second.s**-1phot.flux;em.opt;stat.meandoublenullablephot_g_mean_flux_errorError on phot_g_mean_fluxs**-1stat.error;phot.flux;em.opt;stat.meanfloatnullablephot_rp_mean_fluxMean flux in the integrated RP band.s**-1phot.flux;em.opt.Rdoublenullablephot_rp_mean_flux_errorError in the mean flux in the integrated RP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Rfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Rfloatindexednullablephot_bp_mean_fluxMean flux in the integrated BP band.s**-1phot.flux;em.opt.Bdoublenullablephot_bp_mean_flux_errorError in the mean flux in the integrated BP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Bfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Bfloatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. The radial velocity provided is the median value of the radial velocity measurements at all epochs. Warning: in the vicinity of bright stars, DR2 RVs can be grossly wrong. See arXiv:1901.10460 for details.km/sspect.dopplerVelocfloatnullableradial_velocity_errorThe radial velocity error is the error on the median to which a constant noise floor of 0.11 km/s has been added in quadrature to take into account the calibration contribution.km/sstat.error;spect.dopplerVelocfloatnullableastrometric_gof_alGoodness-of-fit statistic of the astrometric solution for the source in the along-scan direction (you probably want to use RUWE instead of this).stat.fit.goodnessfloatnullableastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.codeshortnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.codelongindexedlGalactic longitude (converted from ra, dec)degpos.galactic.londoublenullablebGalactic latitude (converted from ra, dec)degpos.galactic.latdoublenullablephot_g_n_obsNumber of observations contributing to G photometrymeta.numbershortnullablephot_variable_flagPhotometric variability flagmeta.code;src.varcharnullablephot_rp_n_obsNumber of observations (CCD transits) that contributed to the integrated RP mean flux and mean flux error.meta.number;obs;phot.mag;em.opt.Rshortphot_bp_n_obsNumber of observations (CCD transits) that contributed to the integrated BP mean flux and mean flux error.meta.number;obs;phot.mag;em.opt.Bshortbp_rpBP-RP colormagphot.color;em.opt.B;em.opt.Rfloatnullablebp_gBP-G colormagphot.color;em.opt.B;em.opt.Vfloatnullableg_rpG-RP colormagphot.color;em.opt.V;em.opt.Rfloatnullablephot_rvs_mean_mag[GeDR3mock only] apparent magnitude of the RVS band.magphot.color;em.opt.Ifloatnullablephot_g_mean_mag_error[GeDR3mock only] G mag error approximated by the symmetrised flux error.magphot.color;em.opt.Vfloatnullablephot_bp_mean_mag_error[GeDR3mock only] BP mag error (generated by scaling the G mag error with an empirical factor of 19.854 derived from GDR2).magphot.color;em.opt.Bfloatnullablephot_rp_mean_mag_error[GeDR3mock only] RP mag error (generated by scaling the G mag error with an empirical factor of 9.1205 derived from GDR2).magphot.color;em.opt.Rfloatnullablephot_rvs_mean_mag_error[GeDR3mock only] RVS mag error (generated by scaling the G mag error with with 30; this is essentially a wild guess which is probably too low if RVS magnitudes are provided at all).magphot.color;em.opt.Rfloatnullablerv_nb_transits[NULL] Number of transits (epochs) used to compute radial velocity.meta.number;obs;spect.dopplerVelocshortref_epoch[NULL] Reference epoch to which the astrometic source parameters are referred, expressed as a Julian Year in TCB.yrmeta.ref;time.epochdoublenullableastrometric_delta_q[NULL] Hipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)stat.valuefloatnullableastrometric_excess_noise[NULL] Excess noise of the sourcemasstat.valuefloatnullableastrometric_excess_noise_sig[NULL] Significance of excess noisestat.valuefloatnullableastrometric_n_obs_ac[NULL ]Total number of observations ACmeta.numbershortastrometric_n_obs_al[NULL] Total number of observations ALmeta.numbershortastrometric_n_bad_obs_ac[NULL] Number of bad observations ACmeta.numbershortastrometric_n_bad_obs_al[NULL] Number of bad observations ALmeta.numbershortastrometric_n_good_obs_ac[NULL] Number of good observations ACmeta.numbershortastrometric_n_good_obs_al[NULL] Number of good observations ALmeta.numbershortastrometric_chi2_al[NULL] Astrometric goodness-of-fit (χ²) in the AL direction; χ² values were computed for the ‘good’ AL observations of the source, without taking into account the astrometric excess noise (if any) of the source. They do, however, take into account the attitude excess noise (if any) of each observation.stat.fit.chi2floatnullableastrometric_primary_flag[NULL] Only primary sources (for which this flag is True) contribute to the estimation of attitude, calibration, and global parameters. The estimation of source parameters is not affected by primariness.meta.codeshortastrometric_pseudo_colour[NULL] Colour of the source assumed in the final astrometric processing, given as he effective wavenumber of the photon flux distribution in the astrometric (G) band. The value given in this field was astrometrically determined in a preliminary solution, using the chromatic displacement of image centroids calibrated by means of the effective wavenumbers (ν_eff) of primary sources calculated from BP and RP magnitudes. The field is empty when no such determination was possible, in which case a default value of 1.6 1/µm was assumed.um**-1floatnullablemean_varpi_factor_al[NULL] Mean parallax factor in the AL direction, computed from all the good observations of the source processed in the astrometry. The value given in this field is typically in the range [−0.23, +0.32] (1st and 99th percentiles). A value outside this range indicates a distribution of observations that is unfavourable for the determination of the parallax, and the calculated parallax could then be more vulnerable to errors, e.g. from the calibration model, not reflected in the formal uncertainties.stat.fit.paramfloatnullablevisibility_periods_usedNumber of visibility periods used in Astrometric solution. A visibility period is a group of observations separated from other groups by a gap of at least 4 days.meta.number;obsshortastrometric_sigma5d_max[NULL] The longest principal axis in the 5-dimensional error ellipsoid. This is useful for filtering out cases where one of the five parameters, or some linear combination of several parameters, is particularly ill-determined. It is measured in mas and computed as the square root of the largest singular value of the scaled 5 × 5 covariance matrix of the astrometric parameters.masstat.error;obs;stat.maxfloatnullablematched_observations[NULL] The number of observations (detection transits) that have been matched to a given source during the last internal crossmatch revision.meta.numbershortastrometric_priors_used[NULL] Type of prior used in in the astrometric solutionshortnullableastrometric_relegation_factor[NULL] Relegation factor of the source calculated as per Eq. (118) in 2012A&A...538A..78L used for the primary selection process.arith.factorfloatnullableastrometric_weight_ac[NULL] Mean astrometric weight of the sourcemas**-2stat.weight;stat.meanfloatnullableastrometric_weight_al[NULL] Mean astrometric weight of the sourcemas**-2stat.weight;stat.meanfloatnullableduplicated_source[NULL] During data processing, this source happened to have been duplicated and one source only has been kept.shortd11y[GeDR3mock only] Probability that this source can be detected by Gaia, estimated according to interpolated Table 1 in 2019A&A...621A..86B, in percent (this is below 100 for fainter sources of close pairs).stat.likelihood;obs00.01.094.0990.04337956shortra_dec_corr[NULL] Correlation between right ascension and declinationstat.correlationfloatnullablera_pmra_corr[NULL] Correlation between right ascension and proper motion in right ascensionstat.correlationfloatnullablera_pmdec_corr[NULL] Correlation between right ascension and proper motion in declinationstat.correlationfloatnullabledec_pmra_corr[NULL] Correlation between declination and proper motion in right ascensionstat.correlationfloatnullabledec_pmdec_corr[NULL] Correlation between declination and proper motion in declinationstat.correlationfloatnullablepmra_pmdec_corr[NULL] Correlation between proper motion in right ascension and proper motion in declinationstat.correlationfloatnullablera_parallax_corr[NULL] Correlation between right ascension and parallaxstat.correlationfloatnullabledec_parallax_corr[NULL] Correlation between declination and parallaxstat.correlationfloatnullableparallax_pmra_corr[NULL] Correlation between parallax and proper motion in right ascensionstat.correlationfloatnullableparallax_pmdec_corr[NULL] Correlation between parallax and proper motion in declinationstat.correlationfloatnullablescan_direction_mean_k1[NULL] Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k1[NULL] Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k2[NULL] Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k2[NULL] Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k3[NULL] Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k3[NULL] Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k4[NULL] Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k4[NULL] Degree of concentration of scan directions across the sourcefloatnullablepriam_flags[NULL] Flags describing the status of the astrophysical parameters Teff, A G and E[BP-RP] (i.e., those determined by Apsis-Priam). See the release documentation.meta.codelongnullableflame_flags[NULL] Flags describing the status of the astrophysical parameters radius and luminosity (i.e., those determined by Apsis-FLAME). See the release documentation.meta.codelongnullableteff_valEffective temperature of the starKphys.temperaturefloatnullableteff_percentile_lower[Null] Lower uncertainty bound of the effective temperature estimate from Apsis-Priam. This is the 16th percentile of its PDF.Kphys.temperature;stat.minfloatnullableteff_percentile_upper[Null] Upper uncertainty bound of the effective temperature estimate from Apsis-Priam. This is the 84th percentile of its PDF.Kphys.temperature;stat.maxfloatnullablea_g_valLine-of-sight extinction in the G band, A_Gmagphys.absorptionfloatnullablea_g_percentile_lower[Null] Lower uncertainty bound of the line-of-sight extinction in the G-band estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablea_g_percentile_upper[Null] Upper uncertainty bound of the line-of-sight extinction in the G-band estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullablea_bp_valEstimate of the line-of-sight extinction in the BP-band from Apsis-Priammagphys.absorptionfloatnullablea_bp_percentile_lower[Null] Lower uncertainty bound of the line-of-sight extinction in the BP-band estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablea_bp_percentile_upper[Null] Upper uncertainty bound of the line-of-sight extinction in the BP-band estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullablea_rp_valEstimate of the line-of-sight extinction in the RP-band from Apsis-Priammagphys.absorptionfloatnullablea_rp_percentile_lower[Null] Lower uncertainty bound of the line-of-sight extinction in the RP-band estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablea_rp_percentile_upper[Null] Upper uncertainty bound of the line-of-sight extinction in the RP-band estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullablea_rvs_valEstimate of the line-of-sight extinction in the RVS-band from Apsis-Priammagphys.absorptionfloatnullablea_rvs_percentile_lower[Null] Lower uncertainty bound of the line-of-sight extinction in the RVS-band estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablea_rvs_percentile_upper[Null] Upper uncertainty bound of the line-of-sight extinction in the RVS-band estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullablee_bp_min_rp_valLine-of-sight reddening E(BP-RP)magphys.absorptionfloatnullablee_bp_min_rp_percentile_lower[Null] Lower uncertainty bound of the line-of-sight reddening E(BP-RP) estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablee_bp_min_rp_percentile_upper[Null] Upper uncertainty bound of the line-of-sight reddening E(BP-RP) estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullableradius_valStellar radius in solar radiisolRadphys.size.radiusfloatnullableradius_percentile_lower[Null] Lower uncertainty bound of the radius estimate from Apsis-FLAME. This is the 16th percentile of its PDF.solRadphys.size.radius;stat.minfloatnullableradius_percentile_upper[Null] Upper uncertainty bound of the radius estimate from Apsis-FLAME. This is the 84th percentile of its PDF.solRadphys.size.radius;stat.maxfloatnullablelum_valStellar luminosity in solar luminosities.solLumphys.luminosityfloatnullablelum_percentile_lower[Null] Lower uncertainty bound of the luminosity estimate from Apsis-FLAME. This is the 16th percentile of its PDF.solLumphys.luminosity;stat.minfloatnullablelum_percentile_upper[Null] Upper uncertainty bound of the luminosity estimate from Apsis-FLAME. This is the 84th percentile of its PDF.solLumphys.luminosity;stat.maxfloatnullablefeh[GeDR3mock only] Fe/H as log10 of solar ratio ('dex')phys.abund.Fefloatnullablea0[GeDR3mock only] Monochromatic extinction at lambda = 547.7nmmagphys.absorptionfloatnullableinitial_mass[GeDR3mock only] Initial mass of the starsolMassphys.massfloatnullablecurrent_mass[GeDR3mock only] Current mass of the starsolMassphys.massfloatnullableage[GeDR3mock only] Age of the starGyrtime.agefloatnullablelogg[GeDR3mock only] Logarithm of surface gravity.log(cm/(s**2))phys.gravityfloatnullablepopid[GeDR3mock only] Population ID according to the Besancon model. 10=SMC/LMC, 11=stellar clusterssrc.classshortpm_total[GeDR3mock only] Total proper motion of the star, i.e., sqrt(pmra^2+pmdec^2).mas/yrpos.pmfloatnullableindex_parsec[GeDR3mock only] Foreign key into the photometry/extinction table.meta.id.crossintindexedgedr3mock.parsec_propsindex_parsecindex_parsecgedr3mock.parsec_props This table is intended to augment the Gaia photometry of GeDR3 Mock stars with other bands and extinctions (Sloan, Johnson and 2MASS). The grid was generated by binning all isochrones in logg, teff, and feh and taking the median values of all isochrone models that fall within one bin. We also report the median values of some astrophysical parameters so that one can check how far the actual star abundances deviate from the bin's median. For the extinction we report the extinction for the specific isochrone bin in a specific photometric band for 6 different values of monochromatic extinction, A_0, i.e. 1,2,3,5,10,20 mag. Sometimes stars in GeDR3 Mock depart from the isochrone grid, because, e.g., the feh value is outside of the grid or values have been interpolated by Galaxia in the catalog generation from the Parsec isochrones. Then the index_parsec is assigned to the nearest neighbour in log_lum and log_teff.243238index_parsecThe primary key of the photometry table, useful for joining with index_parsec in gedr3mock.main. This has the format LLLTTTFFF indexing bins in log_lum, log_teff, feh in the parsec isochrones. To find the actual bin centers, see the log_lum, log_teff, and meh_ini columns.meta.ref718101741198004.11168186021.5216229917.12242630191.0intindexedmeh_iniLog of initial model metalicity at the center of this bin.phys.abund.z-1.49213-1.45-0.5750.2750.336311floatnullablelog_ageMedian log of model star age at the parsec bin.log(yr)time.age6.66.648.099.9500310.121floatnullablem_iniMedian of the initial (zero age) mass of all model stars in the parsec bin.solMassphys.mass0.090.468143.8497246.349267.57211floatnullablem_actMedian of the current (at log_age) mass of all model star in the parsec bin.solMassphys.mass0.090.4682.70436.616363.6881floatnullablelog_lumMedian Log of luminosity of all model stars in the parsec bin.log(solLum)phys.luminosity-4.603-2.9263.4195.8386.241floatnullablelog_teffMedian Log of the effective temperature of all model stars in the parsec bin.log(K)phys.temperature.effective2.44843.480614.06925.29155.68431floatnullablelog_gravMedian Log of the surface gravity of all model stars in the parsec bin.log(m/s**2)phys.gravity-4.932-0.2263.5238.3398.5361floatnullablegaia_gMedian absolute magnitude in the Gaia G band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.V-10.962-9.184-1.42112.691916.54051floatnullablegaia_bpbrMedian absolute magnitude in the Gaia BP band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.B-10.882-9.062-1.18313.311918.3031floatnullablegaia_bpftMedian absolute magnitude in the Gaia BP band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.B-10.877-9.061-1.1862513.322418.3241floatnullablegaia_rpMedian absolute magnitude in the Gaia RP band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.R-11.421-9.434-1.64712.32615.661floatnullablegaia_rvsMedian absolute magnitude in the Gaia RVS band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.R-11.655-9.598-1.72312.23915.3271floatnullableubv_uMedian absolute magnitude in the Johnson U band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.U-10.793-9.177-1.03614.33322.6561floatnullableubv_bMedian absolute magnitude in the Johnson B band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.B-10.792-8.91394-0.81313.935919.97751floatnullableubv_vMedian absolute magnitude in the Johnson V band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.V-10.894-9.074-1.1492513.223518.1361floatnullableubv_rMedian absolute magnitude in the Johnson R band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.R-11.116-9.25-1.39612.713916.28851floatnullableubv_iMedian absolute magnitude in the Johnson I band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.I-11.492-9.4565-1.65612.29915.531floatnullableubv_jMedian absolute magnitude in the Johnson J band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.J-12.038-9.84-1.6627512.303914.7621floatnullableubv_hMedian absolute magnitude in the Johnson H band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.H-12.436-10.152-1.71812.26714.1981floatnullableubv_kMedian absolute magnitude in the Johnson K band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.K-12.507-10.2255-1.69412.293914.0481floatnullableubv_lMedian absolute magnitude in the Johnson L band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.3-4um-12.571-10.404-1.66912.45613.9311floatnullableubv_mMedian absolute magnitude in the Johnson M band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.4-8um-12.597-10.457-1.65711.16313.9451floatnullablesloan_uMedian absolute magnitude in the SDSS u band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.U-9.905-8.32-0.23115.155923.6951floatnullablesloan_gMedian absolute magnitude in the SDSS g band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.V-10.942-9.073-1.0813.57819.0831floatnullablesloan_rMedian absolute magnitude in the SDSS r band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.R-10.903-9.087-1.187513.06217.3681floatnullablesloan_iMedian absolute magnitude in the SDSS i band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.I-11.033-9.044-1.22712.729416.0631floatnullablesloan_zMedian absolute magnitude in the SDSS z band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.opt.I-11.131-9.06695-1.1667512.75915.831floatnullabletmass_jMedian absolute magnitude in the 2MASS J band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.J-12.089-9.8905-1.711512.246514.7111floatnullabletmass_hMedian absolute magnitude in the 2MASS H band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.H-12.463-10.179-1.7402512.244514.1691floatnullabletmass_ksMedian absolute magnitude in the 2MASS K' band (note that no extinction is applied) in the respective isochrone bin.magphot.mag;em.ir.K-12.535-10.26-1.725512.261414.0231floatnullablea0_1_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.V0.5450.6550.9721.0331.0441floatnullablea0_1_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.B0.9060.9581.1431.2021.211floatnullablea0_1_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.B0.8980.9541.15851.2221.231floatnullablea0_1_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.R0.510.58050.6620.6740.6751floatnullablea0_1_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.R0.5170.5210.5230.5230.5251floatnullablea0_1_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.U1.5271.5371.571.5911.5991floatnullablea0_1_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.V1.1311.161.2341.24451.2511floatnullablea0_1_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.R0.8450.8560.8770.8790.9191floatnullablea0_1_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.I0.6430.6660.6870.6890.6911floatnullablea0_1_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.I0.45950.4830.4940.4970.4981floatnullablea0_1_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.J0.2820.2870.2920.2920.2931floatnullablea0_1_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.H0.1780.1820.1830.1840.1841floatnullablea0_1_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.K0.1160.11750.1180.1180.121floatnullablea0_1_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.U1.4991.511.5491.5841.5941floatnullablea0_1_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.B1.1881.2381.3271.3371.3461floatnullablea0_1_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.V0.9590.981.01751.0221.0231floatnullablea0_1_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.R0.6660.75850.82750.8330.9011floatnullablea0_1_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.opt.I0.56950.5870.6070.610.6161floatnullablea0_1_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um0.2820.2870.2930.2940.2951floatnullablea0_1_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.H0.1780.1820.1840.1850.1851floatnullablea0_1_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.K0.1130.1140.1150.1150.1171floatnullablea0_1_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 1 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.0330.0330.0330.0690.0691floatnullablea0_2_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.V1.081.2881.881.9952.0181floatnullablea0_2_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.B1.8021.8982.2462.3562.3721floatnullablea0_2_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.B1.7871.892.2742.3942.4111floatnullablea0_2_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.R1.0121.1491.3091.33351.3371floatnullablea0_2_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.R1.0341.0421.0451.0461.051floatnullablea0_2_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.U3.0493.0683.1333.1763.1911floatnullablea0_2_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.V2.2552.3122.4562.4762.491floatnullablea0_2_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.R1.6881.711.7511.7561.8361floatnullablea0_2_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.I1.2831.3291.3711.3751.3791floatnullablea0_2_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.I0.9170.9630.9860.99250.99351floatnullablea0_2_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.J0.5650.5740.5830.5840.5851floatnullablea0_2_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.H0.3560.3630.3660.3670.3681floatnullablea0_2_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.K0.2330.2350.2360.2360.241floatnullablea0_2_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.U2.993.0153.0883.1583.1771floatnullablea0_2_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.B2.3682.4672.6462.6652.6811floatnullablea0_2_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.V1.9151.9542.0292.0382.03951floatnullablea0_2_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.R1.3251.5071.6471.6591.7981floatnullablea0_2_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.opt.I1.1361.1691.211.2161.2281floatnullablea0_2_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um0.5640.5740.5860.5870.5891floatnullablea0_2_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.H0.3560.3640.3680.3690.3691floatnullablea0_2_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.K0.2260.2280.2290.230.2341floatnullablea0_2_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 2 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.0660.0660.0670.1380.1381floatnullablea0_3_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.V1.5981.88552.6762.8342.8641floatnullablea0_3_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.B2.6842.8113.283.4253.4491floatnullablea0_3_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.B2.6622.7973.3143.4733.4981floatnullablea0_3_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.R1.5031.6961.9281.9651.9691floatnullablea0_3_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.R1.551.5631.56751.5681.5741floatnullablea0_3_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.U4.5634.594.6844.7484.7711floatnullablea0_3_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.V3.373.453.6543.6843.7071floatnullablea0_3_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.R2.5272.5592.6192.6272.7511floatnullablea0_3_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.I1.9191.9862.0492.0552.0611floatnullablea0_3_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.I1.371.4391.4731.4831.4851floatnullablea0_3_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.J0.8460.8590.87250.8740.8761floatnullablea0_3_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.H0.5340.5440.5490.550.5511floatnullablea0_3_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.K0.3490.3520.3540.3540.361floatnullablea0_3_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.U4.4714.5094.6134.7144.7411floatnullablea0_3_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.B3.5353.6773.9443.9743.9861floatnullablea0_3_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.V2.862.91653.0283.0413.0441floatnullablea0_3_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.R1.9722.2342.4492.4682.6821floatnullablea0_3_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.opt.I1.6961.7441.8051.8141.8331floatnullablea0_3_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um0.8450.860.8770.8790.8821floatnullablea0_3_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.H0.5340.5450.5510.5530.5531floatnullablea0_3_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.K0.33950.3420.3440.3450.3511floatnullablea0_3_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 3 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.0990.0990.10.2070.2071floatnullablea0_5_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.V2.6353.0794.2694.5124.5581floatnullablea0_5_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.B4.4474.6375.355.5645.6011floatnullablea0_5_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.B4.4124.6115.3945.6315.6711floatnullablea0_5_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.R2.4832.793.16553.2283.2351floatnullablea0_5_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.R2.5842.6052.6122.6142.6231floatnullablea0_5_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.U7.597.63357.78757.8927.931floatnullablea0_5_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.V5.5995.7256.05056.09956.1441floatnullablea0_5_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.R4.2044.2574.3564.3694.581floatnullablea0_5_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.I3.193.3023.40553.4153.4261floatnullablea0_5_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.I2.2762.3922.4482.4652.4671floatnullablea0_5_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.J1.4081.431.4521.4551.4591floatnullablea0_5_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.H0.8890.9060.91450.91650.9171floatnullablea0_5_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.K0.5820.5870.5890.590.61floatnullablea0_5_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.U7.4327.4987.6627.8257.871floatnullablea0_5_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.B5.8686.0986.546.5926.6031floatnullablea0_5_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.V4.7474.8415.0275.0485.0531floatnullablea0_5_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.R3.2653.6894.0544.0854.451floatnullablea0_5_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.opt.I2.8152.8932.9943.013.0431floatnullablea0_5_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um1.4061.431.4591.4621.4671floatnullablea0_5_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.H0.890.9080.9180.920.9211floatnullablea0_5_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.K0.5660.570.5730.5740.5841floatnullablea0_5_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 5 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.1650.1660.1660.3450.3451floatnullablea0_10_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.V5.1015.817.5177.8788.1891floatnullablea0_10_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.B8.7579.03810.07110.35610.4111floatnullablea0_10_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.B8.6938.9810.09710.41310.4731floatnullablea0_10_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.R4.8355.35255.9946.1156.12751floatnullablea0_10_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.R5.1665.2085.2225.2245.2441floatnullablea0_10_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.U15.09115.16615.44815.64115.7131floatnullablea0_10_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.V11.08611.29311.83611.92312.0791floatnullablea0_10_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.R8.3638.4598.6458.679.1171floatnullablea0_10_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.I6.3246.53856.7386.7556.77651floatnullablea0_10_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.I4.4974.7274.84154.8754.8791floatnullablea0_10_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.J2.8042.8472.892.8952.9031floatnullablea0_10_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.H1.7761.8081.82451.8281.82951floatnullablea0_10_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.K1.1621.1731.17751.1791.1981floatnullablea0_10_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.U14.75214.89615.16915.45215.5321floatnullablea0_10_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.B11.56711.9712.80512.9112.9351floatnullablea0_10_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.V9.3499.5359.89859.9429.9521floatnullablea0_10_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.R6.3867.1287.8687.9378.6791floatnullablea0_10_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.opt.I5.5545.6965.8885.925.9921floatnullablea0_10_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um2.7972.8442.89852.9052.9121floatnullablea0_10_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.H1.7761.811.831.8341.8361floatnullablea0_10_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.K1.131.1371.1441.1461.1651floatnullablea0_10_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 10 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.330.3320.3330.6890.691floatnullablea0_20_gaia_gMedian extinction in the Gaia G band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.V9.73310.75212.838513.313.7491floatnullablea0_20_gaia_bpbrMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.B17.18317.54518.842519.16319.2281floatnullablea0_20_gaia_bpftMedian extinction in the Gaia BP band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.B17.07117.43618.81119.16219.2331floatnullablea0_20_gaia_rpMedian extinction in the Gaia RP band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.R9.29410.08310.99611.19211.2111floatnullablea0_20_gaia_rvsMedian extinction in the Gaia RVS band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.R10.32510.40710.43510.43810.4781floatnullablea0_20_sloan_uMedian extinction in the SDSS u band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.U29.9530.05730.51430.83730.9541floatnullablea0_20_sloan_gMedian extinction in the SDSS g band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.V21.82422.12722.90923.03823.3731floatnullablea0_20_sloan_rMedian extinction in the SDSS r band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.R16.58616.73717.05617.10218.011floatnullablea0_20_sloan_iMedian extinction in the SDSS i band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.I12.45412.84313.19313.22413.25651floatnullablea0_20_sloan_zMedian extinction in the SDSS z band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.I8.7929.2289.4639.5279.5341floatnullablea0_20_tmass_jMedian extinction in the 2MASS J band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.J5.5615.6435.7255.7345.7531floatnullablea0_20_tmass_hMedian extinction in the 2MASS H band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.H3.5373.5983.6313.6383.641floatnullablea0_20_tmass_ksMedian extinction in the 2MASS Ks band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.K2.3192.3412.352.35152.3911floatnullablea0_20_ubv_uMedian extinction in the Johnson U band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.U29.20429.527529.93430.36530.4851floatnullablea0_20_ubv_bMedian extinction in the Johnson B band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.B22.55123.16924.524.68424.7811floatnullablea0_20_ubv_vMedian extinction in the Johnson V band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.V18.19318.54619.208519.2919.311floatnullablea0_20_ubv_rMedian extinction in the Johnson R band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.R12.27713.408514.70214.84316.0221floatnullablea0_20_ubv_iMedian extinction in the Johnson I band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.opt.I10.8611.09111.42611.48511.6251floatnullablea0_20_ubv_jMedian extinction in the Johnson L band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.3-4um5.5375.62455.7275.7385.7521floatnullablea0_20_ubv_hMedian extinction in the Johnson H band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.H3.5353.5993.63853.6463.6491floatnullablea0_20_ubv_kMedian extinction in the Johnson K band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.K2.2532.2662.2782.2842.3221floatnullablea0_20_ubv_mMedian extinction in the Johnson M band for monochromatic extinction (A_0) of 20 mag for the respective isochrone binmagphys.absorption;em.ir.4-8um0.6610.6640.6651.3791.3791floatnullablegedr3spur This table contains estimates of the "fidelity" of Gaia eDR3 astrometric solutions, a measure of the likelihood the eDR3 solution is physical rather than spurious obtained using a neural network trained on a small, hand-selected sample.gedr3spur.main This table contains estimates of the "fidelity" of Gaia eDR3 astrometric solutions, a measure of the likelihood the eDR3 solution is physical rather than spurious obtained using a neural network trained on a small, hand-selected sample.1500000000source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongindexedprimaryfidelity_v2A probability that eDR3 has a good astrometric solution for this source, with values between 0 (meaning likely spurious solution) and 1 (meaning likely good solution). This is the published probability estimate.stat.fitfloatindexednullabletheta_arcsec_worst_sourceDistance to the eDR3 source within 30 arcsec of the object for which ΔG-θ is maximal. See norm_dg for details.arcsecpos.angDistancefloatnullablenorm_dgThis is a heuristic measure for contamination by bright stars in the neighbourhood. It is computed as ΔG-θ, where θ is the distance to another Gaia eDR3 object in arcsec (reported in theta_arcsec_worst_source), and ΔG is the magnitude difference in mag. This column gives the maximum of the values for all eDR3 sources within 30 arcsecs of the object.instr.backgroundfloatnullabledist_nearest_neighbor_at_least_m2_brighterDistance to the nearest neighbour in gaia_source at least 2 m fainter than this source.arcsecpos.angDistancefloatnullabledist_nearest_neighbor_at_least_0_brighterDistance to the nearest neighbour in gaia_source at least as bright as this source.arcsecpos.angDistancefloatnullabledist_nearest_neighbor_at_least_2_brighterDistance to the nearest neighbour in gaia_source at least 2 m brighter than this source.arcsecpos.angDistancefloatnullabledist_nearest_neighbor_at_least_4_brighterDistance to the nearest neighbour in gaia_source at least 4 m brighter than this source.arcsecpos.angDistancefloatnullabledist_nearest_neighbor_at_least_6_brighterDistance to the nearest neighbour in gaia_source at least 6 m brighter than this source.arcsecpos.angDistancefloatnullabledist_nearest_neighbor_at_least_10_brighterDistance to the nearest neighbour in gaia_source at least 10 m brighter than this source.arcsecpos.angDistancefloatnullablefidelity_v1A probablity that eDR3 has a good astrometric solution for this source, with values between 0 (meaning likely spurious solution) and 1 (meaning likely good solution). This comes from a first version of the estimator that was reviewed based on an astro-ph paper.stat.fitfloatnullablelswScans of plates kept at Landessternwarte Heidelberg-Königstuhl. They were obtained at location, at the German-Spanish Astronomical Center (Calar Alto Observatory), Spain, and at La Silla, Chile. The plates cover a time span between 1880 and 1999. Specifically, HDAP is essentially complete for the plates taken with the Bruce telescope, the Walz reflector, and Wolf's Doppelastrograph at both the original location in Heidelberg and its later home on Königstuhl.lsw.plates The main catalog of the plates contained in the archive.accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoubleindexednullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableexposureEffective exposure timestime.duration;obs.exposurefloatnullableairmassAirmass at mean epochobs.airMassfloatnullableobjectSpecial object on platemeta.idcharnullableemulsionEmulsion of the original plateinstr.plate.emulsioncharnullablefilterFilter descriptionmeta.id;instr.filter;meta.maincharnullableobserverObserverobs.observercharnullablestarttimeUT at start of exposuredtime.start;obscharnullableendtimeUT at end of exposuredtime.end;obscharnullableplateidPlate name as specified in observation cataloguecharindexednullablepub_didDataset identifier assigned by the publisher.meta.ref.urlcharnullablelsw.wolfpalisa A mapping between HDAP plate identifiers and Wolf-Palisa survey plate numbers.w_p_idPlate number in the Wolf-Palisa surveymeta.idcharnullableplateidPlate name as specified in observation cataloguecharnullableplc3 From the Gaia eDR3 catalogue we predict astrometric microlensing events by foreground stars with high proper motion (μ > 100 mas/yr) passing a background source in the next decades. Using Gaia DR3 photometry we determine an approximate mass of the lens, which we use to calculate the expected microlensing effects. This yields 4842 microlensing events by 3791 different lenses between 2010 and 2066 with expected shifts larger than 0.1 mas between the lensed and unlensed positions of the source. The past events might be interested when analyzing the individual Gaia measurements). 685 of those are expected to happen within the next decade (2021-2031). For 140 events we also expect a magnification between 1 mmag and 0.6 mag.plc3.dataThe final candidate table for astrometric microlensing events predicted from Gaia eDR3. This has estimates of minimal distances, epochs, etc. Columns prefixed with lens_ are for the lens, columns prefixed with ob_ are for the lensed object.4842event_idUnique identifier of this event. This is the decimal representation of the Gaia eDR3 source_id of the lens, and a disambiguator for the lensed object.meta.id;meta.maincharindexedprimarylens_idGaia eDR3 source_id of the lens.meta.idlonglens_raGaia eDR3 RA of the lensdegpos.eq.ra;meta.maindoubleindexednullablelens_decGaia eDR3 Declination of the lensdegpos.eq.dec;meta.maindoubleindexednullablelens_err_raError of lens__ra from Gaia eDR3masstat.error;pos.eq.ra;meta.mainfloatnullablelens_err_decError of lens__dec from Gaia eDR3masstat.error;pos.eq.dec;meta.mainfloatnullablelens_pmraProper motion in RA of the lens from Gaia eDR3mas/yrpos.pm;pos.eq.rafloatnullablelens_pmdecProper motion in Declination of the lens from Gaia eDR3mas/yrpos.pm;pos.eq.rafloatnullablelens_err_pmraError of lens_pmra from Gaia eDR3deg/yrpos.pm;pos.eq.rafloatnullablelens_err_pmdecError of lens_pmdec from Gaia eDR3deg/yrpos.pm;pos.eq.decfloatnullablelens_parallaxParallax of the lens from Gaia eDR3maspos.parallaxfloatnullablelens_err_parallaxStandard error of the parallax the lens from Gaia eDR3masstat.error;pos.parallaxfloatnullablelens_phot_g_mean_magMean magnitude of the lens in the integrated G band from Gaia eDR3.magphot.mag;em.opt.Vfloatnullablelens_phot_rp_mean_magMean magnitude of the lens in the integrated RP band from Gaia eDR3.magphot.mag;em.opt.Rfloatnullablelens_phot_bp_mean_magMean magnitude of the lens in the integrated BP band from Gaia eDR3.magphot.mag;em.opt.Bfloatnullableob_idGaia eDR3 source_id of the lensed object.meta.idlongob_raGaia eDR3 RA of the lensed objectdegpos.eq.radoublenullableob_decGaia eDR3 Declination of the lensed objectdegpos.eq.decdoublenullableob_err_raError of ob__ra from Gaia eDR3masstat.error;pos.eq.rafloatnullableob_err_decError of ob__dec from Gaia eDR3masstat.error;pos.eq.decfloatnullableob_pmraProper motion in RA of the lensed object from Gaia eDR3mas/yrpos.pm;pos.eq.rafloatnullableob_pmdecProper motion in Declination of the lensed object from Gaia eDR3mas/yrpos.pm;pos.eq.rafloatnullableob_err_pmraError of ob_pmra from Gaia eDR3deg/yrpos.pm;pos.eq.rafloatnullableob_err_pmdecError of ob_pmdec from Gaia eDR3deg/yrpos.pm;pos.eq.decfloatnullableob_parallaxParallax of the lensed object from Gaia eDR3maspos.parallaxfloatnullableob_err_parallaxStandard error of the parallax the lensed object from Gaia eDR3masstat.error;pos.parallaxfloatnullableob_phot_g_mean_magMean magnitude of the lensed object in the integrated G band from Gaia eDR3.magphot.mag;em.opt.Vfloatnullableob_phot_rp_mean_magMean magnitude of the lensed object in the integrated RP band from Gaia eDR3.magphot.mag;em.opt.Rfloatnullableob_phot_bp_mean_magMean magnitude of the lensed object in the integrated BP band from Gaia eDR3.magphot.mag;em.opt.Bfloatnullableob_displacement_ra_doubledDoubled Displacement in RA between DR2 and DR3, cos(δ) applied.maspos.eq.ra;arith.difffloatnullableob_displacement_dec_doubledDoubled Displacement in Dec between DR2 and DR3maspos.eq.dec;arith.difffloatnullablestar_typeType of the lensing star: WD = White Dwarf, MS = Main Sequence, RG = Red Giant, BD = Brown Dwarfsrc.classcharnullablemassEstimated mass of the lens from Gaia eDR3solMassphys.massfloatnullableerr_massError in the mass of the lens from Gaia eDR3solMassstat.error;phys.massfloatnullabletheta_eEinstein radius of the eventmasphys.angsizedoublenullableerr_theta_eError in the Einstein radius of the eventmasstat.error;phys.angsizefloatnullablet_amlApproximate duration of the event (i.e., shift > ~0.1 mas).yrtime.durationdoublenullabletcaEstimated time of the closest approach.yrtime.epochdoublenullableerr_tcaError in tca.yrstat.error;time.epochfloatnullabledistEstimated distance at closest approach.maspos.angdistancefloatnullableerr_distError d_min.masstat.error;pos.angdistancefloatnullableuEstimated distance at closest approach in Einstein radii.pos.angdistance;stat.mindoublenullableu_error_mLeft 67% confidence interval of u.stat.error;pos.angdistance;stat.minfloatnullableu_error_pRight 67% confidence interval of u.stat.error;pos.angdistance;stat.minfloatnullableshiftMaximal astrometric shift of the center of light.maspos;arith.diffdoublenullableshift_error_mLeft 67% confidence interval of shift.masstat.error;pos;arith.difffloatnullableshift_error_pRight 67% confidence interval of shift.masstat.error;pos;arith.difffloatnullableshift_lumMaximal astrometric shift including lens-luminosity effects.maspos;arith.diffdoublenullableshift_lum_error_mLeft 67% confidence interval of shift_lum.masstat.error;pos;arith.difffloatnullableshift_lum_error_pRight 67% confidence interval of shift_lum.masstat.error;pos;arith.difffloatnullableshift_plusMaximal astrometric shift of brighter image.maspos;arith.diffdoublenullableshift_plus_error_mLeft 67% confidence interval of shift_plus.masstat.error;pos;arith.difffloatnullableshift_plus_error_pRight 67% confidence interval of shift_plus.masstat.error;pos;arith.difffloatnullablemagnificationMaximal magnification.magphot.mag;arith.ratiodoublenullablemagnification_error_mLeft 67% confidence interval of magnification.magstat.error;phot.mag;arith.ratiofloatnullablemagnification_error_pRight 67% confidence interval of magnification.magstat.error;phot.mag;arith.ratiofloatnullablel2_tcaEstimated time of the closest approachas seen from Earth-Sun L2 point.yrtime.epochdoublenullablel2_err_tcaError in l2_tca.yrstat.error;time.epochfloatnullablel2_distEstimated distance at closest approachas seen from Earth-Sun L2 point.maspos.angdistancefloatnullablel2_err_distError l2_d_min.masstat.error;pos.angdistancefloatnullablel2_uEstimated distance at closest approach in Einstein radiias seen from Earth-Sun L2 point.pos.angdistance;stat.mindoublenullablel2_u_error_mLeft 67% confidence interval of l2_u.stat.error;pos.angdistance;stat.minfloatnullablel2_u_error_pRight 67% confidence interval of l2_u.stat.error;pos.angdistance;stat.minfloatnullablel2_shiftMaximal astrometric shift of the center of lightas seen from Earth-Sun L2 point.maspos;arith.diffdoublenullablel2_shift_error_mLeft 67% confidence interval of l2_shift.masstat.error;pos;arith.difffloatnullablel2_shift_error_pRight 67% confidence interval of l2_shift.masstat.error;pos;arith.difffloatnullablel2_shift_lumMaximal astrometric shift including lens-luminosity effectsas seen from Earth-Sun L2 point.maspos;arith.diffdoublenullablel2_shift_lum_error_mLeft 67% confidence interval of l2_shift_lum.masstat.error;pos;arith.difffloatnullablel2_shift_lum_error_pRight 67% confidence interval of l2_shift_lum.masstat.error;pos;arith.difffloatnullablel2_shift_plusMaximal astrometric shift of brighter imageas seen from Earth-Sun L2 point.maspos;arith.diffdoublenullablel2_shift_plus_error_mLeft 67% confidence interval of l2_shift_plus.masstat.error;pos;arith.difffloatnullablel2_shift_plus_error_pRight 67% confidence interval of l2_shift_plus.masstat.error;pos;arith.difffloatnullablel2_magnificationMaximal magnificationas seen from Earth-Sun L2 point.magphot.mag;arith.ratiodoublenullablel2_magnification_error_mLeft 67% confidence interval of l2_magnification.magstat.error;phot.mag;arith.ratiofloatnullablel2_magnification_error_pRight 67% confidence interval of l2_magnification.magstat.error;phot.mag;arith.ratiofloatnullablet_0_1_masApproximate duration on which shift_plus changes by 0.1 mas from its maximumyrtime.durationfloatnullablet_50pcApproximate duration on which shift_plus changes by 50% from its maximumyrtime.durationfloatnullablerobott The Robotic Bochum Twin Telescope (RoBoTT) operated from December 2008 to September 2019 at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It consists of two refractor telescopes (15 cm aperture, 2°42'' × 2°42'' FoV CCDs) attached to the same mount. The fields were observed in Johnson UVBRI, Sloan ugriz, and the narrowband OIII, NB, Halpha, and SII filters. The first batch contains fields that were observed in Johnson U and Sloan z; further RoBoTT fields will be added at a later date. Bochum Galactic Disk Survey (BGDS) images, which were also taken with the RoBoTT, are available separately from ivo://org.gavo.dc/bgds/q/sia.robott.data The Robotic Bochum Twin Telescope (RoBoTT) operated from December 2008 to September 2019 at the Universitaetssternwarte Bochum near Cerro Armazones in the Chilean Atacama desert. It consists of two refractor telescopes (15 cm aperture, 2°42'' × 2°42'' FoV CCDs) attached to the same mount. The fields were observed in Johnson UVBRI, Sloan ugriz, and the narrowband OIII, NB, Halpha, and SII filters. The first batch contains fields that were observed in Johnson U and Sloan z; further RoBoTT fields will be added at a later date. Bochum Galactic Disk Survey (BGDS) images, which were also taken with the RoBoTT, are available separately from ivo://org.gavo.dc/bgds/q/sia.2741dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel0123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.sizelongnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameterfloatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.valuefloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extentfloatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.valuefloatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimitfloatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimitfloatindexednullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refvalfloatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.namecharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.namecharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBinsintnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBinsintnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBinsintnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriodfloatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullablebandpass_idFree-form name of the bandpass (filter, detector, whatever else defines the spectral response) this observation was taken in.instr.bandpasscharindexednullablefieldSurvey field observed.meta.id;obs.fieldcharindexednullableairmassAirmass at mean epochobs.airMassfloatnullablemoondistMoon distance at mean epochdegobs.paramfloatnullablerosat ROSAT was an orbiting x-ray observatory active in the 1990s. We provide a table of all photons observed during ROSAT's all-sky survey (RASS) as well as images of both survey and pointed observations. For ROSAT data products, see http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-surveyrosat.imagesMetadata for ROSAT pointed observations and the ROSAT All Sky Survey (RASS) images115678accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharindexednullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableseqnoROR sequence numbermeta.id;obsintindexedfollowupNumber of follow-up observation (0=first observation, NULL=mispointing)meta.code;obsintnullableobstypeType of data in the file (associated products available through datalink of by querying through seqno)meta.code;meta.filecharnullablepubdidPublisher dataset identifier (this lets you access datalink services and the like)meta.idcharnullabledlurlLink to a datalink document for this dataset, this lets you access associate data)meta.ref.urlcharnullablerosat.photonsA table of x-ray photons detected by ROSAT88000000raj2000Right Ascension, equinox 2000.0degpos.eq.ra;meta.maindoubleindexednullabledej2000Declination, equinox 2000.0degpos.eq.dec;meta.maindoubleindexednullabledetection_timeTime the photon was detected, in Julian years.yrtime.startdoubleindexednullableenergy_corEnergy of incoming photon (corrected) [keV]keVphys.energy;em.X-rayfloatindexednullableposition_errorTotal positional error, 1{sigma} arcsecarcsecstat.error;pos.eqfloatnullableglongGalactic longitudedegpos.galactic.lonfloatnullableglatGalactic latitudedegpos.galactic.latfloatnullablepulseht_channelChannel of the pulse height. This is a measure for the energy of the incoming photon, where one channel corresponds to about 10 eV; a pulse height channel of 127 thus indicates an incoming photon of about 1.3 keV.shortnullableexposure_timeROSAT cluster survey exposure timestime.duration;obs.exposurefloatnullablefield_idRASS field idmeta.id;obs.fieldshortnullableixX pixel coordinatepixelpos.cartesian.x;instr.detshortnullableiyY pixel coordinatepixelpos.cartesian.y;instr.detshortnullableidPhoton identifier (a combination of observation date and detector coordinates)meta.id;meta.mainlongindexedprimarytheossaTheoSSA provides spectral energy distributions based on model atmosphere calculations. Currently, we serve results obtained using the Tübingen NLTE Model Atmosphere Package (TMAP) for hot compact stars.theossa.dataTheoSSA metadata in the SSAP schema.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size633169872.28126339.01266903.8842037871.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Date52045.0021296296356675.47873842592559691.7716435185260691.70158564814560722.487523148151.0charnullablessa_pdateDate last published.ssa:Curation.Date59592.54311518637459592.54756652129460779.67676536275461060.32020536403461090.551854537361.0charnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassRadiocharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshift0floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.00010.00010.00010.00010.00013.85279e-05floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start1e-102e-101.15005e-073.0005e-075.00106e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop5.99979e-091.188e-071.78e-074e-054e-051floatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Length9127679.014723.0173663.06861961.0intnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.densitycharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unit0.1J/(m**2.s.m)charssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcetheorycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationABSOLUTEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSize-1.87824e-113.61896e-124.27868e-122.3033e-104.0127e-091floatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolution-1.87824e-113.61896e-124.27868e-122.3033e-104.0127e-091floatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablet_effEffective temperature assumedKphys.temperature.effective181003300059500940001.05e+061floatnullablelog_gLog of surface gravity assumedcm/s**2phys.gravity3.84.185.77.369.221floatnullablemdotMass loss ratesolMass/yrphys.mass.loss000001floatnullablew_hMass fraction of H in the model computed.phys.abund00.058910.5434111floatnullablew_heMass fraction of He in the model computed.phys.abund000.45420.937611floatnullablew_liMass fraction of Li in the model computed.phys.abund000000.999196floatnullablew_beMass fraction of Be in the model computed.phys.abund000000.999196floatnullablew_bMass fraction of B in the model computed.phys.abund000000.999196floatnullablew_cMass fraction of C in the model computed.phys.abund000.0023910.0035250.59011floatnullablew_nMass fraction of N in the model computed.phys.abund00000.044061floatnullablew_oMass fraction of O in the model computed.phys.abund00000.69431floatnullablew_fMass fraction of F in the model computed.phys.abund00000.00010.999472floatnullablew_neMass fraction of Ne in the model computed.phys.abund00000.16670.999512floatnullablew_naMass fraction of Na in the model computed.phys.abund00000.0099010.999379floatnullablew_mgMass fraction of Mg in the model computed.phys.abund00000.093820.999501floatnullablew_alMass fraction of Al in the model computed.phys.abund00000.0099011floatnullablew_siMass fraction of Si in the model computed.phys.abund00000.019261floatnullablew_pMass fraction of P in the model computed.phys.abund00003.172e-050.99996floatnullablew_sMass fraction of S in the model computed.phys.abund00000.0030831floatnullablew_clMass fraction of Cl in the model computed.phys.abund00004.943e-060.999196floatnullablew_arMass fraction of Ar in the model computed.phys.abund00000.00013990.999472floatnullablew_kMass fraction of K in the model computed.phys.abund00003.44e-060.999196floatnullablew_caMass fraction of Ca in the model computed.phys.abund00000.0063591floatnullablew_scMass fraction of Sc in the model computed.phys.abund00000.0045790.999367floatnullablew_tiMass fraction of Ti in the model computed.phys.abund00000.003090.999362floatnullablew_vMass fraction of V in the model computed.phys.abund00005.675e-090.999196floatnullablew_crMass fraction of Cr in the model computed.phys.abund00000.0019240.999412floatnullablew_mnMass fraction of Mn in the model computed.phys.abund00000.0019240.999383floatnullablew_feMass fraction of Fe in the model computed.phys.abund00000.012920.99996floatnullablew_coMass fraction of Co in the model computed.phys.abund00000.00087150.999415floatnullablew_niMass fraction of Ni in the model computed.phys.abund00000.007050.999859floatnullablew_znMass fraction of Zn in the model computed.phys.abund00000.000171floatnullablew_gaMass fraction of Ga in the model computed.phys.abund00000.00055970.865835floatnullablew_geMass fraction of Ge in the model computed.phys.abund00000.00023991floatnullablew_krMass fraction of Kr in the model computed.phys.abund00000.0010991floatnullablew_moMass fraction of Mo in the model computed.phys.abund00000.00018810.86563floatnullablew_tcMass fraction of Tc in the model computed.phys.abund000000.865142floatnullablew_snMass fraction of Sn in the model computed.phys.abund00000.00020361floatnullablew_xeMass fraction of Xe in the model computed.phys.abund00000.0016971floatnullablew_baMass fraction of Ba in the model computed.phys.abund00000.0014981floatnullablexpparams We present astrophysical parameters of 220 million stars, based on Gaia XP spectra and near-infrared photometry from 2MASS and WISE. Instead of using ab initio stellar models, we develop a data-driven model of Gaia XP spectra as a function of the stellar parameters, with a few straightforward built-in physical assumptions. This resource is a VO re-publication of the resulting catalog of stellar parameters. For bulk downloads, the covariances, the trained model, and more, see https://zenodo.org/record/7811871.xpparams.main We present astrophysical parameters of 220 million stars, based on Gaia XP spectra and near-infrared photometry from 2MASS and WISE. Instead of using ab initio stellar models, we develop a data-driven model of Gaia XP spectra as a function of the stellar parameters, with a few straightforward built-in physical assumptions. This resource is a VO re-publication of the resulting catalog of stellar parameters. For bulk downloads, the covariances, the trained model, and more, see https://zenodo.org/record/7811871.220000000source_idGaia DR3 unique source identifier. You can match this against gaia.dr3lite on this TAP service.meta.id;meta.main866939156652803.512553146661156e+174.2899471707395456e+186.706376482488434e+1869175099279225084161.0longindexedprimaryraGaia ICRS right ascension for this object.degpos.eq.ra;meta.main3.96484e-0628.818247.093335.3473601doubleindexednullabledecGaia ICRS declination for this object.degpos.eq.dec;meta.main-89.9887-69.8648-22.841162.735289.97711doubleindexednullableteffEstimated effective Temperature. Note that the raw HDF5 files released by Zhang et al. (2023) give Teff in a different unit (Kilokelvin).Kphys.temperature.effective-787.5943613.845460.627605.1825020.81floatindexednullablefe_hLog of Fe/H in solar unitsphys.abund.Fe-8.66649-1.6993-0.1844590.4151694.369151floatindexednullableloggLog of surface gravity in solar unitsphys.gravity-3.74191.697354.135314.6932119.73271floatindexednullableextEstimated extinction parameter. To convert to the extension at a particular wavelength, multiply this by that wavelength's value in the extinction curve, available at https://zenodo.org/record/7811871/files/extinction_curve.txt?download=1 and in the footnote.magphys.absorption2.06316e-050.02219680.2833251.5368770.36931floatnullablemod_parallaxParallax estimated from the model.maspos.parallax0.008172620.07458310.413052.17084363.5721floatnullableerr_teffError in estimated effective temperature. Note that the raw HDF5 files released by Zhang et al. (2023) give the error in Teff in a different unit (Kilokelvin).Kstat.error;phys.temperature.effective2.8363427.2088101.209487.3039967111floatnullableerr_fe_hError in fe_hstat.error;phys.abund.Fe0.004439960.03100860.1298090.656735994.1421floatnullableerr_loggError in log_gstat.error;phys.gravity0.0008341420.01827640.1241730.736772996.6661floatnullableerr_extError in extmagstat.error;phys.absorption0.001231010.008627230.02595740.0802052981.151floatnullableerr_mod_parallaxError in the parallax estimated from the model.masstat.error;pos.parallax0.0003336220.010240.04462910.111599831.0521floatnullablechi2_optχ² of the best-fit solution. Divide by 61 to obtain χ² per degree of freedom.stat.fit.chi22.7753935.687564.87511221floatnullableln_priorNatural log of the GMM prior on stellar type, at the location of the optimal solution.stat.fit.goodness-444-10.10161.573243.519533.822271floatnullableteff_confidenceA neural-network-based estimate of the confidence in the effective temperature estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.00321960.6630860.98974611floatnullablefeh_confidenceA neural-network-based estimate of the confidence in the [Fe/H] estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.04055790.6933590.98828111floatnullablelogg_confidenceA neural-network-based estimate of the confidence in the log(g) estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.09948730.6723630.97265611floatnullablequality_flagsThe three least significant bits represent whether the confidence in effective temperature, [Fe/H] and log(g) is less than 0.5, respectively. The 4th bit is set if chi2_opt/61 > 2. The 5th bit is set if ln_prior < -7.43. The 6th bit is set if our parallax estimate is more than 10 sigma from the GDR3 measurement (using reported parallax uncertainties from GDR3). The two most significant bits are always unset. We recommend a cut of quality_flags < 8 (the "basic reliability cut"), although a stricter cut of quality_flags == 0 ensures higher reliability at the cost of lower completeness.meta.code.qual00.02.031.0631.0shortxpparams2 We measure the extinction curves of 220 million stars with Gaia XP spectra and near-infrared photometry from 2MASS and WISE. We use a data-driven model that is developed from :bibcode:`2023MNRAS.524.1855Z`, with variable extinction curves, to determine stellar parameters and extinction curves simultaneously. For bulk downloads and the trained model, see https://doi.org/10.5281/zenodo.10719756.xpparams2.covs A table of covariances (as upper triangle matrices) for the stellar parameters in xpparams2.main). This is intended for use as in:: SELECT ..., cov_triu FROM xpparams2.main NATURAL JOIN xpparams2.covs WHERE ... If you only need particular elements of the covariance matrix, you can subscript cov_triu, perhaps as in ``cov_triu[4] AS teff_xi_cov``.220000000source_idGaia DR3 unique source identifier. You can match this against gaia.dr3lite on this TAP service.meta.id;meta.main217883698972163.5412776955166304e+174.288263474842695e+186.705406288540965e+1869175284134610831361.0longindexedprimarytriuUpper triangle of the covariance matrix of the stellar parameters from xpparams2.main. The variables are, in sequence: T_eff, [Fe/H], logg, ξ, E, and parallax.stat.covariancefloatnullablexpparams2.main We measure the extinction curves of 220 million stars with Gaia XP spectra and near-infrared photometry from 2MASS and WISE. We use a data-driven model that is developed from :bibcode:`2023MNRAS.524.1855Z`, with variable extinction curves, to determine stellar parameters and extinction curves simultaneously. For bulk downloads and the trained model, see https://doi.org/10.5281/zenodo.10719756.220000000source_idGaia DR3 unique source identifier. You can match this against gaia.dr3lite on this TAP service.meta.id;meta.main217883698972163.5412776955166304e+174.288263474842695e+186.705406288540965e+1869175284134610831361.0longindexedprimaryraGaia ICRS right ascension for this object.degpos.eq.ra;meta.main3.1103e-0528.4603247.083335.1873601doubleindexednullabledecGaia ICRS declination for this object.degpos.eq.dec;meta.main-89.9304-69.8549-22.78162.824389.95331doubleindexednullableteffEstimated effective Temperature. Note that the raw HDF5 files released by Zhang et al. (2023) give Teff in a different unit (Kilokelvin).Kphys.temperature.effective-2520.023736.115448.117427.79299221floatindexednullablefe_hLog of Fe/H in solar unitsphys.abund.Fe-10.7803-1.89521-0.184080.3740569.560591floatindexednullableloggLog of surface gravity in solar unitsphys.gravity-9.28381.351224.13284.683569.845821floatindexednullablexiParameter used by 2025Sci...387.1209Z to parameterize the shape of the extinction curve. For convenience, a conversion to R(55) is given as a separate column in this table._stat.fit.param;phys.absorption-4.18473-0.5404340.02837970.6630634.598751floatnullabler55Parameter describing the inverse slope of the extinction curve, defined by R(55) := A(550 nm) / [A(440 nm) - A(550 nm)]. This parameter can be approximately converted to the more traditional R(V) parameter by R(V) = 1.1*R(55) + 0.07. Note that this conversion is dependent on the specific B and V bandpasses and on stellar type!stat.fit.param;phys.absorption1.233591.760422.840956.4223438.67051floatnullableextEstimated extinction parameter. To convert to the extension at a particular wavelength, multiply this by that wavelength's value in the extinction curve, available at https://zenodo.org/record/7811871/files/extinction_curve.txt?download=1 and in the footnote.magphys.absorption0.0001062250.03531810.2727791.3467820.22251floatnullablemod_parallaxParallax estimated from the model.maspos.parallax3.08004e-060.04181260.42932.32034977.2741floatindexednullableerr_teffError in estimated effective temperature. Note that the raw HDF5 files released by 2025Sci...387.1209Z give the error in Teff in a different unit (Kilokelvin).Kstat.error;phys.temperature.effective3.5850729.7351126.66422.0529824121floatnullableerr_fe_hError in fe_hstat.error;phys.abund.Fe0.008445350.03762350.1554550.537113341.911floatnullableerr_loggError in log_gstat.error;phys.gravity0.002363020.01784870.1197830.552599947.9941floatnullableerr_xiError in xistat.error;stat.fit.param;phys.absorption0.00200280.01146150.0683740.524142115.5841floatnullableerr_r55Error in r55stat.error;stat.fit.param;phys.absorption0.0007246380.02993170.2123981.90351169.5591floatnullableerr_extError in extmagstat.error;phys.absorption0.001095880.008544640.0281360.076836568.66321floatnullableerr_mod_parallaxError in the parallax estimated from the model.masstat.error;pos.parallax9.40796e-070.01041020.04792420.11669510001floatnullablechi2_optχ² of the best-fit solution. Divide by 61 to obtain χ² per degree of freedom.stat.fit.chi20.06555180.5590820.99658213.0391630.51floatnullableln_priorNatural log of the GMM prior on stellar type, at the location of the optimal solution.stat.fit.goodness-510.75-8.273441.536133.441413.656251floatnullableteff_confidenceA neural-network-based estimate of the confidence in the effective temperature estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.02592470.9067380.9853520.9892581floatnullablefeh_confidenceA neural-network-based estimate of the confidence in the [Fe/H] estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.02406310.8999020.9863280.9892581floatnullablelogg_confidenceA neural-network-based estimate of the confidence in the log(g) estimate, on a scale of 0 (no confidence) to 1 (high confidence).stat.fit.goodness00.05749510.8881840.9775390.9892581floatnullablequality_flagsThe three least significant bits represent whether the confidence in effective temperature, [Fe/H] and log(g) is less than 0.5, respectively. The 4th bit is set if chi2_opt/61 > 2. The 5th bit is set if ln_prior < -7.43. The 6th bit is set if our parallax estimate is more than 10 sigma from the GDR3 measurement (using reported parallax uncertainties from GDR3). The two most significant bits are always unset. We recommend a cut of quality_flags < 8 (the "basic reliability cut"), although a stricter cut of quality_flags == 0 ensures higher reliability at the cost of lower completeness.meta.code.qual00.00.027.0631.0shortapass AAVSO Photometric All-Sky Survey (APASS), underway since 2010, covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY bandpasses. A northern and a southern site are used, each with twin ASA 20cm astrographs and Apogee Aspen CG16m cameras, covering 2.9x2.9 square degrees with 2.6arcsec pixels. Landolt and SDSS standards are used for all-sky solutions, with typical 0.02mag calibration errors on the bright end. Data Release 10 is a complete reprocessing of all 500K images taken with the system, including hundreds of nights not part of DR9. Sextractor is used for star finding and centroiding; DAOPHOT is used for aperture photometry; the astrometry.net plate-solving library is used for basic astrometry, supplanted with more precise WCS that utilizes knowledge of the optical train distortions. With these changes, DR10 includes many more stars than prior releases. More information is available at http://www.aavso.org/apass.apass.dr10 AAVSO Photometric All-Sky Survey (APASS), underway since 2010, covers the entire sky from 7.5 < V < 16.5 magnitude, and in the BVugrizY bandpasses. A northern and a southern site are used, each with twin ASA 20cm astrographs and Apogee Aspen CG16m cameras, covering 2.9x2.9 square degrees with 2.6arcsec pixels. Landolt and SDSS standards are used for all-sky solutions, with typical 0.02mag calibration errors on the bright end. Data Release 10 is a complete reprocessing of all 500K images taken with the system, including hundreds of nights not part of DR9. Sextractor is used for star finding and centroiding; DAOPHOT is used for aperture photometry; the astrometry.net plate-solving library is used for basic astrometry, supplanted with more precise WCS that utilizes knowledge of the optical train distortions. With these changes, DR10 includes many more stars than prior releases. More information is available at http://www.aavso.org/apass.130000000idAPASS DR10 identifier formed as (SPD zone)-(star number)meta.id;meta.maincharindexedprimaryraICRS right ascension for this object.pos.eq.ra;meta.main0.00010522.3253214.135339.4993601doubleindexednullabledecICRS declination for this object.pos.eq.dec;meta.main-89.9695-71.1344-17.654762.918788.73171doubleindexednullablera_errorEstimated error in ra (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.ra02.72222e-050.0001086110.0002636110.002310561floatnullabledec_errorEstimated error in dec (there will be additional systematics especially in crowded fields).degstat.error;pos.eq.dec02.27778e-058.52778e-050.0002116670.001908331floatnullablenobs_bNumber of observations that went into mag_bmeta.number;obs;em.opt.B00.03.013.012781.0shortmag_bMagnitude in Johnson B (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.B5.13313.15816.82218.20923.6320.787311floatnullableerr_mag_bEstimated error in mag_b. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.B00.0120.0980.3069.9990.787311floatnullablenobs_vNumber of observations that went into mag_vmeta.number;obs;em.opt.V00.03.013.012831.0shortmag_vMagnitude in Johnson V (Vega system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.V5.14412.36415.86717.42624.5320.787853floatnullableerr_mag_vEstimated error in mag_v. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.V00.010.0730.2279.9990.787853floatnullablenobs_uNumber of observations that went into mag_umeta.number;obs;em.opt.U00.00.00.001.0shortmag_uMagnitude in Sloan u' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.U0floatnullableerr_mag_uEstimated error in mag_u. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.U0floatnullablenobs_gNumber of observations that went into mag_gmeta.number;obs;em.opt.V01.04.016.012771.0shortmag_gMagnitude in Sloan g' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.V5.72713.00416.6518.23529.7460.978378floatnullableerr_mag_gEstimated error in mag_g. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.V00.010.0710.2619.9990.978378floatnullablenobs_rNumber of observations that went into mag_rmeta.number;obs;em.opt.R01.04.015.012681.0shortmag_rMagnitude in Sloan r' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.R4.91812.31515.81917.421.2190.97411floatnullableerr_mag_rEstimated error in mag_r. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.R00.0110.0830.2499.5450.97411floatnullablenobs_iNumber of observations that went into mag_imeta.number;obs;em.opt.I00.03.014.012651.0shortmag_iMagnitude in Sloan i' (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I3.68811.72915.11816.50821.2240.772479floatnullableerr_mag_iEstimated error in mag_i. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.I00.0140.110.3329.9990.772479floatnullablenobs_z_sNumber of observations that went into mag_z_smeta.number;obs;em.opt.I00.00.02.03941.0shortmag_z_sMagnitude in Sloan z_s (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I2.2079.62712.83313.96519.9190.0984147floatnullableerr_mag_z_sEstimated error in mag_z_s. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.I00.0080.1060.3889.9990.0984147floatnullablenobs_yNumber of observations that went into mag_ymeta.number;obs;em.opt.I00.00.00.001.0shortmag_yMagnitude in Sloan Y (AB system). This is an aperture magnitude obtained with DAOPHOT.magphot.mag;em.opt.I0floatnullableerr_mag_yEstimated error in mag_y. From a comparison with DR9, it appears these estimates are overly pessimistic.magstat.error;phot.mag;em.opt.I0floatnullablehipparcosThe main result catalog from the ESA Hipparcos satellite, obtained November 1989 through March 1993. In the GAVO DC, several columns were left out and all angles are given in degrees.hipparcos.mainThe main result catalog from the ESA Hipparcos satellite, obtained November 1989 through March 1993. In the GAVO DC, several columns were left out and all angles are given in degrees.117955hipnoIdentifier (HIP number)meta.id;meta.main13547.6259172.0114802.379999999991204041.0intindexedprimaryraRight ascension ICRS (Epoch J1991.25)degpos.eq.ra;meta.main0.0009118511.3332181.97348.745359.9791doubleindexeddecDeclination ICRS (Epoch J1991.25)degpos.eq.dec;meta.main-89.7825-70.5209-1.9459369.0389.56941doubleindexedvmagMagnitude in Johnson Vmagphot.mag;em.opt.V-1.445.698.4410.814.081floatnullablevarflagCoarse variability flagmeta.code;src.varbooleanwhatposPosition is for -- A-Z: multiple component, *: Photocenter, +: Center of massmeta.notecharnullableparallaxTrigonometric parallaxdegpos.parallax.trig-1.52639e-05-4.72222e-081.28056e-067.64167e-060.0002145361floatnullablepmraProper motion in RA, cos(delta) applieddeg/yrpos.pm;pos.eq.ra-0.00122522-3.52344e-05-4.66667e-073.46944e-050.001879791doublenullablepmdeProper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.00161472-4.47421e-05-1.56944e-061.61806e-050.002868591doublenullablee_radegStandard error in RA*cos(delta)degstat.error7.5e-081.22222e-072.41667e-079.19444e-077.81e-051floatnullablee_dedegStandard error in DEdegstat.error9.16667e-081.25e-072e-077.55556e-076.69611e-051floatnullablee_parallaxStandard error of parallaxdegstat.error1.05556e-071.63889e-073.05556e-079.08333e-073.17944e-051floatnullablee_pmraStandard error in PM in RAdeg/yrstat.error8.05556e-081.38889e-072.83333e-079.52778e-075.54306e-051floatnullablee_pmdeStandard error in PM in Decdeg/yrstat.error8.88889e-081.36111e-072.36111e-077.63889e-072.72583e-051floatnullablef2Goodness-of-fit parameter, >3 means bad datastat.fit.goodness-4.41-1.760.262.4227.220.986749floatnullablehpmagMedian magnitude in Hipparcos systemmagphot.mag;em.opt.V-1.08765.762728.550910.917314.56221floatnullablee_hpmagStandard error on median magnitudemagstat.error0.00020.00070.00180.01230.93171floatnullablehpscatScatter on median magnitudemagphot.mag;em.opt.V0.0030.0060.0160.0651.9760.991887floatnullableo_hpmagNumber of observations in median magnitudemeta.number751.0105.0207.03730.99188673shortnullablewhatmagMag is for -- A-Z: multiple component, *: combined and corrected for attenuation, +: combined and not corrected for attenuationmeta.code.multipcharnullablehpmaxHpmag at maximum (5th percentile)magphot.mag;em.opt.V-1.175.748.5110.7913.790.991887floatnullablehpminHpmag at minimum (95th percentile)magphot.mag;em.opt.V-0.985.788.5810.9914.990.991887floatnullableperiodVariability periodstime.period4320112322082243.29115e+078.08764e+070.0215082floatnullablesptypeSpectral type from various sourcessrc.spTypecharnullablemultflagMultiplicity flag, see note.meta.code.multipcharnullablebinpaPosition angle between componentsdegpos.posAng;src.orbital091833503590.0941122floatnullablebinsepAngular separation between componentsarcsecpos.angDistance;src.orbital0.0820.1350.97811.57723.5880.0941122floatnullablebinseperrStandard error on ang. separationarcsecstat.error;pos.angDistance;src.orbital0.0010.0020.0110.0730.2420.0941122floatnullablemagdiffMagnitude difference of componentsmagphot.mag;arith.diff00.071.633.844.470.0941122floatnullableopenngc OpenNGC is a database containing positions and main data of NGC (New General Catalogue) and IC (Index Catalogue) objects. It has been built by merging data from NED, HyperLEDA, SIMBAD, and several databases available at HEASARC. In this VO publication, we have changed most of the column names, mostly to make them work as ADQL column names without resorting to delimited identifiers. The mapping should be obvious.openngc.dataThe OpenNGC object list with the main metadata13969nameObject identifier, either from NGC or from IC.meta.id;meta.maincharindexednullableobj_typeObject Type. See note for terms and symbols used.src.classcharindexednullableraj2000Right Ascension in ICRS for Epoch J2000.0.degpos.eq.ra;meta.main0.0382511.5193184.291348.645359.9610.999499doublenullabledej2000Declination in ICRS for Epoch J2000.0.degpos.eq.dec;meta.main-89.3345-68.768910.40762.382889.09310.999499doublenullableconstellationConstellation the object is located in.meta.id.parentcharnullablemaj_ax_degMajor axis of covering ellipsoid.degphys.angSize.sMajAxis0.0003333330.006333330.020.124.998670.859403floatnullablemin_ax_degMinor axis of covering ellipsoid.degphys.angSize.sMinAxis0.0003333330.003666670.01150.05043172.998170.790894floatnullablepos_angPosition angle of covering ellipsoid, north over east.degpos.posAng04871751800.768344floatnullablemag_bApparent total magnitude in the B Band.magphot.mag;em.opt.B1.519.6514.4216.7921.010.81144floatnullablemag_vApparent total magnitude in the V Band.magphot.mag;em.opt.V1.696.612.3815.026120.410.301668floatnullablemag_jApparent total magnitude in the J Band.magphot.mag;em.ir.J1.118.5611.4213.8317.020.690959floatnullablemag_hApparent total magnitude in the H Band.magphot.mag;em.ir.H0.837.8910.7413.242416.670.693894floatnullablemag_kApparent total magnitude in the K Band.magphot.mag;em.ir.K0.727.6310.4612.9315.760.690959floatnullablesurf_br_bMean surface brigthness within the 25 mag isophote (B-band); only given for galaxiesmag/arcsec**2phot.mag.sb18.3622.137823.3324.4228.480.732121floatnullablehubble_typeMorphological Hubble type for galaxies.src.morph.typeEE-S0E?IIABIBS0S0-aS?SABaSABbSABcSABdSABmSBaSBabSBbSBbcSBcSBcdSBdSBmSaSabSbSbcScScdSdSmcharindexednullablepmraProper motion in RAmas/yrpos.pm;pos.eq.ra-43.57-9.26679-0.90155.49962760.0747369floatnullablepmdecProper motion in Declinationmas/yrpos.pm;pos.eq.dec-58.961-10.5947-1.0885.68698640.0747369floatnullablervHeliocentric radial velocitykm/sspect.dopplerVeloc-483-9.54488515721.3520250.757606floatnullablezHeliocentric redshiftsrc.redshift-0.00161-3.108e-050.016430.05388940.1916160.757606floatnullablecstar_mag_uFor planetary nebulae: Apparent magnitude of the central star in the U Band.magphot.mag;em.opt.U9.39.45312.0914.574514.750.00114539floatnullablecstar_mag_bFor planetary nebulae: Apparent magnitude of the central star in the B Band.magphot.mag;em.opt.B9.9310.34515.519.69521.10.00794617floatnullablecstar_mag_vFor planetary nebulae: Apparent magnitude of the central star in the V Band.magphot.mag;em.opt.V9.4210.37415.14519.01819.60.00687236floatnullablemessier_nrMessier number for this objectmeta.id.cross14.1856.0106.821100.007659818intnullableother_ngcOther NGC number for this object in case it was duplicated in IC or NCG.meta.id.crosscharnullableic_crossOther IC number for this object in case it was duplicated in IC or NCG.meta.id.crosscharnullablecstar_idIdentifier of the central star for planetary nebulae.meta.id.crosscharnullableother_idCross reference to other catalogs.meta.id.crosscharnullablecomnameCommon name(s) of the object.charnullablened_notesNotes about the object exported from NEDmeta.notecharnullablesourcesSources of the various categories of datameta.bibcharnullablenotesNotes about the object from OpenNGCmeta.notecharnullableopenngc.shapes Hand-drawn coverages of selected openngc objects. Up to three coverages at different surface brightness are obtained using the default DSS2 Color layer in Aladin. Usually, the level 2 shape is taken with default histogram, while level 1 and level 3 use, respectvely, the first and the last half of the histogram.193nameName of the (main) object the coverage is for.meta.idcharindexedprimaryshape_level1Coverage obtained by tracing the object's outline visually in DSS colour, with full output intensity at half saturation.phys.angAreacharnullableshape_level2Coverage obtained by tracing the object's outline visually in DSS colour, with zero output intensity at zero saturation and full output intensity at full saturation.phys.angAreacharnullableshape_level3Coverage obtained by tracing the object's outline visually in DSS colour, with zero output intensity at half saturation and full output intensity at full saturation.phys.angAreacharnullabledeepest_shapeDeepest coverage available. As opposed to the other shape columns, this will always contain something as long as we have some coverage information; this is provided for convenience.phys.angArea;meta.maincharnullableopenngc.datanamenameppmxl PPMXL is a catalog of positions, proper motions, 2MASS- and optical photometry of 900 million stars and galaxies, aiming to be complete down to about V=20 full-sky. It is the result of a re-reduction of USNO-B1 together with 2MASS to the ICRS as represented by PPMX. This service additionally provides improved proper motions computed according to Vickers et al, 2016 (:bibcode:`2016AJ....151...99V`).ppmxl.main PPMXL is a catalog of positions, proper motions, 2MASS- and optical photometry of 900 million stars and galaxies, aiming to be complete down to about V=20 full-sky. It is the result of a re-reduction of USNO-B1 together with 2MASS to the ICRS as represented by PPMX. This service additionally provides improved proper motions computed according to Vickers et al, 2016 (:bibcode:`2016AJ....151...99V`).900000000ipixIdentifier (Q3C ipix of the USNO-B 1.0 object)meta.id;meta.main68187852794531.4555397969262336e+174.897678929650011e+186.544739885363848e+1869175110039938228571.0longindexedraj2000Right Ascension J2000.0, epoch 2000.0degpos.eq.ra;meta.main6e-0620.8815237.901340.5833601doubleindexednullabledej2000Declination J2000.0, epoch 2000.0degpos.eq.dec;meta.main-89.886-70.7159-17.90564.550289.93921doubleindexednullablee_raepraMean error in RA*cos(delta) at mean epochdegstat.error;pos.eq.ra;meta.main2.78e-071.75e-053.11e-054.53e-055.75e-051floatnullablee_deepdeMean error in Dec at mean epochdegstat.error;pos.eq.dec;meta.main2.78e-071.75e-053.14e-054.53e-055.69e-051floatnullablepmraProper Motion in RA*cos(delta)deg/yrpos.pm;pos.eq.ra-0.0026833-3.6267e-05-4.6389e-073.1322e-050.00271881floatindexednullablepmdeProper Motion in Decdeg/yrpos.pm;pos.eq.dec-0.002712-4.03e-05-7.8056e-073.6792e-050.0027711floatindexednullablee_pmraMean error in pmRA*cos(delta)deg/yrstat.error;pos.pm;pos.eq.ra5.56e-081.06e-062.11e-066.86e-062.48e-051floatnullablee_pmdeMean error in pmDEdeg/yrstat.error;pos.pm;pos.eq.dec2.78e-081.06e-062.11e-066.86e-062.48e-051floatnullablenobsNumber of observations usedmeta.number;obs22.04.06.0150.99985075shortnullableepraMean Epoch (RA)yrtime.epoch;pos.eq.ra1924.171968.311984.651995.592005.131floatnullableepdeMean Epoch (Dec)yrtime.epoch;pos.eq.dec1922.621968.31984.651995.62005.131floatnullablejmagJ selected default magnitude from 2MASSmagphot.mag;em.IR.J-1.31411.71715.52116.79621.7490.453138floatnullablee_jmagJ total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0660.1639.9990.446147floatnullablehmagH selected default magnitude from 2MASSmagphot.mag;em.IR.H-2.23511.0314.96116.28220.1470.453138floatnullablee_hmagH total magnitude uncertaintymagstat.error;phot.mag;em.IR.H00.0220.0780.2139.9980.419335floatnullablekmagK_s selected default magnitude from 2MASSmagphot.mag;em.IR.K-2.66310.78614.75516.23219.8720.453138floatnullablee_kmagK_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K00.0210.0890.2459.9990.353952floatnullableb1magB mag from USNO-B, first epochmagphot.mag;em.opt.B-0.6214.7419.4321.0464.880.400937floatnullableb2magB mag from USNO-B, second epochmagphot.mag;em.opt.B-0.4415.2219.2121.665.380.853922floatnullabler1magR mag from USNO-B, first epochmagphot.mag;em.opt.R-1.2213.817.9220.0465.430.793746floatnullabler2magR mag from USNO-B, second epochmagphot.mag;em.opt.R0.1714.2118.2420.965.450.806482floatnullableimagI mag from USNO-Bmagphot.mag;em.opt.I-0.6413.1617.2518.9865.120.73584floatnullablemagsurveysSurveys the USNO-B magnitudes are taken frommeta.codecharnullableflagsFlagsmeta.code00.00.01.0101.0shortvickers_pmraProper motion in RA as re-corrected according to 2016AJ....151...99V, cos(delta) applied. This is only available for objects with 2MASS J magnitudes. e_pmRA still is suitable as an error estimate.deg/yrpos.pm;pos.eq.ra-0.0025239-1.124e-05-3.3235e-071.2709e-050.00211370.453138floatnullablevickers_pmdeProper motion in Dec as re-corrected according to 2016AJ....151...99V. This is only available for objects with 2MASS J magnitudes. e_pmDE still is suitable as an error estimate.deg/yrpos.pm;pos.eq.dec-0.0026772-1.324e-05-8.97155e-081.0725e-050.00215670.453138floatnullableppmxl.usnocorrCorrections between USNO-B1 and PPMXL on a grid of degrees, obtained by substracting PPMXL from USNO in cones of radius sqrt(2)/2 degrees around the given center position.64800nobNumber of objects the correction is based onmeta.number18158168.019271.0132741.499999999944534101.0intalphaCenter for field, RAdegpos.eq.ra;meta.main0.510.5180349.5359.51floatindexednullabledeltaCenter for field, Decdegpos.eq.dec;meta.main-89.5-84.5084.589.51floatindexednullabled_alphaCorrection PPMXL-USNO in alpha (Epoch 2000.0)degpos.eq.ra;arith.diff-0.0133948-0.00122579-4.56111e-059.39135e-050.001097611floatnullabled_deltaCorrection PPMXL-USNO in delta (Epoch 2000.0)degpos.eq.dec;arith.diff-0.000136125-5.45663e-058.55515e-079.37356e-050.0001790651floatnullabled_pmalphaCorrection PPMXL-USNO in proper motion alpha*cos(delta)deg/yrpos.pm;pos.eq.ra;arith.diff-4.30888e-06-2.32278e-06-3.40458e-072.13868e-064.92653e-061floatnullabled_pmdeltaCorrection PPMXL-USNO in deltadeg/yrpos.pm;pos.eq.dec;arith.diff-4.4126e-06-2.16193e-06-6.47953e-071.99619e-064.65377e-061floatnullablerome The ROME/REA (Robotic Observations of Microlensing Events/Reactive Event Assessment) Survey was a Key Project at Las Cumbres Observatory (hereafter LCO) which continuously monitored 20 selected fields (3.76 sq.deg.) in the Galactic Bulge throughout their seasonal visibility window over a three-year period, between March 2017 and March 2020. Observations were made in three optical passbands (SDSS g', r', i'), and LCO's multi-site telescope network enabled the survey to achieve a typical cadence of ~10hrs in i' and ~15hrs in g' and r'. In addition, intervals of higher cadence (<1hr) data were obtained during monitoring of key microlensing events within the fields. This catalog includes the full timeseries photometry for all ~8 million stars, down to a limiting magnitude of i~18mag.rome.images The ROME/REA (Robotic Observations of Microlensing Events/Reactive Event Assessment) Survey was a Key Project at Las Cumbres Observatory (hereafter LCO) which continuously monitored 20 selected fields (3.76 sq.deg.) in the Galactic Bulge throughout their seasonal visibility window over a three-year period, between March 2017 and March 2020. Observations were made in three optical passbands (SDSS g', r', i'), and LCO's multi-site telescope network enabled the survey to achieve a typical cadence of ~10hrs in i' and ~15hrs in g' and r'. In addition, intervals of higher cadence (<1hr) data were obtained during monitoring of key microlensing events within the fields. This catalog includes the full timeseries photometry for all ~8 million stars, down to a limiting magnitude of i~18mag.41050accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Sizelongnullablerome_idIdentifier for the ROME/REA image. This is field*100000+per-field-indexmeta.id;meta.mainintfieldROME field the object was observed inmeta.id;obs.fieldshortimage_indexInternal index of the image within a dataset, starting from 0. This correspondds to the index of a photometry row in the photometry hdf5smeta.idshortfilenameUpstream file name for this imagecharnullabledataset_codeDataset this image belongs to (a dataset in ROME/REA is the collection of all images from a given instrument)charnullablefilterFilter this image was taken withmeta.id;instr.filtercharnullablehjdHJD (i.e., UTC with light-time corrections for the solar centre) of the midpoint of exposuredtime.epochdoublenullableexposureExposure time for this imagestime.duration;obs.exposuredoublenullablemoon_ang_separationAngular Distance to the moondeginstr.param;pos.angDistancefloatnullablemoon_fractionMoon phase, 0=new mooninstr.paramdoublenullableairmassAirmass for this observationobs.airMassdoublenullablenstarsNumber of photometry points extracted from this imagemeta.numberintfrac_sat_pixFraction of saturated pixels on this imagephot.count;arith.ratiodoublenullableqc_flagQuality flags; null means a good image, for other codes see table notemeta.code.qualshortnullablerome.time_series The ROME/REA (Robotic Observations of Microlensing Events/Reactive Event Assessment) Survey was a Key Project at Las Cumbres Observatory (hereafter LCO) which continuously monitored 20 selected fields (3.76 sq.deg.) in the Galactic Bulge throughout their seasonal visibility window over a three-year period, between March 2017 and March 2020. Observations were made in three optical passbands (SDSS g', r', i'), and LCO's multi-site telescope network enabled the survey to achieve a typical cadence of ~10hrs in i' and ~15hrs in g' and r'. In addition, intervals of higher cadence (<1hr) data were obtained during monitoring of key microlensing events within the fields. This catalog includes the full timeseries photometry for all ~8 million stars, down to a limiting magnitude of i~18mag.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size3000030000.030000.030000.0300001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMean MJD of observationsdtime.epoch5784858117.1582995843358739.81doublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.Unitcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.mag;em.optcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitmagcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionROME/REA time seriescharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcepointedcharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationABSOLUTEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.Calibrationcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablerome_idLocal unique identifier for this object within ROME/REA: field*10'000'000+quadrant*1'000'000'+quadrant_idmeta.id;meta.main1100000113039417.57112033866.5202117348.432041216641.0intupstream_nameUpstream has a field/field_id naming scheme skipping the quadrants. This column can be used to go from our data to upstream's.meta.idcharindexednullableraICRS right ascension of this objectdegmeta.id;meta.main267.582267.845269.363270.949271.0911doublenullabledecICRS declination of this objectdegmeta.id;meta.main-30.4776-30.2599-29.0399-27.9015-27.75911doublenullablehjd_minEarliest observation represented in the time seriesdtime.epoch;stat.min2.45783e+062.45785e+062.45786e+062.45834e+062.45874e+061doublenullablehjd_maxLatest observation represented in the time seriesdtime.epoch;stat.max2.45785e+062.45828e+062.45874e+062.45877e+062.45902e+061doublenullablemag_i_minMinimal (brightest) magnitude measured in the SDSS i' band.magphot.mag;em.opt.i;stat.min2.9140311.348615.640417.777829.38480.937083floatindexednullablemag_i_maxMaximal (faintest) magnitude measured the SDSS i' band.magphot.mag;em.opt.i;stat.max8.6723615.351719.429224.651140.1950.937083floatindexednullablemag_i_meanMean magnitude of the SDSS i' lightcurve.magphot.mag;em.opt.i;stat.mean8.6723614.728117.429519.604729.38480.937083floatnullablenp_iNumber of measurements in the SDSS i' lightcurve.meta.number;obs00.0137.0535.07541.0shortmag_g_minMinimal (brightest) magnitude measured in the SDSS g' band.magphot.mag;em.opt.v;stat.min6.7724615.854318.389420.418230.08450.55899floatnullablemag_g_maxMaximal (faintest) magnitude measured the SDSS g' band.magphot.mag;em.opt.v;stat.max12.438317.556120.796425.322639.16740.55899floatnullablemag_g_meanMean magnitude of the SDSS g' lightcurve.magphot.mag;em.opt.v;stat.mean11.846817.124819.637721.624430.08450.55899floatnullablenp_gNumber of measurements in the SDSS g' lightcurve.meta.number;obs00.07.0193.02221.0shortmag_r_minMinimal (brightest) magnitude measured in the SDSS r' band.magphot.mag;em.opt.r;stat.min5.5276914.239117.022719.147630.51010.761248floatnullablemag_r_maxMaximal (faintest) magnitude measured the SDSS r' band.magphot.mag;em.opt.r;stat.max10.350316.202819.474224.408338.06220.761248floatnullablemag_r_meanMean magnitude of the SDSS r' lightcurve.magphot.mag;em.opt.r;stat.mean10.350315.80718.315120.48330.51010.761248floatnullablenp_rNumber of measurements in the SDSS r' lightcurve.meta.number;obs00.062.0214.02941.0shortfieldROME field the object was observed inmeta.id;obs.field11.011.020.0201.0shortquadrantQuadrant of this object (for purely technical reasons, ROME has split each field into four quadrants).meta.id;obs.field11.02.04.041.0shortquadrant_idIdentifier for this object within its quadrantmeta.id13560.049191.0106596.01276121.0intgaia_source_idGaia DR3 source_id for this objectmeta.id.cross40503874971173656324.05620800677535e+184.0622685448858225e+184.0627713352638607e+1840635225765630880000.50245965longnullablesdssdr16 This is a redacted version of the SDSS DR16 table prepared for VizieR (V/154/sdss16). It is mainly here to facilitate local matches; for original SDSS-related research, it is probably better to somewhere else. Over VizieR and SDSS, we are keeping most of the per-band values in arrays to keep the column list manageable. Note that in ADQL, array indexes are 1-based. We are trying to orient our column names on SDSS but use underscores instead of camel-casing (e.g. spec_obj_id instead of SpecObjID), since mixed-case identifiers in SQL is asking for trouble. To save space, we do not keep psf-based classifications, per-band offsets, spectrum metadata, and USNO-related information in this table. Let the operators know if you need any of that.sdssdr16.main This is a redacted version of the SDSS DR16 table prepared for VizieR (V/154/sdss16). It is mainly here to facilitate local matches; for original SDSS-related research, it is probably better to somewhere else. Over VizieR and SDSS, we are keeping most of the per-band values in arrays to keep the column list manageable. Note that in ADQL, array indexes are 1-based. We are trying to orient our column names on SDSS but use underscores instead of camel-casing (e.g. spec_obj_id instead of SpecObjID), since mixed-case identifiers in SQL is asking for trouble. To save space, we do not keep psf-based classifications, per-band offsets, spectrum metadata, and USNO-related information in this table. Let the operators know if you need any of that.1300000000obj_idSDSS unique object identifiermeta.id;meta.main12376458768612720721.2376487029592556e+181.237663789570392e+181.2376802409161032e+1812376805313565831161.0longindexedprimaryraRight Ascension of the object (ICRS)degpos.eq.ra;meta.main8.15592e-079.62755191.806352.1833601doubleindexednullabledecDeclination of the object (ICRS)degpos.eq.dec;meta.main-25.0091-10.109913.833862.842684.97911doubleindexednullablera_errMean error on raarcsecstat.error;pos.eq.ra00.001130530.07389110.3449319238.571floatnullabledec_errMean error on decarcsecstat.error;pos.eq.dec00.001108430.07284670.3369759238.571floatnullablepm_raProper motion along Right Ascensionmas/yrpos.pm;pos.eq.ra-4964.48-18.0276016.08253986.860.273693floatnullablee_pm_raMean error on pmramas/yrstat.error;pos.pm;pos.eq.ra002.528835.663022055.030.273693floatnullablepm_decProper motion along Declinationmas/yrpos.pm;pos.eq.dec-4033.23-20.7891012.85252017.10.273693floatnullablepm_dec_errMean error on pmDE.mas/yrstat.error;pos.pm;pos.eq.dec002.528835.663022055.030.273693floatnullablepm_sig_raRMS residual of proper motion fit in RA.masstat.fit.residual0077.6644498.8658362.950.273693floatnullablepm_sig_decRMS residual of proper motion fit in Dec.masstat.fit.residual0074.436504.3458519.070.273693floatnullableuModel magnitude in u filter AB scalemagphot.mag;em.opt.u4.9787917.377723.433426.173637.2390.961699floatnullableerr_uError in the model magnitude in u filter AB scalemagstat.error;phot.mag;em.opt.u2.65705e-070.01006090.6128051.684961984.410.961699floatnullablegModel magnitude in g filter AB scalemagphot.mag;em.opt.v4.9384215.856822.449225.524239.09720.95831floatnullableerr_gError in the model magnitude in g filter AB scalemagstat.error;phot.mag;em.opt.v3.93157e-080.003757220.1508460.855073894.4170.95831floatnullablerModel magnitude in r filter AB scalemagphot.mag;em.opt.r5.2685515.206821.364124.953337.92830.965748floatnullableerr_rError in the model magnitude in r filter AB scalemagstat.error;phot.mag;em.opt.r1.66778e-070.003584960.08796560.765091684.6430.965748floatnullableiModel magnitude in i filter AB scalemagphot.mag;em.opt.i4.5105914.977920.7124.408638.05220.96356floatnullableerr_iError in the model magnitude in i filter AB scalemagstat.error;phot.mag;em.opt.i1.53781e-070.003719770.07318130.719741480.1930.96356floatnullablezModel magnitude in z filter AB scalemagphot.mag;em.opt.i4.1633214.682720.250723.205436.61830.960951floatnullableerr_zError in the model magnitude in z filter AB scalemagstat.error;phot.mag;em.opt.i2.04563e-070.005017460.1767141.011911041.670.960951floatnullablefield_idThe field this object is in.meta.note12376458768612720641.2376487029592556e+181.237663789570392e+181.2376802409161032e+1812376805313565818881.0longmodePhoto mode (1=primary, 2=secondary, 3=family, 4=outside)meta.code.class11.02.04.041.0shortclassType of object (3=galaxy, 6=star)src.class00.06.06.081.0shortindexedcleanClean photometry flag (1=clean; 0=unclean)meta.code00.00.01.011.0shortphoto_flagsPhoto Object Attribute flagsmeta.code.error26843545668987912192.0105622137864208.0545426790027536.013712737918332485901.0longpsfmagsArray of PSF magnitudes, in ugriz sequencemagphot.magfloatnullablepsfmag_errsArray of the errors of the PSF magnitudes, in ubriz sequencemagstat.error;phot.magfloatnullablepetmagsArray of Petrosian magnitudes, in ugriz sequencemagphot.magfloatnullablepetmag_errsArray of the errors Petrosian magnitudes, in ugriz sequencemagstat.error;phot.magfloatnullablepetradsArray of Petrosian radii, in ugriz sequencearcsecphys.angSize;srcfloatnullablepetrad_errsArray of Petrosian radii, in ugriz sequencearcsecstat.error;phys.angSize;srcfloatnullabledev_radsArray of de Vaucouleurs fit radii, in ugriz sequencearcsecphys.angSize;srcfloatnullabledev_absArray of de Vaucouleurs fit b/a ratios, in ugriz sequencephys.size.axisRatiofloatnullabledev_phiArray of position angles of de Vaucouleurs fits in ugriz sequence (warning: anything smaller than 0 in here must be considered NULL).degpos.posAngfloatnullableflagsArray of detection flags, in ugriz sequencemeta.codelongnullabletypesArray of phototypes (6=Star ; 3=galaxy) in ugriz sequencesrc.class.starGalaxyshortnullableparent_idPointer to parent (if object deblended)meta.id.parent12376458768612720691.2376487040566077e+181.2376653303895163e+181.237680241432265e+1812376805313565830380.40204456longnullablespec_zSpectroscopic final redshift (when SpObjID>0)src.redshift-0.0101934-0.0004861680.4277882.473757.013090.00374838floatindexednullablespec_z_errMean error on spec_z (negative for bad fit)stat.error-67.32932e-069.20743e-050.00103451235.310.00374838floatnullablespec_z_warningWarning flag on redshift.meta.code00.00.04.09020.0037483769shortnullablespec_classSpectroscopic class: "GALAXY"; "QSO"; "STAR"meta.code.class;pos.parallax.spectcharnullablespec_sub_classSpectroscopic subclass.src.classcharnullablespec_vel_dispVelocity dispersionkm/sphys.veloc.dispersion00131.81685.7348500.00339887floatnullablespec_vel_disp_errMean error on spec_vel_dispkm/sstat.error-7014.4179120.2632262.740.00339887floatnullablespec_sn_medianMedian signal-to-noise over all good pixels.em.wl.central;stat.median-1926.590.7174153.7563641.6322131.2360.00339887floatnullablephotoz_zPhotometric redshift estimated by robust fit to nearest neighbors in a reference setsrc.redshift0.00050.111430.4410590.86923510.150934floatindexednullablephotoz_z_errEstimated error of the photometric redshiftstat.error;src.redshift0.0033940.0296170.0899910.1848210.2915180.150934floatnullablephotoz_nn_avg_zAverage redshift of the nearest neighbors; if significantly different from photoz_z this might be a better estimate than photoz_zsrc.redshift.phot0.010190.1366740.4118340.7034550.8010410.169369floatnullablephotoz_chisqChi-square value for the minimum chi-square template fitstat.value8.32632e-120.4042688.0555898.36123.27581e+070.169369floatnullablefield_qualityQuality of the observation: 1=bad; 2=barely acceptable; 3=goodmeta.code.qual;obs.param;obs11.03.03.031.0shortfield_mjdsArray of dates of observation per ugriz banddtime.epochdoublenullablesdss_idSDSS object identifier (run-rerun-camcol-field-object)meta.idcharnullablespectral_idSpectroscopic Plate-MJD-Fiber identifier (plate-mjd-fiberID)meta.idcharnullabletwomassThe 2MASS Point Source Catalogue, short a couple of exotic fields. We provide this data mainly for matching with other catalogs within our TAP service.twomass.dataThe 2MASS Point Source Catalogue, short a couple of exotic fields. We provide this data mainly for matching with other catalogs within our TAP service.480000000raj2000Right ascension (J2000)degpos.eq.ra;meta.main1.3e-0529.5025250.807336.0483601doubleindexednullabledej2000Declination (J2000)degpos.eq.dec;meta.main-89.9928-68.5024-16.858162.995389.96821doubleindexednullableerrmajMajor axis of position error ellipsedegstat.error;pos.eq1.66667e-051.66667e-052.22222e-058.61111e-050.0002861111floatnullableerrminMinor axis of position error ellipsedegstat.error;pos.eq1.38889e-051.66667e-052.22222e-057.5e-050.0002777781floatnullableerrpaPosition angle of error ellipse major axis (E of N)degstat.error;pos.eq00451741801floatnullablemainidSource designationmeta.id;meta.maincharindexedprimaryjmag2MASS J magnitudemagphot.mag;em.IR.J-2.98911.82815.54816.84322.8431floatindexednullablejcmsigJ default magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0010.0190.0680.1679.9990.953595floatnullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0690.1679.9990.953595floatnullablejsnrJ Signal-to-noise ratiostat.snr;phot.mag;em.IR.J06.517.8541.51e+060.953595floatnullablehmag2MASS H magnitudemagphot.mag;em.IR.H-4.00711.06314.90816.27824.2920.999999floatindexednullablehcmsigH default magnitude uncertaintymagstat.error;phot.mag;em.IR.H0.0010.020.0780.2139.9990.909418floatnullablee_hmag2MASS H total magnitude uncertaintymagstat.error;phot.mag;em.IR.H0.010.0220.0790.2139.9990.909418floatnullablehsnrH Signal-to-noise ratiostat.snr;phot.mag;em.IR.H05.115.2476.81e+060.909418floatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.K-4.37810.73314.66516.20520.5320.999998floatindexednullablekcmsigmagnitude uncertaintymagstat.error;phot.mag;em.IR.K0.0010.0190.0850.2439.9990.770189floatnullablee_kmag2MASS K_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K0.0110.0210.0860.2439.9990.770189floatnullableksnrK Signal-to-noise ratiostat.snr;phot.mag;em.IR.K0.14.413.2427.41e+060.770189floatnullableqflgJHK photometric quality flagmeta.code.qual;photcharnullablerflgJHK default magnitude read flagmeta.refcharnullablebflgJHK blend flagmeta.codecharnullablecflgContamination and confusion flagmeta.codecharnullablexflgExtended source contaminationmeta.codecharnullableaflgAssociation with asteroid or cometmeta.codecharnullablepts_keyUnique source identifier in cataloguemeta.id;meta.table16835164496.6628124788.01299824730.313400368801.0longindexed"date"Observation dateyrtime.epoch;obscharnullablescanScan number (within date)meta.id;obs.field614.067.0138.03271.0shortxscanDistance of source from focal plane centerlinedegpos.distance;pos.cartesian;instr.det-248.4-199.9-0.9199.5247.71floatnullablejdJulian date of detectiondtime.epochcharnullableedgensDistance from the source to the nearest North or South scan edgedegpos;arith.diff10583566610751110871floatnullableedgeewDistance from the source to the nearest East or West scan edgedegpos;arith.diff10441482462581floatnullableedgeflag indicating to which edges the edgeNS and edgeEW values refermeta.code;pos.cartesian;instr.detcharnullabledupFlag indicating duplicate sourcemeta.codecharnullableuse_srcUse source flagmeta.codecharnullablewise The Wide-field Infrared Survey Explorer (WISE) is a space-based imaging survey of the entire sky in the 3.4 (W1), 4.6 (W2), 12 (W3), and 22 (W4) μm mid-infrared. This is the project's reliable Source Catalog containing accurate photometry and astrometry for over 500 million objects. More details are available in the `Explanatory Supplement`_, which also has a list of `Cautionary Notes`_. .. _Explanatory Supplement: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_1.html .. _Cautionary Notes: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec1_4b.htmlwise.main This is the All-Sky source catalog, with several columns left out since we considered them to be only relevant for re-reduction, too arcane, or just because of a whim on our side. If you need them, let us know. The columns left out include: elon, elat, source_id, w?nm w?m, w?cov, w?cc_map_str, w?flux, w?sigflux, w?sky, w?sigsk, w?conf, w?mag_?, w?sigm_?, w?flg_?, w?magp, w?sigp1, w?sigp2, rho??, r_2mass, pa_2mass, n_2mass, [jhk]_m_2mass, [jhk]_msig_2mass, best_use_cntr, ngrp, x, y, z, spt_ind570000000designationSexagesimal, equatorial position-based source name in the form: hhmmss.ss+ddmmss.s. The full naming convention for WISE All-Sky Release Catalog sources has the form 'WISE Jhhmmss.ss+ddmmss.s,', where WISE is not given in this column.meta.id;meta.maincharindexedprimaryraj2000J2000 right ascension with respect to the 2MASS PSC reference framedegpos.eq.ra;meta.main4.37e-0513.642196.432346.4893601doubleindexednullabledej2000J2000 declination with respect to the 2MASS PSC reference frame.degpos.eq.dec;meta.main-89.9428-71.2711-2.9088269.568189.98531doubleindexednullablesigraOne-sigma uncertainty in right ascension coordinate.degstat.error;pos.eq.ra1.94444e-072.13611e-058.91667e-050.0003122220.007405860.999998floatnullablesigdecOne-sigma uncertainty in declination coordinate.degstat.error;pos.eq.dec1.66667e-072.08333e-059.38889e-050.0003318060.01140580.999998floatnullablesigradecThe co-sigma of the equatorial position uncertainties, sig_ra, sig_dec (σα, σδ).degstat.error;pos.eq-15.9238-0.307-0.02590.21471.14070.999998floatnullableglonGalactic longitude. CAUTION: This coordinate should not be used as an astrometric reference.degpos.galactic.lon3.1e-069.46008179.79350.4023601doublenullableglatGalactic latitude. CAUTION: This coordinate should not be used as an astrometric reference.degpos.galactic.lat-89.9943-65.7531-0.081102666.169989.95451doublenullablewxThe x-pixel coordinate of this source on the Atlas Image.pixpos.cartesian.x;instr.det36.4205.412046.943889.394058.61floatnullablewyThe y-pixel coordinate of this source on the Atlas Image.pixpos.cartesian.y;instr.det36.401182.4832046.923912.234058.61floatnullablecntrUnique identification number for the Catalog source.meta.id16012410000011.2315300124100269e+171.9531106012410196e+183.453022801241007e+1835841196012410388341.0longcoadd_idAtlas Tile identifier from which source was extracted.meta.idcharnullablesrcSequential number of this source extraction in the Atlas Tile from which this source was extracted, in approximate descending order of W1 source brightness.meta.id;obs11377.023640.053577.0701791.0intw1mproMagnitude at 3.4µm measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the 3.4µm flux measurement has SNR<2. This column is null if the source is nominally detected in 3.4µm, but no useful brightness estimate could be made.magphot.mag;em.IR.3-4um0.3910.83415.83517.67520.2290.999971floatindexednullablew1sigmrpo3.4µm profile-fit photometric measurement uncertainty in mag units. This column is null if the 3.4µm profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.magstat.error;phot.mag;em.IR.3-4um0.0020.0230.0610.2010.5430.990581floatnullablew1snr3.4µm profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w1flux) to flux uncertainty (w1sigflux)in the W1 profile-fit photometry measurement. This column is null if w1flux is negative, or if w1flux or w1sigflux are null.stat.snr;phot.mag;em.IR.3-4um-5404.95.317.546.55230.999971floatnullablew1rchi2Reduced χ² of the 3.4µm profile-fit photometry measurement. This column is null if the 3.4µm magnitude is a 95% confidence upper limit (i.e. the source is not detected).stat.fit.chi2;phot.mag;em.IR.3-4um0.0032450.77330.99513.78377580.999971floatnullablew1satSaturated pixel fraction, 3.4µm. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [3.4µm]~8 mag. Saturation may occur in fainter sources because of a charged particle strike.stat.fit.param00000.9790.999971floatnullablew1frtrFraction of pixels affected by transients. This column gives the fraction of all 3.4µm pixels in the stack of individual 3.4µm exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.000000.999971floatnullablew1cc_mapContamination and confusion map for this source in 3.4µmmeta.code.qual00.00.08.032251.0shortnullablew1mag3.4µm "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in 3.4µmmcor.magphot.mag;em.IR.3-4um6.01110.6715.44717.15326.7780.999971floatnullablew1sigmUncertainty in the 3.4µm "standard" aperture magnitude. This column is null if the 3.4µm "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.magstat.error;phot.mag;em.IR.3-4um0.0050.0070.1070.4180.5430.952702floatnullablew1flg3.4µm "standard" aperture measurement quality flag.meta.code.qual;phot.mag;em.IR.3-4um00.01.032.0320.99997085shortnullablew1mcor3.4µm aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness to give the "standard-aperture" magnitude.mag0.2610.2610.2610.2610.2610.999971floatnullablew1dmagDifference between maximum and minimum magnitude of the source from all usable single-exposure frames, 3.4µm. Single-exposure measurements with w1rchi2 values greater than 3.0 times the median are rejected from this computation.magphot.mag;em.IR.3-4um;arith.diff00.0990.9683.85813.4760.998432floatnullablew1ndfNumber of degrees of freedom in the flux variability chi-square, 3.4µm.stat.fit.dof;phot.mag;em.IR.3-4um09.014.048.03231.0shortnullablew1mlqProbability measure that the source is variable in 3.4µm flux.stat.fit.goodness;src.var00.00.02.090.99843174shortnullablew1mjdminThe earliest modified Julian Date (mJD) of the 3.4µm single-exposures covering the source.dtime.epoch;stat.min55203.155205.155280.255372.655411.20.999968floatnullablew1mjdmaxThe latest modified Julian Date (mJD) of the 3.4µm single-exposures covering the source.dtime.epoch;stat.max55203.555237.155311.555411.455414.40.999968floatnullablew1mjdmeanThe average modified Julian Date (mJD) of the 3.4µm single-exposures covering the source.dtime.epoch;stat.mean55203.355236.455304.855374.455413.80.999968floatnullablew1rsemiSemi-major axis of the elliptical aperture used to measure source in 3.4µmdegphys.angSize.smajAxis0.002269440.0024750.002822220.006352780.050.000877276floatnullablew1baAxis ratio (b/a) of the elliptical aperture used to measure source in 3.4µmphys.angSize;arith.ratio3.05556e-050.0001333330.0002166670.0002777780.0002777780.000877276floatnullablew1paPosition angle (degrees E of N) of the elliptical aperture major axis used to measure source in 3.4µmdegpos.posAng-89-805901170.000877276floatnullablew1gmag3.4µm magnitude of source measured in the elliptical aperture described by w1rsemi, w1w1ba, and w1w1pa.magphot.mag;em.IR.3-4um3.93810.72213.00314.0917.2620.000877255floatnullablew1gerrUncertainty in the 3.4µm magnitude of source measured in elliptical aperture.magstat.error;phot.mag;em.IR.3-4um0.0050.0060.010.0340.5730.000877255floatnullablew1gflgW1 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.meta.code;phot.mag;em.IR.3-4um00.01.01.0170.0008772547shortnullablew2mproMagnitude at 4.6µm measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the 4.6µm flux measurement has SNR<2. This column is null if the source is nominally detected in 4.6µm, but no useful brightness estimate could be made.magphot.mag;em.IR.4-8um-0.13610.88715.79417.27619.1340.999947floatindexednullablew2sigmrpo4.6µm profile-fit photometric measurement uncertainty in mag units. This column is null if the 4.6µm profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.magstat.error;phot.mag;em.IR.4-8um0.0010.0220.1270.4720.5430.835299floatnullablew2snr4.6µm profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w2flux) to flux uncertainty (w2sigflux)in the W1 profile-fit photometry measurement. This column is null if w2flux is negative, or if w2flux or w2sigflux are null.stat.snr;phot.mag;em.IR.4-8um-971.4-0.56.548.61131.30.999947floatnullablew2rchi2Reduced χ² of the 4.6µm profile-fit photometry measurement. This column is null if the 4.6µm magnitude is a 95% confidence upper limit (i.e. the source is not detected).stat.fit.chi2;phot.mag;em.IR.4-8um0.010810.81290.98261.99464570.999947floatnullablew2satSaturated pixel fraction, 4.6µm. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [4.6µm]~7 mag. Saturation may occur in fainter sources because of a charged particle strike.stat.fit.param00000.970.999947floatnullablew2frtrFraction of pixels affected by transients. This column gives the fraction of all 4.6µm pixels in the stack of individual 4.6µm exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.000000.999947floatnullablew2cc_mapContamination and confusion map for this source in 4.6µmmeta.code.qual00.00.08.032251.0shortnullablew2mag4.6µm "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in 4.6µmmcor.magphot.mag;em.IR.4-8um2.57510.6915.24216.47226.730.999947floatnullablew2sigmUncertainty in the 4.6µm "standard" aperture magnitude. This column is null if the 4.6µm "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.magstat.error;phot.mag;em.IR.4-8um0.0050.010.1780.4990.5430.753446floatnullablew2flg4.6µm "standard" aperture measurement quality flag.meta.code.qual;phot.mag;em.IR.4-8um00.01.032.0320.999947shortnullablew2mcor4.6µm aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness to give the "standard-aperture" magnitude.mag0.3190.3190.3190.3190.3190.999947floatnullablew2dmagDifference between maximum and minimum magnitude of the source from all usable single-exposure frames, 4.6µm. Single-exposure measurements with w2rchi2 values greater than 3.0 times the median are rejected from this computation.magphot.mag;em.IR.4-8um;arith.diff00.1392.2324.31411.7810.99835floatnullablew2ndfNumber of degrees of freedom in the flux variability chi-square, 4.6µm.stat.fit.dof;phot.mag;em.IR.4-8um05.012.043.03231.0shortnullablew2mlqProbability measure that the source is variable in 4.6µm flux.stat.fit.goodness;src.var00.00.02.090.99835014shortnullablew2mjdminThe earliest modified Julian Date (mJD) of the 4.6µm single-exposures covering the source.dtime.epoch;stat.min55203.155205.355280.455372.8554140.999945floatnullablew2mjdmaxThe latest modified Julian Date (mJD) of the 4.6µm single-exposures covering the source.dtime.epoch;stat.max55204.455237.155311.555411.455414.40.999945floatnullablew2mjdmeanThe average modified Julian Date (mJD) of the 4.6µm single-exposures covering the source.dtime.epoch;stat.mean55204.155236.455304.955374.755414.10.999945floatnullablew2rsemiSemi-major axis of the elliptical aperture used to measure source in 4.6µmdegphys.angSize.smajAxis0.002269440.0024750.002822220.006352780.050.000877265floatnullablew2baAxis ratio (b/a) of the elliptical aperture used to measure source in 4.6µmphys.angSize;arith.ratio3.05556e-050.0001333330.0002166670.0002777780.0002777780.000877265floatnullablew2paPosition angle (degrees E of N) of the elliptical aperture major axis used to measure source in 4.6µmdegpos.posAng-89-805901170.000877265floatnullablew2gmag4.6µm magnitude of source measured in the elliptical aperture described by w2rsemi, w2w1ba, and w2w1pa.magphot.mag;em.IR.4-8um2.81110.62412.93814.02518.3310.000877244floatnullablew2gerrUncertainty in the 4.6µm magnitude of source measured in elliptical aperture.magstat.error;phot.mag;em.IR.4-8um0.0050.0070.0210.0679.9990.000877244floatnullablew2gflgW1 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.meta.code;phot.mag;em.IR.4-8um00.01.01.0170.0008772443shortnullablew3mproMagnitude at 12µm measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the 12µm flux measurement has SNR<2. This column is null if the source is nominally detected in 12µm, but no useful brightness estimate could be made.magphot.mag;em.IR.8-15um-3.45110.24512.54513.40516.7980.999602floatindexednullablew3sigmrpo12µm profile-fit photometric measurement uncertainty in mag units. This column is null if the 12µm profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.magstat.error;phot.mag;em.IR.8-15um0.0020.0360.2560.5210.5430.301968floatnullablew3snr12µm profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w3flux) to flux uncertainty (w3sigflux)in the W1 profile-fit photometry measurement. This column is null if w3flux is negative, or if w3flux or w3sigflux are null.stat.snr;phot.mag;em.IR.8-15um-885.9-3.40.613.5500.30.9996floatnullablew3rchi2Reduced χ² of the 12µm profile-fit photometry measurement. This column is null if the 12µm magnitude is a 95% confidence upper limit (i.e. the source is not detected).stat.fit.chi2;phot.mag;em.IR.8-15um0.0055110.78010.96831.23580800.999602floatnullablew3satSaturated pixel fraction, 12µm. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [12µm]~4 mag. Saturation may occur in fainter sources because of a charged particle strike.stat.fit.param00000.9990.999604floatnullablew3frtrFraction of pixels affected by transients. This column gives the fraction of all 12µm pixels in the stack of individual 12µm exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.000000.999604floatnullablew3cc_mapContamination and confusion map for this source in 12µmmeta.code.qual00.00.011.034831.0shortnullablew3mag12µm "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in 12µmmcor.magphot.mag;em.IR.8-15um2.1869.12511.94112.97726.540.999604floatnullablew3sigmUncertainty in the 12µm "standard" aperture magnitude. This column is null if the 12µm "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.magstat.error;phot.mag;em.IR.8-15um0.0050.0320.3150.5290.5430.198894floatnullablew3flg12µm "standard" aperture measurement quality flag.meta.code.qual;phot.mag;em.IR.8-15um00.032.032.0320.9996036shortnullablew3mcor12µm aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness to give the "standard-aperture" magnitude.mag0.8250.8250.8250.8250.8250.999602floatnullablew3dmagDifference between maximum and minimum magnitude of the source from all usable single-exposure frames, 12µm. Single-exposure measurements with w3rchi2 values greater than 3.0 times the median are rejected from this computation.magphot.mag;em.IR.8-15um;arith.diff00.5832.9425.92913.9180.968691floatnullablew3ndfNumber of degrees of freedom in the flux variability chi-square, 12µm.stat.fit.dof;phot.mag;em.IR.8-15um00.08.031.02871.0shortnullablew3mlqProbability measure that the source is variable in 12µm flux.stat.fit.goodness;src.var00.00.02.090.96869093shortnullablew3mjdminThe earliest modified Julian Date (mJD) of the 12µm single-exposures covering the source.dtime.epoch;stat.min55203.155205.355280.75537355414.40.998463floatnullablew3mjdmaxThe latest modified Julian Date (mJD) of the 12µm single-exposures covering the source.dtime.epoch;stat.max55203.155237.155311.555411.355414.40.998463floatnullablew3mjdmeanThe average modified Julian Date (mJD) of the 12µm single-exposures covering the source.dtime.epoch;stat.mean55203.155236.355305.155374.955414.40.998463floatnullablew3rsemiSemi-major axis of the elliptical aperture used to measure source in 12µmdegphys.angSize.smajAxis0.002269440.0024750.002822220.006352780.050.000876931floatnullablew3baAxis ratio (b/a) of the elliptical aperture used to measure source in 12µmphys.angSize;arith.ratio3.05556e-050.0001333330.0002166670.0002777780.0002777780.000876931floatnullablew3paPosition angle (degrees E of N) of the elliptical aperture major axis used to measure source in 12µmdegpos.posAng-89-805901170.000876931floatnullablew3gmag12µm magnitude of source measured in the elliptical aperture described by w3rsemi, w3w1ba, and w3w1pa.magphot.mag;em.IR.8-15um-0.4747.9618311.15713.92220.4790.000863288floatnullablew3gerrUncertainty in the 12µm magnitude of source measured in elliptical aperture.magstat.error;phot.mag;em.IR.8-15um0.0050.0090.11.3989.9990.000863288floatnullablew3gflgW1 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.meta.code;phot.mag;em.IR.8-15um00.00.01.0210.00086328766shortnullablew4mproMagnitude at 22µm measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the 22µm flux measurement has SNR<2. This column is null if the source is nominally detected in 22µm, but no useful brightness estimate could be made.magphot.mag;em.IR.15-30um-7.8288.1119.0849.78710.9170.999777floatindexednullablew4sigmrpo22µm profile-fit photometric measurement uncertainty in mag units. This column is null if the 22µm profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.magstat.error;phot.mag;em.IR.15-30um00.070.3690.5330.5430.108262floatnullablew4snr22µm profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w4flux) to flux uncertainty (w4sigflux)in the W1 profile-fit photometry measurement. This column is null if w4flux is negative, or if w4flux or w4sigflux are null.stat.snr;phot.mag;em.IR.15-30um-1837.6-2.40.14.13287.70.999772floatnullablew4rchi2Reduced χ² of the 22µm profile-fit photometry measurement. This column is null if the 22µm magnitude is a 95% confidence upper limit (i.e. the source is not detected).stat.fit.chi2;phot.mag;em.IR.15-30um0.0058510.82650.99871.2351585000.999777floatnullablew4satSaturated pixel fraction, 22µm. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [22µm]~0 mag. Saturation may occur in fainter sources because of a charged particle strike.stat.fit.param0000.0030.9970.99978floatnullablew4frtrFraction of pixels affected by transients. This column gives the fraction of all 22µm pixels in the stack of individual 22µm exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.000000.99978floatnullablew4cc_mapContamination and confusion map for this source in 22µmmeta.code.qual00.00.00.034831.0shortnullablew4mag22µm "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in 22µmmcor.magphot.mag;em.IR.15-30um-2.2566.6098.4079.39223.890.99978floatnullablew4sigmUncertainty in the 22µm "standard" aperture magnitude. This column is null if the 22µm "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.magstat.error;phot.mag;em.IR.15-30um0.0050.0410.3640.5340.5430.0797683floatnullablew4flg22µm "standard" aperture measurement quality flag.meta.code.qual;phot.mag;em.IR.15-30um01.032.032.0320.9997805shortnullablew4mcor22µm aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness to give the "standard-aperture" magnitude.mag0.5760.5760.5760.5760.5760.99978floatnullablew4dmagDifference between maximum and minimum magnitude of the source from all usable single-exposure frames, 22µm. Single-exposure measurements with w4rchi2 values greater than 3.0 times the median are rejected from this computation.magphot.mag;em.IR.15-30um;arith.diff00.8022.9275.0713.1790.983901floatnullablew4ndfNumber of degrees of freedom in the flux variability chi-square, 22µm.stat.fit.dof;phot.mag;em.IR.15-30um01.07.026.02551.0shortnullablew4mlqProbability measure that the source is variable in 22µm flux.stat.fit.goodness;src.var00.00.01.090.9839008shortnullablew4mjdminThe earliest modified Julian Date (mJD) of the 22µm single-exposures covering the source.dtime.epoch;stat.min55203.155205.355280.655372.855414.30.999734floatnullablew4mjdmaxThe latest modified Julian Date (mJD) of the 22µm single-exposures covering the source.dtime.epoch;stat.max55204.955237.155311.555411.355414.40.999734floatnullablew4mjdmeanThe average modified Julian Date (mJD) of the 22µm single-exposures covering the source.dtime.epoch;stat.mean55204.955236.455305.155374.755414.30.999734floatnullablew4rsemiSemi-major axis of the elliptical aperture used to measure source in 22µmdegphys.angSize.smajAxis0.003719440.003961110.004488890.007877780.050.000877161floatnullablew4baAxis ratio (b/a) of the elliptical aperture used to measure source in 22µmphys.angSize;arith.ratio3.33333e-050.0001861110.0002527780.0002777780.0002777780.000877161floatnullablew4paPosition angle (degrees E of N) of the elliptical aperture major axis used to measure source in 22µmdegpos.posAng-89-805901170.000877161floatnullablew4gmag22µm magnitude of source measured in the elliptical aperture described by w4rsemi, w4w1ba, and w4w1pa.magphot.mag;em.IR.15-30um-4.7255.66639.06412.290923.1750.000743425floatnullablew4gerrUncertainty in the 22µm magnitude of source measured in elliptical aperture.magstat.error;phot.mag;em.IR.15-30um0.0050.0260.4498.74479.9990.000743425floatnullablew4gflgW1 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.meta.code;phot.mag;em.IR.15-30um01.01.017.0210.0007434254shortnullablerchi2Combined reduced χ² of the profile-fit photometry measurement in all bands.stat.fit.chi2;phot.mag0.085860.8790.98722.047138401floatnullablenbNumber of PSF components used simultaneously in the profile-fitting for this source. This is greater than "1" when the source is fit concurrently with other nearby detections (passive deblending), or when a single source is split into two components during the fitting process (active deblending).meta.number;stat.fit11.01.02.041.0shortnullablenaActive deblending flag. Indicates if a single detection was split into multiple sources in the process of profile-fitting.meta.code.qual00.00.01.011.0shortnullablesatnumMinimum sample at which saturation occurs in each band. Four character string, one character per band, that indicates the minimum SUTR sample in which any pixel in the profile-fitting area in all of the single-exposure images used to characterize this source was flagged as having reached the saturation level in the on-board WISE payload processing. If no pixels in a given band are flagged as saturated, the value for that band is '0'.meta.code.qualcharnullablecc_flagsContamination and confusion flag.meta.code.qualcharnullableext_flgExtended source flag.meta.code;src.class00.00.01.051.0shortnullablevar_flgVariability flag.meta.code;src.varcharnullableph_qualPhotometric quality flag.meta.code.qual;phot.magcharnullabledet_bitBit-encoded integer indicating bands in which a source has a w?snr>2 detection. For example, a source detected in W1 only has det_bit=1 (binary 0001). A source detected in W4 only has det_bit=8 (binary 1000). A source detected in all four bands has det_bit=15 (binary 1111).meta.code.qual11.03.015.0151.0shortq12Correlation significance between 3.4µm and 4.6µm.stat.fit.goodness00.00.02.090.9948195shortnullableq23Correlation significance between 4.6µm and 12µm.stat.fit.goodness00.00.01.090.9449299shortnullableq34Correlation significance between 12µm and 22µm.stat.fit.goodness00.00.01.090.8521096shortnullablexscprox2MASS Extended Source Catalog (XSC) proximity. This column gives the distance between the WISE source position and the position of a nearby 2MASS XSC source, if the separation is less than 1.1 times the Ks isophotal radius size of the XSC source. This identifies WISE sources that are identically the 2MASS XSC source as well as WISE sources that are fragments of large galaxies.deg04.16667e-050.0002833330.03846940.4930470.0014936floatnullabletmass_key2MASS PSC association. Unique identifier of the closest source in the 2MASS Point Source Catalog (PSC) that falls within 3" of the position of this WISE source. You can use this join to towmass.data, the pts_key column there.meta.id.cross7742572992.42629770570.01302036817.2813400366600.49788675longnullablearigfhARI's "Geschichte des Fixsternhimmels" is an attempt to collect all astrometrically useful observations from before ca. 1970 in a way comparable to what has been done to construct the FK* series of fundamental catalogs. About 7e6 published positions are included. In GAVO's DC, we provide tables of identified and non-identified stars together with the master catalog that objects were identified against.arigfh.gfhThe table of (almost) all objects read from the catalogs, together with most of the data given in them.7100000catidCatalog identifier as t(teleki no)p(part)(version)meta.refcharindexednullablecatanObject number in source catalog, ARI assignedmeta.id0140.019121.0721109.879999999910583321.0intindexedcatcnObject number in source catalog, as in sourcemeta.id-6198.0124472.0808800875.249535000921.0intcatcaSuffix to the designation in the source catalogmeta.idcharnullabledscodeCode for multiple star component designationmeta.code.multip00.00.00.030001.0shortmagApparent magnitude as specified by magsysphot.mag-6.45912900.934445floatnullablemagsysSystem of magmeta.code;phot.magcharnullablevarflagCode for photometric variabilitymeta.code;src.var00.00.00.091.0shortracatRight ascension at catalog equinox and epochdegpos.eq.ra-57290011.6374185.732348.229361.1850.999992doubleindexednullableeqraEquinox of the catalog RA, Julian yearsyrtime.equinox;pos.eq.ra1690.0118351950200020001floatnullableepraEpoch of the catalog RA, Julian yearsyrtime.epoch;pos.eq.ra1100.121837.481968.7520009913.970.983827floatnullablemeanepraMean Epoch of RA, Julian yearsyrtime.epoch1100.121833.21954.81993.419913.970.946414floatnullablee_raMean error in right ascension as given in catalogdegstat.error;pos.eq.ra;meta.main02.09983e-071.11357e-056.77557e-051914.370.369457floatnullablenobraNumber of observations combined into raCatmeta.number;obs0141518540.581092floatnullableusera0=RA unusable, 1=RA usable, 2=RA good, but epoch guessedmeta.code;pos.eq.ra01.01.01.020.9997047shortnullableraflagsDetails on observation and processing of RA (see note)meta.code;pos.eq.ra01000.01010.04910.0411101.0intdeccatDeclination at catalog equinox and epochdegpos.eq.dec-572900-68.59330.74196970.294900.999862doubleindexednullableeqdecEquinox of the catalog declination, Julian yearsyrtime.equinox;pos.eq.dec1690.0118351950200020000.999999floatnullableepdecEpoch of the catalog declination, Julian yearsyrtime.epoch;pos.eq.dec1092.721840.41968.8920009913.970.980308floatnullablemeanepdecMean Epoch of the declination, Julian yearsyrtime.epoch1092.721838.341954.741993.429913.970.94265floatnullablee_decMean error in declination as given in catalogdegstat.error;pos.eq.dec;meta.main02.13889e-071.38889e-058.61111e-050.001388890.36618floatnullablenobdecNumber of observations combined into decCatmeta.number;obs0141425000.57497floatnullableusedec0=Dec unusable, 1=Dec usable, 2=Dec good, but epoch guessedmeta.code;pos.eq.dec01.01.01.020.9997047shortnullabledecflagsDetails on observation and processing of dec (see note)meta.code;pos.eq.dec-88881000.01010.04910.0411101.0intpmraCat. proper motion in RAdeg/yrpos.pm;pos.eq.ra-0.0465511-2.85502e-05-3.84422e-072.78071e-050.1097470.621641floatnullableeqpmraEquinox of cat. PM in RAyrtime.equinox;pos.pm;pos.eq.ra175019002000200020000.621634floatnullableeppmraEpoch of cat. PM in RAyrtime.epoch;pos.pm;pos.eq.ra183019501991.25200020000.297734floatnullablee_pmraMean error in the proper motion in RA according to the catalogdeg/yrstat.error;pos.pm;pos.eq.ra-3.77963e-0701.15303e-061.48256e-054.16007e-050.454047floatnullablenobpmraNumber of observations combined into the proper motion in RAmeta.number;obs02310400.083445floatnullablepmraflagType of PM RA; see notemeta.code;pos.pm;pos.eq.ra00.00.01.020.6216411shortnullablepmdeCat. proper motion in declinationdeg/yrpos.pm;pos.eq.dec-0.0122874-2.86041e-05-1.19157e-061.61161e-050.007377550.621822floatnullableeqpmdeEquinox of cat. PM in Decyrtime.equinox;pos.pm;pos.eq.dec175019002000200020000.621692floatnullableeppmdeEpoch of cat. PM in declinationyrtime.epoch;pos.pm;pos.eq.dec183019501991.25200020000.297667floatnullablee_pmdeMean error in the proper motion in Dec according to the catalogdeg/yrstat.error;pos.pm;pos.eq.dec001.38886e-061.51389e-054.15556e-050.453225floatnullablenobpmdeNumber of observations combined into the proper motion in Declinationmeta.number;obs02310440.0833426floatnullablepmdeflagType of PM Dec; see notemeta.code;pos.pm;pos.eq.dec00.00.00.020.62182224shortnullablearigfh.id The stars from the gfh table having counterparts in the master catalog, together with those counterparts.masternoIdentification number in the ARIGFH master catalogmeta.id;meta.main118379.78306314.0594248.226126271.0intcompmasterComponent designation in a multiple system in the master catalogmeta.code.multipcharnullableraj2000Master Right Ascension, Epoch and Equinox J2000degpos.eq.ra;meta.main0.00039583313.6315182.142346.777359.9991doublenullabledej2000Master Declination, Epoch and Equinox J2000degpos.eq.dec;meta.main-89.8775-71.2833-11.209367.227989.77411doublenullablepmramasterMaster Proper Motion in RA, Epoch and Equinox J2000, cos(delta) applieddeg/yrpos.pm;pos.eq.ra-0.00227744-3.04167e-05-8.33333e-072.875e-050.002788330.806293doublenullablepmdemasterMaster Proper motion in Declination, Epoch and Equinox J2000deg/yrpos.pm;pos.eq.dec-0.00161472-2.27778e-05-1.38889e-061e-050.0028550.806293doublenullablemvmasterVisual magnitude in the master catalogmagphot.mag;em.opt.V-1.66.8689.510.9210.710636floatnullablembmasterBlue magnitude in the master catalogmagphot.mag;em.opt.B-0.5727.19.911.766817.30.464018floatnullablecatidCatalog identifier as t(teleki no)p(part)(version)meta.refcharnullablecatanObject number in source catalog, ARI assignedmeta.id0140.019121.0721109.879999999910583321.0intdistOffset between master catalog position at catalog epoch and equinox and the catalog positiondegpos.angDistance02.77459e-090.000177580.001315280.1207561doublenullableiqQuality of match, quality decreasing with values increasing from 2meta.code.qual-5-2.02.03.0111.0shortcatcnObject number in source catalog, as in sourcemeta.id-6198.0124472.0808800875.249535000921.0intcatcaSuffix to the designation in the source catalogmeta.idcharnullabledscodeCode for multiple star component designationmeta.code.multip00.00.00.030001.0shortmagApparent magnitude as specified by magsysphot.mag-6.45912900.934445floatnullablemagsysSystem of magmeta.code;phot.magcharnullablevarflagCode for photometric variabilitymeta.code;src.var00.00.00.091.0shortracatRight ascension at catalog equinox and epochdegpos.eq.ra-57290011.6374185.732348.229361.1850.999992doublenullableeqraEquinox of the catalog RA, Julian yearsyrtime.equinox;pos.eq.ra1690.0118351950200020001floatnullableepraEpoch of the catalog RA, Julian yearsyrtime.epoch;pos.eq.ra1100.121837.481968.7520009913.970.983827floatnullablemeanepraMean Epoch of RA, Julian yearsyrtime.epoch1100.121833.21954.81993.419913.970.946414floatnullablee_raMean error in right ascension as given in catalogdegstat.error;pos.eq.ra;meta.main02.09983e-071.11357e-056.77557e-051914.370.369457floatnullablenobraNumber of observations combined into raCatmeta.number;obs0141518540.581092floatnullableusera0=RA unusable, 1=RA usable, 2=RA good, but epoch guessedmeta.code;pos.eq.ra01.01.01.020.9997047shortnullableraflagsDetails on observation and processing of RA (see note)meta.code;pos.eq.ra01000.01010.04910.0411101.0intdeccatDeclination at catalog equinox and epochdegpos.eq.dec-572900-68.59330.74196970.294900.999862doublenullableeqdecEquinox of the catalog declination, Julian yearsyrtime.equinox;pos.eq.dec1690.0118351950200020000.999999floatnullableepdecEpoch of the catalog declination, Julian yearsyrtime.epoch;pos.eq.dec1092.721840.41968.8920009913.970.980308floatnullablemeanepdecMean Epoch of the declination, Julian yearsyrtime.epoch1092.721838.341954.741993.429913.970.94265floatnullablee_decMean error in declination as given in catalogdegstat.error;pos.eq.dec;meta.main02.13889e-071.38889e-058.61111e-050.001388890.36618floatnullablenobdecNumber of observations combined into decCatmeta.number;obs0141425000.57497floatnullableusedec0=Dec unusable, 1=Dec usable, 2=Dec good, but epoch guessedmeta.code;pos.eq.dec01.01.01.020.9997047shortnullabledecflagsDetails on observation and processing of dec (see note)meta.code;pos.eq.dec-88881000.01010.04910.0411101.0intpmraCat. proper motion in RAdeg/yrpos.pm;pos.eq.ra-0.0465511-2.85502e-05-3.84422e-072.78071e-050.1097470.621641floatnullableeqpmraEquinox of cat. PM in RAyrtime.equinox;pos.pm;pos.eq.ra175019002000200020000.621634floatnullableeppmraEpoch of cat. PM in RAyrtime.epoch;pos.pm;pos.eq.ra183019501991.25200020000.297734floatnullablee_pmraMean error in the proper motion in RA according to the catalogdeg/yrstat.error;pos.pm;pos.eq.ra-3.77963e-0701.15303e-061.48256e-054.16007e-050.454047floatnullablenobpmraNumber of observations combined into the proper motion in RAmeta.number;obs02310400.083445floatnullablepmraflagType of PM RA; see notemeta.code;pos.pm;pos.eq.ra00.00.01.020.6216411shortnullablepmdeCat. proper motion in declinationdeg/yrpos.pm;pos.eq.dec-0.0122874-2.86041e-05-1.19157e-061.61161e-050.007377550.621822floatnullableeqpmdeEquinox of cat. PM in Decyrtime.equinox;pos.pm;pos.eq.dec175019002000200020000.621692floatnullableeppmdeEpoch of cat. PM in declinationyrtime.epoch;pos.pm;pos.eq.dec183019501991.25200020000.297667floatnullablee_pmdeMean error in the proper motion in Dec according to the catalogdeg/yrstat.error;pos.pm;pos.eq.dec001.38886e-061.51389e-054.15556e-050.453225floatnullablenobpmdeNumber of observations combined into the proper motion in Declinationmeta.number;obs02310440.0833426floatnullablepmdeflagType of PM Dec; see notemeta.code;pos.pm;pos.eq.dec00.00.00.020.62182224shortnullablearigfh.nid The stars from the gfh table that could not be matched with objects in the master catalog.catidCatalog identifier as t(teleki no)p(part)(version)meta.refcharnullablecatanObject number in source catalog, ARI assignedmeta.id0140.019121.0721109.879999999910583321.0intcatcnObject number in source catalog, as in sourcemeta.id-6198.0124472.0808800875.249535000921.0intcatcaSuffix to the designation in the source catalogmeta.idcharnullabledscodeCode for multiple star component designationmeta.code.multip00.00.00.030001.0shortmagApparent magnitude as specified by magsysphot.mag-6.45912900.934445floatnullablemagsysSystem of magmeta.code;phot.magcharnullablevarflagCode for photometric variabilitymeta.code;src.var00.00.00.091.0shortracatRight ascension at catalog equinox and epochdegpos.eq.ra-57290011.6374185.732348.229361.1850.999992doublenullableeqraEquinox of the catalog RA, Julian yearsyrtime.equinox;pos.eq.ra1690.0118351950200020001floatnullableepraEpoch of the catalog RA, Julian yearsyrtime.epoch;pos.eq.ra1100.121837.481968.7520009913.970.983827floatnullablemeanepraMean Epoch of RA, Julian yearsyrtime.epoch1100.121833.21954.81993.419913.970.946414floatnullablee_raMean error in right ascension as given in catalogdegstat.error;pos.eq.ra;meta.main02.09983e-071.11357e-056.77557e-051914.370.369457floatnullablenobraNumber of observations combined into raCatmeta.number;obs0141518540.581092floatnullableusera0=RA unusable, 1=RA usable, 2=RA good, but epoch guessedmeta.code;pos.eq.ra01.01.01.020.9997047shortnullableraflagsDetails on observation and processing of RA (see note)meta.code;pos.eq.ra01000.01010.04910.0411101.0intdeccatDeclination at catalog equinox and epochdegpos.eq.dec-572900-68.59330.74196970.294900.999862doublenullableeqdecEquinox of the catalog declination, Julian yearsyrtime.equinox;pos.eq.dec1690.0118351950200020000.999999floatnullableepdecEpoch of the catalog declination, Julian yearsyrtime.epoch;pos.eq.dec1092.721840.41968.8920009913.970.980308floatnullablemeanepdecMean Epoch of the declination, Julian yearsyrtime.epoch1092.721838.341954.741993.429913.970.94265floatnullablee_decMean error in declination as given in catalogdegstat.error;pos.eq.dec;meta.main02.13889e-071.38889e-058.61111e-050.001388890.36618floatnullablenobdecNumber of observations combined into decCatmeta.number;obs0141425000.57497floatnullableusedec0=Dec unusable, 1=Dec usable, 2=Dec good, but epoch guessedmeta.code;pos.eq.dec01.01.01.020.9997047shortnullabledecflagsDetails on observation and processing of dec (see note)meta.code;pos.eq.dec-88881000.01010.04910.0411101.0intpmraCat. proper motion in RAdeg/yrpos.pm;pos.eq.ra-0.0465511-2.85502e-05-3.84422e-072.78071e-050.1097470.621641floatnullableeqpmraEquinox of cat. PM in RAyrtime.equinox;pos.pm;pos.eq.ra175019002000200020000.621634floatnullableeppmraEpoch of cat. PM in RAyrtime.epoch;pos.pm;pos.eq.ra183019501991.25200020000.297734floatnullablee_pmraMean error in the proper motion in RA according to the catalogdeg/yrstat.error;pos.pm;pos.eq.ra-3.77963e-0701.15303e-061.48256e-054.16007e-050.454047floatnullablenobpmraNumber of observations combined into the proper motion in RAmeta.number;obs02310400.083445floatnullablepmraflagType of PM RA; see notemeta.code;pos.pm;pos.eq.ra00.00.01.020.6216411shortnullablepmdeCat. proper motion in declinationdeg/yrpos.pm;pos.eq.dec-0.0122874-2.86041e-05-1.19157e-061.61161e-050.007377550.621822floatnullableeqpmdeEquinox of cat. PM in Decyrtime.equinox;pos.pm;pos.eq.dec175019002000200020000.621692floatnullableeppmdeEpoch of cat. PM in declinationyrtime.epoch;pos.pm;pos.eq.dec183019501991.25200020000.297667floatnullablee_pmdeMean error in the proper motion in Dec according to the catalogdeg/yrstat.error;pos.pm;pos.eq.dec001.38886e-061.51389e-054.15556e-050.453225floatnullablenobpmdeNumber of observations combined into the proper motion in Declinationmeta.number;obs02310440.0833426floatnullablepmdeflagType of PM Dec; see notemeta.code;pos.pm;pos.eq.dec00.00.00.020.62182224shortnullablearigfh.masterThe master catalog against which all ARIGFH historical observations were matched.612627catnoIdentification number in the ARIGFH master catalogmeta.id;meta.main118379.78306314.0594248.226126271.0intindexedprimaryraj2000Master Right Ascension, Epoch and Equinox J2000degpos.eq.ra;meta.main0.00039583313.6315182.142346.777359.9991doubleindexednullabledej2000Master Declination, Epoch and Equinox J2000degpos.eq.dec;meta.main-89.8775-71.2833-11.209367.227989.77411doubleindexednullablepmraMaster Proper Motion in RA, Epoch and Equinox J2000, cos(delta) applieddeg/yrpos.pm;pos.eq.ra-0.00227744-3.04167e-05-8.33333e-072.875e-050.002788330.806293doublenullablepmdeMaster Proper motion in Declination, Epoch and Equinox J2000deg/yrpos.pm;pos.eq.dec-0.00161472-2.27778e-05-1.38889e-061e-050.0028550.806293doublenullablemvVisual magnitude in the master catalogmagphot.mag;em.opt.V-1.66.8689.510.9210.710636floatnullablembBlue magnitude in the master catalogmagphot.mag;em.opt.B-0.5727.19.911.766817.30.464018floatnullablecomponentComponent designation in a multiple system in the master catalogmeta.code.multipcharnullablearigfh.identifiedMatches between the master catalog and the historical catalogs.6300000distOffset between master catalog position at catalog epoch and equinox and the catalog positiondegpos.angDistance02.77459e-090.000177580.001315280.1207561doublenullablemasternoCatalog number in master catalog (arigfh.master)meta.id;meta.main014621.0259081.0509650.06126261.0intindexeddcompComponent designation for multiple system, as in the master catalogmeta.code.multipcharnullableiqQuality of match, quality decreasing with values increasing from 2meta.code.qual-5-2.02.03.0111.0shortcsortCatalog typemeta.code-9000-1000.0-10.0-2.031.0shortcatidCatalog designation as in arigfh.katkatmeta.id.crosscharindexedcatanObject number in source catalog, ARI assignedmeta.id0140.019121.0721109.879999999910583321.0intindexedarigfh.unidentifiedThe objects in the gfh table that could not be matched with objects in the master catalog by ARIGFH.872720catanObject number in source catalog, ARI assignedmeta.id0140.019121.0721109.879999999910583321.0intindexedcatidCatalog designation as in arigfh.katkatmeta.id.crosscharindexedcarsarcs Candidate gravitational arcs in the 37 deg^2 of CFHTLS-Archive-Research Survey (CARS). The data include their post-stamp images, astrometry, photometry (u*,g',r',i'), geometric properties (length, length-to-width ratio, profile curvature, area), and photometric redshifts. The arc candidates were selected booth with an automatic arcfinder, based on a tailored image segmentation and a color selection, and by visually inspecting the survey.carsarcs.meta Candidate gravitational arcs in the 37 deg^2 of CFHTLS-Archive-Research Survey (CARS). The data include their post-stamp images, astrometry, photometry (u*,g',r',i'), geometric properties (length, length-to-width ratio, profile curvature, area), and photometric redshifts. The arc candidates were selected booth with an automatic arcfinder, based on a tailored image segmentation and a color selection, and by visually inspecting the survey.90previewPreview imagemeta.ref.urlcharnullablematidIdentification number within carsarcsmeta.id;meta.maincharnullablecarsfieldCARS field identifiermeta.id;obs.fieldcharnullableraj2000Right ascension of the center, ICRSdegpos.eq.ra;meta.main33.131733.3137.466335.447335.5961doubleindexednullabledej2000Declination of the center, ICRSdegpos.eq.dec;meta.main-7.71944-6.56511-4.0606952.895453.03581doubleindexednullablearc_lengthLength of the arc (see paper for construction).degphys.angSize;src0.0003666670.0004315560.0009194440.00220550.0025251floatnullablearc_l_wLength to width ratio for the arc (see paper for construction).phys.size;arith.ratio1.481.98013.729.169213.81floatnullablearc_curvCurvature of the arc (see paper for construction).deg**-1src.morph.param009003191.439601floatnullablearc_areaArea of the arc (see paper for construction).deg**2phys.angSize;src7.71605e-088.23302e-082.62346e-078.51312e-071.00309e-061floatnullableuprimearc u' aperture magnitude (based on segmentation)magphot.mag;em.opt.U22.623.06724.625.86527.41floatnullableerr_uprimeError in u magnitude; estimated by image noise including background subtraction uncertainty.magstat.error;phot.mag;em.opt.U0.20.20.41.1663.61floatnullablegprimearc g' aperture magnitude (based on segmentation)magphot.mag;em.opt.V22.122.323.524.76625.41floatnullableerr_gprimeError in g magnitude; estimated by image noise including background subtraction uncertainty.magstat.error;phot.mag;em.opt.V0.10.10.10.3330.51floatnullablerprimearc r' aperture magnitude (based on segmentation)magphot.mag;em.opt.R021.23422.8523.924.91floatnullableerr_rprimeError in r magnitude; estimated by image noise including background subtraction uncertainty.magstat.error;phot.mag;em.opt.R00.10.20.63311floatnullableiprimearc i' aperture magnitude (based on segmentation)magphot.mag;em.opt.I20.420.52223.33324.41floatnullableerr_iprimeError in i magnitude; estimated by image noise including background subtraction uncertainty.magstat.error;phot.mag;em.opt.I0.10.10.10.30.81floatnullablez_lensPhotometric redshift of the lens (from CARS catalog).src.redshift.phot0.260.28670.5050.78320.821floatnullablez_lens_err_plusLens photometric redshift 1-sigma error taken from the CARS catalog.stat.error;src.redshift.phot-0.24-0.21-0.1-0.08-0.081floatnullablez_lens_err_minusLens photometric redshift 1-sigma error taken from the CARS catalog.stat.error;src.redshift.phot0.080.090.10.220.231floatnullablequal_assQuality assessmentmeta.code.qual12.02.03.031.0shortnullablecatnrCatalog number of previously known arcsmeta.id.crosscharnullableimg_uCARS image in the u band.meta.ref.urlcharnullableimg_gCARS image in the g band.meta.ref.urlcharnullableimg_rCARS image in the r band.meta.ref.urlcharnullableimg_iCARS image in the i band.meta.ref.urlcharnullablecns5update The Fifth Catalogue of Nearby Stars (CNS5) aims to provide the most volume-complete sample of stars in the solar neighbourhood. This is a continuously-updated version of the published CNS5 (:bibcode:`2023A&A...670A..19G`). The CNS5 is compiled based on trigonometric parallaxes from Gaia DR3 and Hipparcos, and supplemented with astrometric data from Spitzer and ground-based surveys carried out in the infrared. The CNS5 catalogue is statistically complete down to 19.7 mag in G-band and 11.8 mag in W1-band absolute magnitudes, corresponding to a spectral type of L8. Continuous updates of observational data for nearby stars from all sources were collected and evaluated. For all known stars in the 25 pc sphere around the Sun, the best values of positions in space, velocities, and magnitudes in different filters are presented.cns5update.main The Fifth Catalogue of Nearby Stars (CNS5) aims to provide the most volume-complete sample of stars in the solar neighbourhood. This is a continuously-updated version of the published CNS5 (:bibcode:`2023A&A...670A..19G`). The CNS5 is compiled based on trigonometric parallaxes from Gaia DR3 and Hipparcos, and supplemented with astrometric data from Spitzer and ground-based surveys carried out in the infrared. The CNS5 catalogue is statistically complete down to 19.7 mag in G-band and 11.8 mag in W1-band absolute magnitudes, corresponding to a spectral type of L8. Continuous updates of observational data for nearby stars from all sources were collected and evaluated. For all known stars in the 25 pc sphere around the Sun, the best values of positions in space, velocities, and magnitudes in different filters are presented.6322cns5_idCNS5 designationmeta.id;meta.main0190.633172.56252.3764421.0longgj_idGliese-Jahreiss numbermeta.id.crosscharnullablecomponent_idDesignation of component(s) in binaries or multiple systems. This may consist of several letters if a catalogue entry corresponds to more than one component that is not split into individual entries.meta.code.multipcharnullablen_componentsTotal number of components in the systemmeta.number11.01.03.061.0shortnullableprimary_flagTrue for the primary of a multiple systemmeta.code00.01.01.011.0shortnullablegj_system_primaryGliese-Jahriess number of the primary component of the systemmeta.id.crosscharnullablegaia_dr3_idSource identifier in Gaia DR3meta.id.cross3688766613886652.352635511410039e+173.4744531918358067e+186.70472999817661e+1869169296606617262080.8421386longnullablehip_idHipparcos identifiermeta.id.cross1692292.799999999999360866.0114951.61200050.2500791intnullableraRight ascensiondegpos.eq.ra;meta.main0.0563389.37084181.402349.852359.9680.998576doublenullabledecDeclinationdegpos.eq.dec;meta.main-87.7648-69.5081-0.17551770.435288.40560.998576doublenullableepochReference epoch for coordinatesyrtime.epoch1991.252000201620162020.380.998576doublenullablecoordinates_bibcodeSource of the positionmeta.bib;pos.eqcharnullableparallaxAbsolute trigonometric parallaxmaspos.parallax.trig1739.874650.7818156.775768.0670.998576doublenullableparallax_errorError in parallaxmasstat.error;pos.parallax.trig0.01086980.0163160.03792443.564100.998576floatnullableparallax_bibcodeSource of the parallaxmeta.bib;pos.parallax.trigcharnullablepmraProper motion in right ascensionmas/yrpos.pm;pos.eq.ra-8123.7-901.3226.06277961.13367660.998576doublenullablepmra_errorError in pmramas/yrstat.error;pos.pm;pos.eq.ra0.006817220.01323140.03412072.930.70.998418doublenullablepmdecProper motion in declinationmas/yrpos.pm;pos.eq.dec-5817.8-1071.9-118.394507.84110362.40.998576doublenullablepmdec_errorError of pmdecmas/yrstat.error;pos.pm;pos.eq.dec0.008305350.01356030.02983572.72500.998418doublenullablepm_bibcodeSource of the proper motionmeta.bib;pos.pmcharnullablervSpectroscopic radial velocitykm/sphys.veloc;pos.barycenter-266.369-61.63171.2488867.09482873440.774913doublenullablerv_errorError in rvkm/sstat.error;phys.veloc;pos.barycenter0.00010.070.3561796.89527400.764631doublenullablerv_bibcodeSource of the radial velocitymeta.bib;phys.veloc;pos.barycentercharnullableg_magG band mean magnitude (corrected)magphot.mag;em.opt1.731614.9457912.086218.645820.95810.836444floatnullableg_mag_errorError in g_magmagstat.error;phot.mag;em.opt9.42095e-050.0001854270.000583760.005205440.04137220.836444doublenullablebp_magGaia DR3 integrated BP mean magnitudemagphot.mag;em.opt.b2.469125.2296613.467821.182322.82370.822841floatnullablebp_mag_errorError in bp_magmagstat.error;phot.mag;em.opt.b0.0001612970.0005192660.002064620.1645341.16550.822841doublenullablerp_magGaia DR3 integrated RP mean magnitudemagphot.mag;em.opt.r1.900764.4435810.832317.012419.29880.824264floatnullablerp_mag_errorError in rp_magmagstat.error;phot.mag;em.opt.r0.0001698880.0003449280.0009951780.02233160.7189210.819994doublenullableg_mag_from_hipHipparcos Hp magnitude converted to the G bandmagphot.mag;em.opt-1.063530.1177386.9059810.506411.32290.0216704doublenullableg_mag_from_hip_errorError in g_mag_from_hipmagstat.error;phot.mag;em.opt0.081910.0819110.08192980.08241680.09453620.0218285doublenullableg_rp_from_hipG - RP colour computed from Hipparcos V and Imagphot.color;em.opt.r;em.opt-0.05560640.03711370.672011.215571.248370.0216704doublenullableg_rp_from_hip_errorError in g_rp_from_hipmagstat.error;phot.color;em.opt.r;em.opt0.131130.1311310.1311540.1317630.1471420.0218285doublenullableg_mag_resultingResulting (e.g., deblended) G band magnitudemagphot.mag;em.opt-26.94.7209912.042418.610420.95810.848782floatnullableg_mag_resulting_errorError in g_mag_resultingmagstat.error;phot.mag;em.opt9.42095e-050.000186130.0005909090.01105380.09453620.848782doublenullableg_rp_resultingResulting (e.g., deblended) G - RP colourmagphot.color;em.opt.r;em.opt-0.2315030.3437771.176581.603633.696930.831224doublenullableg_rp_resulting_errorError in g_rp_resultingmagstat.error;phot.color;em.opt.r;em.opt0.00051780.001427620.00268870.08645450.7189290.831066doublenullableg_rp_resulting_flag0 – G-RP is deblended; 1 – G-RP is uncorrected vs. DR3; 2 – G-RP is converted from Hipparcosmeta.code;phot.mag00.00.01.020.8312243shortnullablej_mag2MASS J band magnitudemagphot.mag;em.ir.j-27.93.906049.37416.34325.420.821417floatnullablej_mag_errorError in j_magmagstat.error;phot.mag;em.ir.j0.010.0180.0240.260.9960.821259floatnullableh_mag2MASS H band magnitudemagphot.mag;em.ir.h-28.253.526718.768515.37925.290.807339floatnullableh_mag_errorError in h_magmagstat.error;phot.mag;em.ir.h0.0150.0170.0280.2281.0720.807181floatnullablek_mag2MASS Ks band magnitudemagphot.mag;em.ir.k-28.33.619648.50614.843618.9040.796109floatnullablek_mag_errorError in k_magmagstat.error;phot.mag;em.ir.k0.0120.0160.0220.2480.490.795951floatnullablejhk_mag_bibcodeSource of NIR magnitudesmeta.bib;phot.mag;em.ircharnullablew1_magWISE W1 band magnitudemagphot.mag;em.ir.3-4um-28.314.940668.68716.8719.3320.662449floatnullablew1_mag_errorError in w1_magmagstat.error;phot.mag;em.ir.3-4um0.020.0220.0250.248420.5340.66229floatnullablew2_magWISE W2 band magnitudemagphot.mag;em.ir.4-8um-28.294.653648.529514.860417.6830.671939floatnullablew2_mag_errorError in w2_magmagstat.error;phot.mag;em.ir.4-8um0.0170.0190.0210.116620.5170.671781floatnullablew3_magWISE W3 band magnitudemagphot.mag;em.ir.8-15um-28.314.698.11612.159813.4220.613888floatnullablew3_mag_errorError in w3_magmagstat.error;phot.mag;em.ir.8-15um0.0070.0140.0210.3310.5350.61373floatnullablew4_magWISE W4 band magnitudemagphot.mag;em.ir.15-30um-28.34.071357.30359.02210.1840.447643floatnullablew4_mag_errorError in w4_magmagstat.error;phot.mag;em.ir.15-30um0.0090.0240.110.4830.5420.447485floatnullablewise_mag_bibcodeSource of MIR magnitudesmeta.bib;phot.mag;em.ircharnullablep_rotRotational period taken from p_rot_bibcode.dtime.period0.009000010.1773876.95826125.025191.8280.283455floatnullablep_rot_errorError on p_rotdstat.error;time.period2e-086e-050.066.271440.184593floatnullablep_rot_bibcodeSource of p_rotmeta.bib.bibcode;time.periodcharnullablecns6_system_idCNS6 unique identifier of the stellar system this object belongs to.meta.id.parent0102.02527.55056.3752441.0longn_planetsNumber of confirmed planets associated with the stellar systemmeta.number00.00.02.081.0shortnullablereference_object_cns5_idCNS5_id of the reference object for the object in this entrymeta.id.parentcharnullablenexa_idIdentifier of the object in the NExA (NASA Exoplanet Archive)meta.id.crosscharnullablemultiplicity_bibcodeBibcode for literature references documenting system multiplicity.meta.bib.bibcodecharnullableremarksAdditional free-text information about the object, in particular warnings about possible mis-identifications or results that have been disputed in the literature.meta.notecharnullablecstl This table contains constellation data from Davenhall et al, ivo://cds.vizier/vi/49, converted to ADQL-queriable polygons. The polygons use the J2000 points, and we skip the interpolated points.cstl.geo This table contains constellation data from Davenhall et al, ivo://cds.vizier/vi/49, converted to ADQL-queriable polygons. The polygons use the J2000 points, and we skip the interpolated points.87abbrevAbbreviation of the constellation namemeta.id;meta.maincharnullablenameFull name of the constellation namemeta.idcharnullablepThe coverage of the constellation as an ADQL polygonposdoubleindexednullableraRepresentative RA (actually, the mean of the vertices)degpos.eq.ra;meta.main1.1255911.5015186.724336.104355.9551floatnullabledecRepresentative Dec (actually, the mean of the vertices)degpos.eq.dec;meta.main-80.5115-73.5104-14.971264.854275.67791floatnullabledasch This is a re-publication of the metadata from StarGlass, an information service operated by Harvard College Observatory (HCO) which primarily indexes the holdings of the HCO Astronomical Photographic Glass Plate Collection. This collection is the world's largest archive of astronomical photographic glass plates, consisting of more than 550,000 images documenting the entire sky over a century-long time baseline. Approximately 430,000 plates in the collection, representing the subset of sky images deemed suitable for astrometric and photometric calibration, have been digitized at high resolution by the DASCH project. StarGlass makes available both photographs and calibrated scientific data when available. This resource re-publishes the metadata in separate tables for “narrow” and “wide” (extremely wide-field) plates. The narrow plates are also published in an obscore table and as a SIAP2 service.dasch.narrow_platesThis table holds metadata for the parts of DASCH counting as targeted observations (plate scale below 400 arcsec/mm. “Patrol” and “Meteor” plates in DASCH nomenclature are found in the wide_plates table.340768dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel11.02.02.021.00123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectionDASCHcharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.size1010.010.010.0101.0longnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classNULLcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c10.0023972511.9125197.731349.9133600.545579doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9722-72.2835-2.0422989.382389.9880.545579doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameter0.6134473.3653214.008515.315450.39290.545579floatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharindexednullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.value4.8117e-050.5683881.829412.120686.807880.545579floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime975711605.12319033980.4497511doubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime975711605.12319033980.4497511doubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent0300180058205403000.54577floatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.value0floatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit0floatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit0floatindexednullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refval0floatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.nameHarvard-Smithsonian Center for Astrophysicscharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.name1 in Cook Lens #832 Series renamed from ac-a10-inch Metcalf Triplet11-inch Draper Refractor12-inch Metcalf Doublet13-inch Boyden Refractor16-inch Metcalf Doublet (Refigured after 3500)200 inch Hale Telescope24-33 in Jewett Schmidt24-inch Bruce Doublet24-inch Clark Reflector32-36 inch BakerSchmidt 10 1/2 inch round Armagh-Dunsink-Harvard4-inch Cooke (1-327)4-inch Cooke Lens4-inch Voightlander Lens7.5-inch Cooke/Clark Refractor at Maria Mitchell Observatory8-inch Bache Doublet8-inch Brashear Lens8-inch Draper Doublet8-inch Ross LundinAsiago Observatory 92/67 cm SchmidtLowel 40 inch reflectorPositivesYSO Double Astrographcharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins186848757.017410.022041.0382430.5455794intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2868410977.021953.022041.0382430.5455794intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBins11.01.01.011.0intnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBins11.01.01.011.0intnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBins0.0intnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriod4.8117e-050.5683881.829412.120686.807880.545579floatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullabledasch_idPlate identifier in DASCHmeta.id;meta.maincharindexedprimaryplate_commentComment associated with plate describing context or contentmeta.notecharnullableplate_classPlate class; Values are taken from https://library.cfa.harvard.edu/plate-classesmeta.codecharnullablemosaicsMetadata on the FITS files of the scans available; this is largely used by GAVO to produce the datalink document. In case you want to use it directly, see https://starglass.cfa.harvard.edu/docs/api/mosaics.htmlmeta;meta.datasetcharnullabledasch.platesThis table is a union of the narrow_plates and wide_plates tables. For non-historic use, you probably get better results looking at narrow_plates.559242dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel0123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.sizelongnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameterfloatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharindexednullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.valuefloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extentfloatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.valuefloatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimitfloatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimitfloatindexednullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refvalfloatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.namecharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.namecharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBinsintnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBinsintnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBinsintnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriodfloatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullabledasch_idPlate identifier in DASCHmeta.id;meta.maincharnullableplate_commentComment associated with plate describing context or contentmeta.notecharnullableplate_classPlate class; Values are taken from https://library.cfa.harvard.edu/plate-classesmeta.codecharnullablemosaicsMetadata on the FITS files of the scans available; this is largely used by GAVO to produce the datalink document. In case you want to use it directly, see https://starglass.cfa.harvard.edu/docs/api/mosaics.htmlmeta;meta.datasetcharnullabledasch.wide_platesThis table holds metadata for the “Patrol” and “Meteor” plates from DASCH, i.e., very wide-field observations presumably not useful in global discovery. These data products are therefore not re-published through obscore. For the “narrow” plates, see the narrow_plates table.218474dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel11.02.02.021.00123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectionDASCHcharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.size1010.010.010.0101.0longnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classNULLcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c10.0005086494.07897182.113345.8473600.791041doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9853-74.687815.027976.669289.98310.791041doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameter3.7070231.996249.186591.40895.40980.791041floatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharindexednullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.value3.53284e-053.284216.7240315.052718.24090.791041floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime1259515959.128356.346650.6539791doubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime1259515959.128356.346650.7539791doubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent-93001320372080401900200.791188floatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.value0floatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit0floatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit0floatindexednullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refval0floatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.nameHarvard-Smithsonian Center for Astrophysicscharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.name1-inch1.5 in Cooke "Long Focus"1.5 inch Ross (short focus)1.5-inch Cooke Lenses1.5-inch Ross-Xpress2.5 inch Cooke Lens2.5 inch Voigtlander (Little Bache or "Bachito")2.5-inch Ross Portrait Lens2.6-inch Zeiss-Tessar2.8-inch Kodak Aero-Ektar3 inch Perkin-Zeiss Lens3 inch Ross-Tessar Lens3-inch Elmer Ross3-inch Ross3-inch Ross Fecker4-inch Ross LundinAir Force CameraCerro Tololo 4 meterDamons North BlueDamons North RedDamons North YellowDamons South BlueDamons South RedDamons South YellowEastman Aero-Ektar K-24 Lens on a K-19 BarrelEastman Aero-Ektar K-24 Lens on a K-19 Barrel Formerly KE (1951)Eastman Aero-Ektar K-24 Lens on a K-19 Barrel Formerly KG (1950)K-19 Air Force CameraKE Camera with Installed Rough FocusLogbook Only. Pages without plates.NULLNew Cooke LensPalomar Sky Survey (POSS)Patrol camerasRoe 6-inchcharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1868417371.017410.017493.0220410.7910415intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins21097721953.022041.022041.0220410.7910415intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBins11.01.01.011.0intnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBins11.01.01.011.0intnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBins0.0intnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriod3.53284e-053.284216.7240315.052718.24090.791041floatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullabledasch_idPlate identifier in DASCHmeta.id;meta.maincharindexedprimaryplate_commentComment associated with plate describing context or contentmeta.notecharnullableplate_classPlate class; Values are taken from https://library.cfa.harvard.edu/plate-classesmeta.codecharnullablemosaicsMetadata on the FITS files of the scans available; this is largely used by GAVO to produce the datalink document. In case you want to use it directly, see https://starglass.cfa.harvard.edu/docs/api/mosaics.htmlmeta;meta.datasetcharnullabledfbsplates The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. This service serves the scanned objective prism images and offers SODA-based cutouts.dfbsplates.main The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. This service serves the scanned objective prism images and offers SODA-based cutouts.1711accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableplateIdentifier (plate number) for the DFBS plate.meta.idcharnullableexptimeExposure time.sfloatnullablepublisher_didDataset identifier assigned by the publisher.meta.ref.urlcharnullabledfbsspec The First Byurakan Survey (FBS) is the largest and the first systematic objective prism survey of the extragalactic sky. It covers 17,000 sq.deg. in the Northern sky together with a high galactic latitudes region in the Southern sky. The FBS has been carried out by B.E. Markarian, V.A. Lipovetski and J.A. Stepanian in 1965-1980 with the Byurakan Observatory 102/132/213 cm (40"/52"/84") Schmidt telescope using 1.5 deg. prism. Each FBS plate contains low-dispersion spectra of some 15,000-20,000 objects; the whole survey consists of about 20,000,000 objects.dfbsspec.spectraThis table contains basic metadata as well as the spectra from the Digital First Byurakan Survey (DFBS).accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableplateNumber of the plate this spectrum was extracted from. Technically, this is a foreign key into dfbs.plates.charindexednullablespecidIdentifier of the spectrum built from the plate identifier, a -, and the object position as in objectid.meta.id;meta.maincharindexednullableraICRS RA of the source of this spectrum.degpos.eq.ra;meta.main08.92942174.657352.2273601doubleindexednullabledecICRS Dec of the source of this spectrum.degpos.eq.dec;meta.main-22.9211-10.754725.610777.801389.96291doubleindexednullableposThe object position as s pgsphere spoint.pos.eqdoublenullablesp_classQuality indicator: OK of undisturbed spectra of sufficiently bright objects, NL if disturbers are nearby, U for objects unclassifiable because of lack of signal.meta.code.qualcharnullablepx_lengthNumber of points in this spectrum1111161241301411floatnullablefluxFlux points of the extracted spectrum (arbitrary units)phot.flux.density;em.wlfloatnullablemagbSource object magnitude in Johnson Bmagphot.mag;em.opt.B0.9212.6715.7818.1129.761floatnullablemagrSource object magnitude in Johnson Rmagphot.mag;em.opt.R-11.8611.9515.0117.3834.031floatnullablesnrEstimated signal-to-noise ratio for this spectrum.stat.snr00.43.7105.51.43551e+061floatnullablelam_minMinimal wavelength in this spectrum (the longest wavelength is always 690 nm).mem.wl;stat.min3.126e-073.169e-073.214e-073.28e-073.325e-071floatindexednullablepx_xLocation of the spectrum on the plate scan, x coordinate.pixelpos.cartesian.x;instr02864826932598001floatnullablepx_yLocation of the spectrum on the plate scan, y coordinate.pixelpos.cartesian.y;instr02954832931698011floatnullablepos_angPosition angle of the spectrum on the plate, north over east.degpos.posAng036.6288.79144.021801floatnullableepochDate of observation from WFPDB (this probably does not include the time).dtime.epochdoubleindexednullableexptimeExposure time from WFPDB.stime.duration;obs.exposurefloatnullableemulsionEmulsion used in this plate from WFPDB.instr.plate.emulsioncharnullablespectralSpectral points of the extracted spectrum (wavelengths) as an array (the points are the same for all spectra; the array in this column is cropped at the blue end to match the length of flux).mem.wlfloatnullablecutout_linkCutout of the image this spectrum was extracted frommeta.ref.urlcharnullabledfbsspec.raw_spectra Raw metadata for the spectra, to be combined with image metadata like date_obs and friends for a complete spectrum descriptions. This also contains spectral and flux points in array-valued columns.24000000accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size2000020000.020000.020000.0200001.0longnullablespecidIdentifier of the spectrum built from the plate identifier, a -, and the object position as in objectid.meta.id;meta.maincharindexedprimaryplateNumber of the plate this spectrum was extracted from. Technically, this is a foreign key into dfbs.plates.charindexednullableobjectidSynthetic object id assigned by DFBS.meta.idcharnullableraICRS RA of the source of this spectrum.degpos.eq.ra;meta.main08.92942174.657352.2273601doubleindexednullabledecICRS Dec of the source of this spectrum.degpos.eq.dec;meta.main-22.9211-10.754725.610777.801389.96291doubleindexednullableposThe object position as s pgsphere spoint.pos.eqdoublenullablesp_classQuality indicator: OK of undisturbed spectra of sufficiently bright objects, NL if disturbers are nearby, U for objects unclassifiable because of lack of signal.meta.code.qualcharnullablefluxFlux points of the extracted spectrum (arbitrary units)phot.flux.density;em.wlfloatnullablemagbSource object magnitude in Johnson Bmagphot.mag;em.opt.B0.9212.6715.7818.1129.761floatnullablemagrSource object magnitude in Johnson Rmagphot.mag;em.opt.R-11.8611.9515.0117.3834.031floatnullablesnrEstimated signal-to-noise ratio for this spectrum.stat.snr00.43.7105.51.43551e+061floatnullablelam_minMinimal wavelength in this spectrum (the longest wavelength is always 690 nm).mem.wl;stat.min3.126e-073.169e-073.214e-073.28e-073.325e-071floatindexednullableskySky background estimation from the scan (uncalibrated).instr.skyLevel08756.811818.114137.6320001floatnullablepx_xLocation of the spectrum on the plate scan, x coordinate.pixelpos.cartesian.x;instr02864826932598001floatnullablepx_yLocation of the spectrum on the plate scan, y coordinate.pixelpos.cartesian.y;instr02954832931698011floatnullablepos_angPosition angle of the spectrum on the plate, north over east.degpos.posAng036.6288.79144.021801floatnullablepx_lengthNumber of points in this spectrum1111161241301411floatnullablepub_didDataset identifier assigned by the publisher.meta.ref.urlcharindexednullabledfbsspec.ssaA view providing standard SSA metadata for DBFS metadata in dfbsspec.spectra23213283accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typecharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharnullablessa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcecharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.Calibrationcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.Calibrationcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablemagbSource object magnitude in Johnson Bmagphot.mag;em.opt.B0.9212.6715.7818.1129.761floatnullablemagrSource object magnitude in Johnson Rmagphot.mag;em.opt.R-11.8611.9515.0117.3834.031floatnullableplateNumber of the plate this spectrum was extracted from. Technically, this is a foreign key into dfbs.plates.charindexednullableraICRS RA of the source of this spectrum.degpos.eq.ra;meta.main08.92942174.657352.2273601doubleindexednullabledecICRS Dec of the source of this spectrum.degpos.eq.dec;meta.main-22.9211-10.754725.610777.801389.96291doubleindexednullableemi These are 1.4GHz Very Long Baseline Interferometry images of 532 radio sources with a flux density exceeding 100uJy as determined by Ibar et al. (2009, MNRAS, 397, 281), obtained between 2010-06-03 and 2010-09-03. For all fields, we give frames processed using natural weighting to preserve maximal sensitivity. For the 65 detected sources, we additionally give frames processed using uniform weighting to suppress sidelobes (see Middelberg et al. 2013, A&A 551, 97 for details) in flux density measurements. Some sources have larger images to cover a larger area because the initial coordinates were not sufficiently accurate.emi.main These are 1.4GHz Very Long Baseline Interferometry images of 532 radio sources with a flux density exceeding 100uJy as determined by Ibar et al. (2009, MNRAS, 397, 281), obtained between 2010-06-03 and 2010-09-03. For all fields, we give frames processed using natural weighting to preserve maximal sensitivity. For the 65 detected sources, we additionally give frames processed using uniform weighting to suppress sidelobes (see Middelberg et al. 2013, A&A 551, 97 for details) in flux density measurements. Some sources have larger images to cover a larger area because the initial coordinates were not sufficiently accurate.561dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel0123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.sizelongnullabletarget_nameSource name as in 2009MNRAS.397..281I (VizieR J/MNRAS/397/281)meta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameterfloatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.valuefloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoublenullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extentfloatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.valuefloatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimitfloatnullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimitfloatnullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refvalfloatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.namecharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.namecharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBinsintnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBinsintnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBinsintnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriodfloatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullableobsraAntenna pointing, RAdegpos.eq.rafloatnullableobsdecAntenna pointing, Decdegpos.eq.decfloatnullableweightingNatural or uniform, according to weighting method.meta.codenaturaluniformcharnullables_resolution_minAngular resolution, longest baseline and max frequency dependentarcsecpos.angResolution;stat.minChar.SpatialAxis.Resolution.Bounds.Limits.LoLimfloatnullables_resolution_maxAngular resolution, longest baseline and min frequency dependentarcsecpos.angResolution;stat.maxChar.SpatialAxis.Resolution.Bounds.Limits.HiLimfloatnullableferos Spectra from FEROS spectrograph at La Silla's 1.5m telescope as obtained during commissioning and guaranteed time.feros.data Spectra from FEROS spectrograph at La Silla's 1.5m telescope as obtained during commissioning and guaranteed time.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wl;obs.atmoscharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitmagcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionFeroscharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentFEROScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcepointedcharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationUNCALIBRATEDcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablefk6 Parts I and III of the sixth fundamental catalog, a catalog of high-precision astrometry for bright stars combining centuries of ground-based observations as reflected in FK5 with HIPPARCOS astrometry. The result contains, in particular for the proper motions, statistically significant improvements of the Hipparcos data und represents a system of unprecedented accuracy for these 4150 fundamental stars. The typical mean error in pm is 0.35 mas/year for 878 basic stars, and 0.59 mas/year for the sample of the 3272 additional stars.fk6.fk6joinThe union of all published parts of FK6, comprising only the common fields.4151localidFK6 number of the star (it is identical with its FK5 or FK4sup number)meta.id;meta.maincharhipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997)meta.id1223367.2557555.5115613.081183221.0intcomnameCommon Namemeta.idcharnullableraj2000The right ascension alpha of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.ra;meta.main0.39876210.7311176.985351.304359.9791doubledej2000The declination delta of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.dec;meta.main-88.9565-79.0195-2.8670676.972987.02011doublepmraThe proper-motion component of the star in alpha at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6, cos(delta) applied.deg/yrpos.pm;pos.eq.ra;meta.main-0.000477911-4.84185e-05-1.63889e-076.50351e-050.001112021floatpmdeThe proper-motion component mu_delta of the star in delta at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.deg/yrpos.pm;pos.eq.dec;meta.main-0.0016153-8.12626e-05-2.65972e-063.68433e-050.0003236861floatepraCentral epoch of raj2000 in the SI mode.yrtime.epoch;pos.eq.ra1990.681990.831991.191991.541991.781floate_raj2000Mean error of raj2000 in the SI mode, cos(delta) applied.degstat.error;pos.eq.ra;meta.main8.05556e-089.72222e-081.58333e-072.33333e-073.38889e-071floate_pmraMean error of pmra in the SI mode.deg/yrstat.error;pos.pm;pos.eq.ra;meta.main5.55556e-086.38889e-089.44444e-081.47222e-072.27778e-071floatepdeCentral epoch of delta in the SI mode.yrtime.epoch;pos.eq.dec1990.631990.791991.241991.651991.861floate_dej2000Mean error of dej2000 at the central epoch epdedegstat.error;pos.eq.ra;meta.main8.61111e-081.02778e-071.25e-071.66667e-072.13889e-071floate_pmdeMean error of pmde in the SI mode.deg/yrstat.error;pos.pm;pos.eq.dec;meta.main5e-085.83333e-089.16667e-081.33333e-071.80556e-071floatpres'Resulting' parallax p_res of the star. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax.degpos.parallax1.52778e-076.26722e-072.94722e-061.9599e-057.66e-051floatnullablee_presMean error of parallaxdegstat.error;pos.parallax2.5e-081.11972e-072.02778e-072.76917e-073.41667e-071floatnullablesrc_parSource of parallax (H=HIPPARCOS, P=Newly determined photometric or spectroscopic parallax)meta.code;pos.parallaxcharv_radRadial velocitykm/sspect.dopplerVeloc;pos.heliocentric-117.5-43.4070.142.20499.31floatnullablevmagApparent visual magnitude m_V of the star, taken from the HIPPARCOS Cataloguemagphot.mag;em.opt.V-0.622.39625.0456.79388.251floatvarflagFlag for the variability of the brightness of the star, taken from the HIPPARCOS Catalogue (see note)meta.code;src.varcharnullablek_binFlag for the double-star nature of the object (see note)meta.code.multip1111.021.039.0391.0shortk_delta_muFlag for the double-star nature of the object based on differences between various proper motions (see note)meta.code.multipcharnullablek_aeFlag for astrometrically excellent stars, larger numbers are better (3 is best)meta.code.qual11.03.03.030.38724375shortnullablesectFK6 part of this recordmeta.id.part;meta.main11.01.01.011.0shortnoteNote for this objectmeta.notecharnullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.ra-0.000478275-4.87266e-05-2.01389e-076.50486e-050.001112131floatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.dec-0.00161518-8.12889e-05-2.61111e-063.68622e-050.0003237721floatnullablee_pmrastpMean error in PM(RA)*cos(delta) in STP modedeg/yrstat.error;pos.pm;pos.eq.ra8.33333e-081.05556e-071.72222e-072.83333e-074.75e-071floatnullablee_pmdestpMean error in PM(Dec) in STP modedeg/yrstat.error;pos.pm;pos.eq.dec8.61111e-081.05556e-071.44444e-072.18583e-073.13889e-071floatnullablepmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.ra-0.000477772-4.83733e-05-1.875e-076.50038e-050.001111921floatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.dec-0.00161528-8.11238e-05-2.65417e-063.68509e-050.0003235971floatnullablee_pmraltpMean error in PM(RA)*cos(delta) in LTP modedeg/yrstat.error;pos.pm;pos.eq.ra6.66667e-088.05556e-081.27778e-072.19444e-072.63889e-071floatnullablee_pmdeltpMean error in PM(Dec) in LTP modedeg/yrstat.error;pos.pm;pos.eq.dec5.83333e-087.77778e-081.25e-072.05556e-072.63889e-071floatnullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.ra-0.000478319-4.87726e-05-2.23611e-076.50472e-050.001112141floatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.dec-0.00161518-8.12917e-05-2.59444e-063.68649e-050.0003237781floatnullablee_pmrahipMean error in PM(RA)*cos(delta) in HIP modedeg/yrstat.error;pos.pm;pos.eq.ra8.61111e-081.06417e-071.83333e-073.27778e-077.02778e-071floatnullablee_pmdehipMean error in PM(Dec) in HIP modedeg/yrstat.error;pos.pm;pos.eq.dec8.88889e-081.09194e-071.5e-072.43778e-075.22222e-071floatnullablefk6.part1Part I of the FK6 (successor to Basic FK5)878hipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997)meta.id1223367.2557555.5115613.081183221.0intcomnameCommon Namemeta.idcharnullableraj2000The right ascension alpha of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.ra;meta.main0.39876210.7311176.985351.304359.9791doubleindexeddej2000The declination delta of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.dec;meta.main-88.9565-79.0195-2.8670676.972987.02011doubleindexedpmraThe proper-motion component of the star in alpha at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6, cos(delta) applied.deg/yrpos.pm;pos.eq.ra;meta.main-0.000477911-4.84185e-05-1.63889e-076.50351e-050.001112021floatpmdeThe proper-motion component mu_delta of the star in delta at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.deg/yrpos.pm;pos.eq.dec;meta.main-0.0016153-8.12626e-05-2.65972e-063.68433e-050.0003236861floatepraCentral epoch of raj2000 in the SI mode.yrtime.epoch;pos.eq.ra1990.681990.831991.191991.541991.781floate_raj2000Mean error of raj2000 in the SI mode, cos(delta) applied.degstat.error;pos.eq.ra;meta.main8.05556e-089.72222e-081.58333e-072.33333e-073.38889e-071floate_pmraMean error of pmra in the SI mode.deg/yrstat.error;pos.pm;pos.eq.ra;meta.main5.55556e-086.38889e-089.44444e-081.47222e-072.27778e-071floatepdeCentral epoch of delta in the SI mode.yrtime.epoch;pos.eq.dec1990.631990.791991.241991.651991.861floate_dej2000Mean error of dej2000 at the central epoch epdedegstat.error;pos.eq.ra;meta.main8.61111e-081.02778e-071.25e-071.66667e-072.13889e-071floate_pmdeMean error of pmde in the SI mode.deg/yrstat.error;pos.pm;pos.eq.dec;meta.main5e-085.83333e-089.16667e-081.33333e-071.80556e-071floatpres'Resulting' parallax p_res of the star. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax.degpos.parallax1.52778e-076.26722e-072.94722e-061.9599e-057.66e-051floatnullablee_presMean error of parallaxdegstat.error;pos.parallax2.5e-081.11972e-072.02778e-072.76917e-073.41667e-071floatnullablesrc_parSource of parallax (H=HIPPARCOS, P=Newly determined photometric or spectroscopic parallax)meta.code;pos.parallaxcharv_radRadial velocitykm/sspect.dopplerVeloc;pos.heliocentric-117.5-43.4070.142.20499.31floatnullablevmagApparent visual magnitude m_V of the star, taken from the HIPPARCOS Cataloguemagphot.mag;em.opt.V-0.622.39625.0456.79388.251floatvarflagFlag for the variability of the brightness of the star, taken from the HIPPARCOS Catalogue (see note)meta.code;src.varcharnullablek_binFlag for the double-star nature of the object (see note)meta.code.multip1111.021.039.0391.0shortk_delta_muFlag for the double-star nature of the object based on differences between various proper motions (see note)meta.code.multipcharnullablek_aeFlag for astrometrically excellent stars, larger numbers are better (3 is best)meta.code.qual11.03.03.030.38724375shortnullablesectFK6 part of this recordmeta.id.part;meta.main11.01.01.011.0shortlocalidFK6 number of the star (it is identical with its FK5 or FK4sup number)meta.id;meta.maincharindexedprimaryraltpRight ascension in LTP modedegpos.eq.ra0.39876210.7311176.985351.304359.9791doublenullabledeltpDeclination in LTP modedegpos.eq.dec-88.9565-79.0195-2.8670676.972987.02011doublenullablepmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.ra-0.000477772-4.83733e-05-1.875e-076.50038e-050.001111921floatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.dec-0.00161528-8.11238e-05-2.65417e-063.68509e-050.0003235971floatnullableepraltpCentral epoch of RA (LTP)yrstat.error;time.epoch;pos.eq.ra1957.051965.41981.681989.421990.891floatnullablee_raltpError in RA (LTP) with cos(delta) already applieddegstat.error;pos.eq.ra7.86111e-071.52461e-062.71944e-063.90767e-064.19722e-061floatnullablee_pmraltpMean error in PM(RA)*cos(delta) in LTP modedeg/yrstat.error;pos.pm;pos.eq.ra6.66667e-088.05556e-081.27778e-072.19444e-072.63889e-071floatnullableepdeltpCentral epoch of Dec (LTP)yrstat.error;time.epoch;pos.eq.dec1954.471964.11982.491989.761991.071floatnullablee_deltpError in Dec (LTP)degstat.error;pos.eq.dec7.88889e-071.54233e-062.90278e-064.12222e-064.41667e-061floatnullablee_pmdeltpMean error in PM(Dec) in LTP modedeg/yrstat.error;pos.pm;pos.eq.dec5.83333e-087.77778e-081.25e-072.05556e-072.63889e-071floatnullablerastpRight ascension in STP modedegpos.eq.ra0.39876510.7311176.985351.304359.9791doublenullabledestpDeclination in STP modedegpos.eq.dec-88.9565-79.0195-2.8670676.972987.02011doublenullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.ra-0.000478275-4.87266e-05-2.01389e-076.50486e-050.001112131floatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.dec-0.00161518-8.12889e-05-2.61111e-063.68622e-050.0003237721floatnullableeprastpCentral epoch of RA (STP)yrstat.error;time.epoch;pos.eq.ra1990.751990.911991.231991.591991.81floatnullablee_rastpError in RA (STP) with cos(delta) already applieddegstat.error;pos.eq.ra8.05556e-089.72222e-081.61111e-072.36111e-073.41667e-071floatnullablee_pmrastpMean error in PM(RA)*cos(delta) in STP modedeg/yrstat.error;pos.pm;pos.eq.ra8.33333e-081.05556e-071.72222e-072.83333e-074.75e-071floatnullableepdestpCentral epoch of Dec (STP)yrstat.error;time.epoch;pos.eq.dec1990.661990.811991.261991.661991.851floatnullablee_destpError in Dec (STP)degstat.error;pos.eq.dec8.88889e-081.02778e-071.27778e-071.69444e-072.16667e-071floatnullablee_pmdestpMean error in PM(Dec) in STP modedeg/yrstat.error;pos.pm;pos.eq.dec8.61111e-081.05556e-071.44444e-072.18583e-073.13889e-071floatnullablerahipRight ascension in HIP modedegpos.eq.ra0.39876610.7311176.985351.304359.9791doublenullabledehipDeclination in HIP modedegpos.eq.dec-88.9565-79.0195-2.8670676.972987.02011doublenullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.ra-0.000478319-4.87726e-05-2.23611e-076.50472e-050.001112141floatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.dec-0.00161518-8.12917e-05-2.59444e-063.68649e-050.0003237781floatnullableeprahipCentral epoch of RA (HIP)yrstat.error;time.epoch;pos.eq.ra1990.751990.911991.231991.591991.81floatnullablee_rahipError in RA (HIP) with cos(delta) already applieddegstat.error;pos.eq.ra8.05556e-089.72222e-081.61111e-072.38889e-073.44444e-071floatnullablee_pmrahipMean error in PM(RA)*cos(delta) in HIP modedeg/yrstat.error;pos.pm;pos.eq.ra8.61111e-081.06417e-071.83333e-073.27778e-077.02778e-071floatnullableepdehipCentral epoch of Dec (HIP)yrstat.error;time.epoch;pos.eq.dec1990.661990.821991.261991.671991.871floatnullablee_dehipError in Dec (HIP)degstat.error;pos.eq.dec8.88889e-081.02778e-071.27778e-071.69444e-072.16667e-071floatnullablee_pmdehipMean error in PM(Dec) in HIP modedeg/yrstat.error;pos.pm;pos.eq.dec8.88889e-081.09194e-071.5e-072.43778e-075.22222e-071floatnullableparallaxsiParallax obtained in solution SIdegpos.parallax7.22222e-085.44444e-072.95417e-061.96195e-057.66083e-051floatnullablee_parallaxsiError in parallax obtained in solution SIdegstat.error;pos.parallax1.19444e-071.30556e-072.01389e-072.65806e-073.5e-071floatnullableparallaxstpParallax obtained in solution STPdegpos.parallax7.5e-085.58417e-072.95e-061.96009e-057.66028e-051floatnullablee_parallaxstpError in parallax obtained in solution STPdegstat.error;pos.parallax1.19444e-071.30556e-072.05556e-072.75e-073.55556e-071floatnullableparallaxhipParallax obtained in solution HIPdegpos.parallax7.77778e-085.65694e-072.94722e-061.9599e-057.66e-051floatnullablee_parallaxhipError in parallax obtained in solution HIPdegstat.error;pos.parallax1.19444e-071.30556e-072.05556e-072.75e-073.75e-071floatnullablenoteNote for this objectmeta.notecharnullablefk6.part3Part III of the FK6 (containing stars from the FK5 extension and Rsup)3273localidFK6 number of the star (it is identical with its FK5 or FK4sup number)meta.id;meta.maincharsubsampleFlag for the subsample of FK6(III) stars; BX and FX denote stars from the bright and faint FK5 extensions, respectively, RS denotes stars from RSup (1993VeARI..34....1S)meta.id;meta.datasetcharnullablehipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997)meta.id433605.319999999999759314.0115456.441183201.0intcomnameCommon Namemeta.idcharnullableraj2000The right ascension alpha of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.ra;meta.main0.12870111.5396182.526350.762359.9761doubledej2000The declination delta of the star at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.degpos.eq.dec;meta.main-89.7717-77.49141.1812377.592689.40651doublepmraThe proper-motion component of the star in alpha at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6, cos(delta) applied.deg/yrpos.pm;pos.eq.ra;meta.main-0.00122496-3.16553e-05-4.33333e-072.81241e-050.0002209281floatpmdeThe proper-motion component mu_delta of the star in delta at epoch and equinox J2000.0 in the ICRS/HIPPARCOS system for the SI mode of the FK6.deg/yrpos.pm;pos.eq.dec;meta.main-0.000316472-3.2865e-05-1.61667e-061.58752e-050.0002615641floatepraCentral epoch of raj2000 in the SI mode.yrtime.epoch;pos.eq.ra1990.611990.91991.231991.581992.061floate_raj2000Mean error of raj2000 in the SI mode, cos(delta) applied.degstat.error;pos.eq.ra;meta.main7.77778e-081.05556e-071.83333e-073.13889e-074.72222e-071floate_pmraMean error of pmra in the SI mode.deg/yrstat.error;pos.pm;pos.eq.ra;meta.main7.5e-081e-071.61111e-072.58333e-073.88889e-071floatepdeCentral epoch of delta in the SI mode.yrtime.epoch;pos.eq.dec1990.471990.821991.261991.671992.051floate_dej2000Mean error of dej2000 at the central epoch epdedegstat.error;pos.eq.ra;meta.main8.61111e-081.08333e-071.47222e-072.27778e-073.38889e-071floate_pmdeMean error of pmde in the SI mode.deg/yrstat.error;pos.pm;pos.eq.dec;meta.main8.33333e-081.05556e-071.5e-072.25e-073.19444e-071floatpres'Resulting' parallax p_res of the star. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax.degpos.parallax-3.61111e-072.5e-071.55556e-067.61111e-060.0002061111floatnullablee_presMean error of parallaxdegstat.error;pos.parallax1.11111e-081.14333e-072.22222e-073.69444e-075.55556e-071floatnullablesrc_parSource of parallax (H=HIPPARCOS, P=Newly determined photometric or spectroscopic parallax)meta.code;pos.parallaxcharv_radRadial velocitykm/sspect.dopplerVeloc;pos.heliocentric-116-47.228-1.5441800.520929floatnullablevmagApparent visual magnitude m_V of the star, taken from the HIPPARCOS Cataloguemagphot.mag;em.opt.V3.594.856.999.079.711floatvarflagFlag for the variability of the brightness of the star, taken from the HIPPARCOS Catalogue (see note)meta.code;src.varcharnullablek_binFlag for the double-star nature of the object (see note)meta.code.multip1111.013.038.0391.0shortk_delta_muFlag for the double-star nature of the object based on differences between various proper motions (see note)meta.code.multipcharnullablek_aeFlag for astrometrically excellent stars, larger numbers are better (3 is best)meta.code.qual11.03.03.030.58936757shortnullablesectFK6 part of this recordmeta.id.part;meta.main33.03.03.031.0shortpmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.ra-0.001225-3.14852e-05-4.22222e-072.80358e-050.0002209971floatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.dec-0.000317022-3.27569e-05-1.60278e-061.58766e-050.0002613861floatnullablee_pmraltpMean error in PM(RA)*cos(delta) in LTP modedeg/yrstat.error;pos.pm;pos.eq.ra1.16667e-071.47222e-072.38889e-073.69444e-075.05556e-071floatnullablee_pmdeltpMean error in PM(Dec) in LTP modedeg/yrstat.error;pos.pm;pos.eq.dec1.22222e-071.63889e-072.52778e-073.77778e-075.25e-071floatnullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.ra-0.00122495-3.16948e-05-4.33333e-072.82433e-050.0002208251floatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.dec-0.000316114-3.28592e-05-1.62222e-061.57196e-050.0002617251floatnullablee_pmrastpMean error in PM(RA)*cos(delta) in STP modedeg/yrstat.error;pos.pm;pos.eq.ra8.33333e-081.13889e-071.94444e-073.16667e-074.5e-071floatnullablee_pmdestpMean error in PM(Dec) in STP modedeg/yrstat.error;pos.pm;pos.eq.dec9.16667e-081.13889e-071.66667e-072.63889e-073.58333e-071floatnullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.ra-0.00122495-3.17639e-05-4.05556e-072.82882e-050.0002208031floatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.dec-0.000316067-3.28584e-05-1.60556e-061.57204e-050.000261751floatnullablee_pmrahipMean error in PM(RA)*cos(delta) in HIP modedeg/yrstat.error;pos.pm;pos.eq.ra8.61111e-081.16667e-072.13889e-074.19e-076.5e-071floatnullablee_pmdehipMean error in PM(Dec) in HIP modedeg/yrstat.error;pos.pm;pos.eq.dec9.16667e-081.19444e-071.77778e-073.13889e-075.13889e-071floatnullablehipdupHIPPARCOS indicators for a suspected visual binary; d=duplicity induced variability (H52), s=Hipparcos suspected non-single (H61), t=bothmeta.code.multipcharnullablehipfitqualHIPPARCOS goodness-of-fit parameter (HIP Field H30, F2); A large value of F2 (e.g. larger than 3) may be caused by a duplicity of the object, but other reasons cannot be excluded. NULL means a negative goodness-of-fit in HIP.meta.code.qual00.00.02.040.20745493shortnullablespeckleflagIndications on binarity provided by the catalogue of speckle observations (1999AJ....117.1890M); b=binarity resolved, u=possibly resolved, n=object observed but not resolvedmeta.code.multipcharnullableviscompIndicator for a star which has one (or more) visual component(s) with a separation rho of at least 60 arcsec.meta.code.multipcharnullablebinindsrvIndications for binarity provided by radial velocities from various sources (see Note)meta.code.multipcharnullablebinindeclIndicators for binarity from photometric variability (a=Algol-type, b=β Lyr-type, e=uncertain type, w=W UMa type)meta.code;src.varcharnullablepulsatingIndicator for a variability of the radial velocity V_rad due to stellar pulsation (which may be confused with a variability of V_rad due to spectroscopic binarity; c=Cepheid, s=δ Sct, b=β Cep)meta.code;src.varcharnullablenoteNote for this objectmeta.notecharnullableflashheros Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.flashheros.data Spectra from the Flash and Heros Echelle spectrographs developed at Landessternwarte Heidelberg and mounted at La Silla and various other observatories. The data mostly contains spectra of OB stars. Heros was the name of the instrument after Flash got a second channel in 1995.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablelocalkeyLocal observation key (used to connect to single orders).meta.idcharnullablessa_fluxcalibType of flux calibrationssa:Char.FluxAxis.CalibrationABSOLUTECALIBRATEDRELATIVENORMALIZEDUNCALIBRATEDANYcharnullableflashheros.ordersmetaSSA metadata for split-order Flash/Heros Echelle spectraaccrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.LengthintnullablelocalkeyLocal observation key.meta.idcharnullablen_ordersNumber of orders in the spectrum.meta.numberintnullableorder_minMinimal Echelle order in the spectrum.instr.order;stat.minintnullableorder_maxMaximal Echelle order in the spectrum.instr.order;stat.maxintnullablefornax This is a deep optical mosaic of the Fornax cluster’s core, covering 1.6 square degrees. The data were acquired with ESO/MPG 2.2m/WFI, using a transparent filter that nearly equals the no-filter throughput and thus provides a high signal-to-noise ratio. Based on an approximate conversion to V-band magnitudes, the unbinned and binned mosaics (0.24 and 0.71 arcsec/pixel) reach a median depth of 26.6 and 27.8 mag/sq.arcsec, respectively.fornax.data This is a deep optical mosaic of the Fornax cluster’s core, covering 1.6 square degrees. The data were acquired with ESO/MPG 2.2m/WFI, using a transparent filter that nearly equals the no-filter throughput and thus provides a high signal-to-noise ratio. Based on an approximate conversion to V-band magnitudes, the unbinned and binned mosaics (0.24 and 0.71 arcsec/pixel) reach a median depth of 26.6 and 27.8 mag/sq.arcsec, respectively.2accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size215625600267373843.21078096320.01888818796.819405670401.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra54.814254.814254.814254.814354.81431doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec-35.4465-35.4465-35.4465-35.4465-35.44651doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure55031.555031.555031.555031.555031.51doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median0floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max0floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min0floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullabledidGlobally unique IVOA publisher DID for this dataset.meta.idcharnullabledatalink_urlURL to a datalink document for this mosaic (ancillary files, cutouts)meta.ref.urlcharnullablegcns This is a clean and well characterised catalogue of objects within 100pc of the Sun from the Gaia early third data release. We characterise the catalogue using the full data release, and comparisons to other catalogues in literature and simulations. For all candidates (measured parallax < 8 mas), we calculate a distance probability function using Bayesian procedures and mock catalogues for the prediction of the priors. For each entry using a random forest classifier we attempt to remove sources with spurious astrometric solutions. This results in 331312 objects that should contain at least 92% of stars within 100 pc at spectral type M9. GCNS comes with several auxiliary tables, in particular lists of resolved stellar systems, of known neary stars not found in eDR3 and of candidates of Hyades and ComaBer cluster members.gcns.mainThis is the main catalogue. Additional resources include: gcns.resolvedss (resolved stellar systems), gcns.missing_10mas (objects missing from eDR3 that have been suspected of being within 100 pc before), and gcns.hyacob (probable members of the Hyades and the Coma Berenices open cluster).331312source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongindexedprimaryraICRS right ascension from Gaia eDR3.degpos.eq.ra;meta.maindoubleindexednullabledecICRS declination from Gaia eDR3.degpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch J2016.0. If looking for a distance, consider joining with gedr3dist.main and using the distances from there.maspos.parallaxfloatnullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablepmraProper motion in right ascension of the source in ICRS at J2016.0. This is the tangent plane projection (i.e., multiplied by cos(δ)) of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatnullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdecProper motion in declination at J2016.0.mas/yrpos.pm;pos.eq.decfloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.meanfloatnullablephot_g_mean_flux_over_errorIntegrated mean G flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt;stat.meanfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.Bfloatnullablephot_bp_mean_flux_over_errorIntegrated mean BP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Bfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.Rfloatnullablephot_rp_mean_flux_over_errorIntegrated mean RP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Rfloatnullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weightfloatnullableipd_frac_multi_peakPercentage of distance windows in which a double peak was seen (high values mean high likelihood of a resolved double star).meta.code.multipshortadoptedrvAdopted Radial Velocitykm/sphys.veloc;pos.heliocentricfloatnullableadoptedrv_errorError in adopted RVkm/sstat.error;phys.veloc;pos.heliocentricfloatnullableadoptedrv_refnameBibcode for the source of the radial velocitymeta.bib.bibcodecharnullableradial_velocity_is_valid1 if this object has a radial velocity in eDR3, 0 otherwisemeta.code.qualshortgcns_probProbability that the astrometry is reliablestat.fit.goodnessfloatnullablewd_probprobability that this is a white dwarf.stat.likelihood;src.classfloatnullabledist_11st percentile of the distance PDF, used in GCNS selectionkpcstat.value;pos.distancefloatnullabledist_1616th percentile of the distance PDF (1 σ lower bound)kpcstat.value;pos.distancefloatnullabledist_50Median of the distance PDFkpcpos.distance;stat.medianfloatnullabledist_8484th percentile of the distance PDF (1 σ upper bound)kpcstat.value;pos.distancefloatnullablexcoord_50Median x coordinate in the Galactic frame assuming dist_50pcpos.cartesian.x;stat.medianfloatnullablexcoord_161 σ lower bound of Galactic frame x coordinatepcstat.value;pos.cartesian.xfloatnullablexcoord_841 σ upper bound of Galactic frame x coordinatepcstat.value;pos.cartesian.xfloatnullableycoord_50Median y coordinate in the Galactic frame assuming dist_50pcpos.cartesian.y;stat.medianfloatnullableycoord_161 σ lower bound of Galactic frame y coordinatepcstat.value;pos.cartesian.yfloatnullableycoord_841 σ upper bound of Galactic frame y coordinatepcstat.value;pos.cartesian.yfloatnullablezcoord_50Median z coordinate in the Galactic frame assuming dist_50pcpos.cartesian.z;stat.medianfloatnullablezcoord_161 σ lower bound of Galactic frame z coordinatepcstat.value;pos.cartesian.zfloatnullablezcoord_841 σ upper bound of Galactic frame z coordinatepcstat.value;pos.cartesian.zfloatnullableuvel_50Median velocity u in the Galactic frame, direction positive xkm/sphys.veloc;pos.cartesian.x;stat.medianfloatnullableuvel_161 σ lower bound for ukm/sstat.value;phys.veloc;pos.cartesian.xfloatnullableuvel_841 σ upper bound for ukm/sstat.value;phys.veloc;pos.cartesian.xfloatnullablevvel_50Median velocity v in the Galactic frame, direction positive ykm/sphys.veloc;pos.cartesian.y;stat.medianfloatnullablevvel_161 σ lower bound for vkm/sstat.value;phys.veloc;pos.cartesian.yfloatnullablevvel_841 σ upper bound for vkm/sstat.value;phys.veloc;pos.cartesian.yfloatnullablewvel_50Median velocity w in the Galactic frame, direction positive zkm/sphys.veloc;pos.cartesian.z;stat.medianfloatnullablewvel_161 σ lower bound for wkm/sstat.value;phys.veloc;pos.cartesian.zfloatnullablewvel_841 σ upper bound for wkm/sstat.value;phys.veloc;pos.cartesian.zfloatnullablename_gunnObject Name from PanSTARRS/SDSS/SkyMapper surveymeta.id.crosscharnullablerefname_gunnReference for the source of the Gunn photometrymeta.bib.bibcodecharnullablegmag_gunnGunn G band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Vfloatnullablee_gmag_gunnUncertainty in G band magnitudemagstat.error;phot.mag;em.opt.Vfloatnullablermag_gunnGunn R band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Rfloatnullablee_rmag_gunnUncertainty in R band magnitudemagstat.error;phot.mag;em.opt.Rfloatnullableimag_gunnGunn I band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Ifloatnullablee_imag_gunnUncertainty in I band magnitudemagstat.error;phot.mag;em.opt.Ifloatnullablezmag_gunnGunn Z band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Ifloatnullablee_zmag_gunnUncertainty in Z band magnitudemagstat.error;phot.mag;em.opt.Ifloatnullablename_2massName of this object in 2MASSmeta.id.crosscharnullablej_m_2mass2MASS J band magnitudemagphot.mag;em.IR.Jfloatnullablej_msig_2massUncertainty in 2MASS J band magnitudemagstat.error;phot.mag;em.IR.Jfloatnullableh_m_2mass2MASS H band magnitudemagphot.mag;em.IR.Hfloatnullableh_msig_2massUncertainty in 2MASS H band magnitudemagstat.error;phot.mag;em.IR.Hfloatnullablek_m_2mass2MASS K band magnitudemagphot.mag;em.IR.Kfloatnullablek_msig_2massUncertainty in 2MASS K band magnitudemagstat.error;phot.mag;em.IR.Kfloatnullablename_wiseName of this object in WISEmeta.id.crosscharnullablew1mpro_pm_wiseCATWISE W1 band magnitudemagphot.mag;em.IR.3-4umfloatnullablew1sigmpro_pm_wiseUncertainty in CATWISE W1 band magnitudemagstat.error;phot.mag;em.IR.3-4umfloatnullablew2mpro_pm_wiseCATWISE W2 band magnitudemagphot.mag;em.IR.4-8umfloatnullablew2sigmpro_pm_wiseUncertainty in CATWISE W2 band magnitudemagstat.error;phot.mag;em.IR.4-8umfloatnullablew3mpro_wiseCATWISE W3 band magnitudemagphot.mag;em.IR.8-15umfloatnullablew3sigmpro_wiseUncertainty in CATWISE W3 band magnitudemagstat.error;phot.mag;em.IR.8-15umfloatnullablew4mpro_wiseALLWISE W4 band magnitudemagphot.mag;em.IR.15-30umfloatnullablew4sigmpro_wiseUncertainty in ALLWISE W4 band magnitudemagstat.error;phot.mag;em.IR.15-30umfloatnullablegcns.maglims5 The G magnitude distribution percentiles per level 5 HEALpixes for all Gaia sources with a parallax and a G magnitude measurement. Can be used to approximate the G magnitude limit for Gaia at that position of the sky. Sources up to a limiting magnitude equal to 'magnitude_70' are 98% complete when compared to PS1. The 80th and 90th percentile decrease the completeness in Gaia to 97% and 95%, respectively. These cuts can be very useful, when trying to compare Gaia data to models, e.g. the GeDR3mock catalog (gedrmock.main).12288hpxHEALPix on level 5 these statistics are forpos.healpixfloatnullablemagnitude_7070th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_8080th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_9090th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablesourcecountNumber of objects contributing to the distributionmeta.numberintgcns.maglims6 The G magnitude distribution percentiles per level 6 HEALpixes for all Gaia sources with a parallax and a G magnitude measurement. Can be used to approximate the G magnitude limit for Gaia at that position of the sky. Sources up to a limiting magnitude equal to 'magnitude_70' are 98% complete when compared to PS1. The 80th and 90th percentile decrease the completeness in Gaia to 97% and 95%, respectively. These cuts can be very useful, when trying to compare Gaia data to models, e.g. the GeDR3mock catalog (gedrmock.main).49152hpxHEALPix on level 6 these statistics are forpos.healpixfloatnullablemagnitude_7070th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_8080th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_9090th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablesourcecountNumber of objects contributing to the distributionmeta.numberintgcns.maglims7 The G magnitude distribution percentiles per level 7 HEALpixes for all Gaia sources with a parallax and a G magnitude measurement. Can be used to approximate the G magnitude limit for Gaia at that position of the sky. Sources up to a limiting magnitude equal to 'magnitude_70' are 98% complete when compared to PS1. The 80th and 90th percentile decrease the completeness in Gaia to 97% and 95%, respectively. These cuts can be very useful, when trying to compare Gaia data to models, e.g. the GeDR3mock catalog (gedrmock.main).196608hpxHEALPix on level 7 these statistics are forpos.healpixfloatnullablemagnitude_7070th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_8080th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablemagnitude_9090th percentle of the G-magnitude distribution in Gaia eDR3 for all objects with both parallax and a G magnitudemagstat.paramfloatnullablesourcecountNumber of objects contributing to the distributionmeta.numberintgcns.hyacob A list of 920+212 probable Hyades and ComaBer members in the eDR3 GCNS sample.1132source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongnullablenameName of the cluster this object probably belongs tometa.idcharnullablec_clusterDimensionless chi-square test statistic. Small values indicate highly probable members (cf. eq. 4 in 2018MNRAS.477.3197R)stat.likelihoodfloatnullabledist_clusterDistance of each star from the cluster barycentre.pcpos.distancefloatnullablegcns.mainsource_idsource_idgcns.missing_10masA table of 1258 objects with published parallaxes greater than 10mas that are not or have no parallax in Gaia eDR3 and are hence not listed in gcns.main.1259main_idSource name from Simbadmeta.id;meta.maincharnullableraICRS RA from Simbaddegpos.eq.ra;meta.maindoubleindexednullabledecICRS Dec from Simbaddegpos.eq.dec;meta.maindoubleindexednullableplx_valueParallax from Simbadmaspos.parallaxfloatnullableplx_bibcodeSource reference for the parallaxmeta.bib.bibcodecharnullableotypeSimbad object typemeta.code.classcharnullablegcns.rejectedThis is the catalogue of objects in the 8mas sample that were rejected for the main Gaia Catalogue of Nearby Stars as having a zero probability of being inside 100pc or indicated as a spurious astrometric solution.source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.mainlongindexedprimaryraICRS right ascension from Gaia eDR3.degpos.eq.ra;meta.maindoubleindexednullabledecICRS declination from Gaia eDR3.degpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch J2016.0. If looking for a distance, consider joining with gedr3dist.main and using the distances from there.maspos.parallaxfloatnullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablepmraProper motion in right ascension of the source in ICRS at J2016.0. This is the tangent plane projection (i.e., multiplied by cos(δ)) of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatnullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdecProper motion in declination at J2016.0.mas/yrpos.pm;pos.eq.decfloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_g_mean_flux_over_error.magphot.mag;em.opt;stat.meanfloatnullablephot_g_mean_flux_over_errorIntegrated mean G flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt;stat.meanfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_bp_mean_flux_over_error.magphot.mag;em.opt.Bfloatnullablephot_bp_mean_flux_over_errorIntegrated mean BP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Bfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. To obtain error estimates, see phot_rp_mean_flux_over_error.magphot.mag;em.opt.Rfloatnullablephot_rp_mean_flux_over_errorIntegrated mean RP flux divided by its error. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.stat.snr;phot.flux;em.opt.Rfloatnullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableruweRenormalized Unit Weight Error; this is a revised measure for the overall consistency of the solution as defined by GAIA-C3-TN-LU-LL-124-01. A suggested cut on this is RUWE <1.40) See the note for details.stat.weightfloatnullableipd_frac_multi_peakPercentage of distance windows in which a double peak was seen (high values mean high likelihood of a resolved double star).meta.code.multipshortadoptedrvAdopted Radial Velocitykm/sphys.veloc;pos.heliocentricfloatnullableadoptedrv_errorError in adopted RVkm/sstat.error;phys.veloc;pos.heliocentricfloatnullableadoptedrv_refnameBibcode for the source of the radial velocitymeta.bib.bibcodecharnullableradial_velocity_is_valid1 if this object has a radial velocity in eDR3, 0 otherwisemeta.code.qualshortgcns_probProbability that the astrometry is reliablestat.fit.goodnessfloatnullablewd_probprobability that this is a white dwarf.stat.likelihood;src.classfloatnullabledist_11st percentile of the distance PDF, used in GCNS selectionkpcstat.value;pos.distancefloatnullabledist_1616th percentile of the distance PDF (1 σ lower bound)kpcstat.value;pos.distancefloatnullabledist_50Median of the distance PDFkpcpos.distance;stat.medianfloatnullabledist_8484th percentile of the distance PDF (1 σ upper bound)kpcstat.value;pos.distancefloatnullablexcoord_50Median x coordinate in the Galactic frame assuming dist_50pcpos.cartesian.x;stat.medianfloatnullablexcoord_161 σ lower bound of Galactic frame x coordinatepcstat.value;pos.cartesian.xfloatnullablexcoord_841 σ upper bound of Galactic frame x coordinatepcstat.value;pos.cartesian.xfloatnullableycoord_50Median y coordinate in the Galactic frame assuming dist_50pcpos.cartesian.y;stat.medianfloatnullableycoord_161 σ lower bound of Galactic frame y coordinatepcstat.value;pos.cartesian.yfloatnullableycoord_841 σ upper bound of Galactic frame y coordinatepcstat.value;pos.cartesian.yfloatnullablezcoord_50Median z coordinate in the Galactic frame assuming dist_50pcpos.cartesian.z;stat.medianfloatnullablezcoord_161 σ lower bound of Galactic frame z coordinatepcstat.value;pos.cartesian.zfloatnullablezcoord_841 σ upper bound of Galactic frame z coordinatepcstat.value;pos.cartesian.zfloatnullableuvel_50Median velocity u in the Galactic frame, direction positive xkm/sphys.veloc;pos.cartesian.x;stat.medianfloatnullableuvel_161 σ lower bound for ukm/sstat.value;phys.veloc;pos.cartesian.xfloatnullableuvel_841 σ upper bound for ukm/sstat.value;phys.veloc;pos.cartesian.xfloatnullablevvel_50Median velocity v in the Galactic frame, direction positive ykm/sphys.veloc;pos.cartesian.y;stat.medianfloatnullablevvel_161 σ lower bound for vkm/sstat.value;phys.veloc;pos.cartesian.yfloatnullablevvel_841 σ upper bound for vkm/sstat.value;phys.veloc;pos.cartesian.yfloatnullablewvel_50Median velocity w in the Galactic frame, direction positive zkm/sphys.veloc;pos.cartesian.z;stat.medianfloatnullablewvel_161 σ lower bound for wkm/sstat.value;phys.veloc;pos.cartesian.zfloatnullablewvel_841 σ upper bound for wkm/sstat.value;phys.veloc;pos.cartesian.zfloatnullablename_gunnObject Name from PanSTARRS/SDSS/SkyMapper surveymeta.id.crosscharnullablerefname_gunnReference for the source of the Gunn photometrymeta.bib.bibcodecharnullablegmag_gunnGunn G band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Vfloatnullablee_gmag_gunnUncertainty in G band magnitudemagstat.error;phot.mag;em.opt.Vfloatnullablermag_gunnGunn R band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Rfloatnullablee_rmag_gunnUncertainty in R band magnitudemagstat.error;phot.mag;em.opt.Rfloatnullableimag_gunnGunn I band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Ifloatnullablee_imag_gunnUncertainty in I band magnitudemagstat.error;phot.mag;em.opt.Ifloatnullablezmag_gunnGunn Z band magnitude (when from SDSS, g, when from Skymapper, g_psf)magphot.mag;em.opt.Ifloatnullablee_zmag_gunnUncertainty in Z band magnitudemagstat.error;phot.mag;em.opt.Ifloatnullablename_2massName of this object in 2MASSmeta.id.crosscharnullablej_m_2mass2MASS J band magnitudemagphot.mag;em.IR.Jfloatnullablej_msig_2massUncertainty in 2MASS J band magnitudemagstat.error;phot.mag;em.IR.Jfloatnullableh_m_2mass2MASS H band magnitudemagphot.mag;em.IR.Hfloatnullableh_msig_2massUncertainty in 2MASS H band magnitudemagstat.error;phot.mag;em.IR.Hfloatnullablek_m_2mass2MASS K band magnitudemagphot.mag;em.IR.Kfloatnullablek_msig_2massUncertainty in 2MASS K band magnitudemagstat.error;phot.mag;em.IR.Kfloatnullablename_wiseName of this object in WISEmeta.id.crosscharnullablew1mpro_pm_wiseCATWISE W1 band magnitudemagphot.mag;em.IR.3-4umfloatnullablew1sigmpro_pm_wiseUncertainty in CATWISE W1 band magnitudemagstat.error;phot.mag;em.IR.3-4umfloatnullablew2mpro_pm_wiseCATWISE W2 band magnitudemagphot.mag;em.IR.4-8umfloatnullablew2sigmpro_pm_wiseUncertainty in CATWISE W2 band magnitudemagstat.error;phot.mag;em.IR.4-8umfloatnullablew3mpro_wiseCATWISE W3 band magnitudemagphot.mag;em.IR.8-15umfloatnullablew3sigmpro_wiseUncertainty in CATWISE W3 band magnitudemagstat.error;phot.mag;em.IR.8-15umfloatnullablew4mpro_wiseALLWISE W4 band magnitudemagphot.mag;em.IR.15-30umfloatnullablew4sigmpro_wiseUncertainty in ALLWISE W4 band magnitudemagstat.error;phot.mag;em.IR.15-30umfloatnullablegcns.resolvedss Resolved binary candidates in the GCNS catalogue as discussed in https://doi.org/10.1051/0004-6361/202039498, “stellar multiplicity: resolved systems”. You probably want to join this table to gaia.edr3lite using source_id1 and/or source_id2.19176source_id1Gaia EDR3 source_id of the primary starmeta.id.partlongsource_id2Gaia EDR3 source_id of secondary startmeta.id.partlongseparationAngular separation of the two sources.arcsecpos.angDistancefloatnullablemag_diffG magnitude difference between the two componentsmagphot.mag;arith.diff;em.opt.Vfloatnullableproj_sepProjected separation of the pairAUphys.sizefloatnullablebin1 if the system is probably made up of more than two stars, 0 otherwise.meta.code.multipshortbound1 if the system is probably gravitationally bound, 0 otherwisemeta.codeshortgedr3auto This is a table that simply gives, for each object in Gaia eDR3, the identifier of its closest neighbour together with the distance of the pair.gedr3auto.main This is a table that simply gives, for each object in Gaia eDR3, the identifier of its closest neighbour together with the distance of the pair.1900000000source_idGaia DR3 unique source identifier. Note that this *cannot* be matched against the DR1 or DR2 source_ids.meta.id;meta.main1140056122685444.587914001619745e+174.2821585696544517e+186.707246776001982e+1869175222244162801921.0longindexedprimarypartner_idIdentifier of the closest eDR3 objectmeta.id.assoc527421984520964.587913976653037e+174.282158707093594e+186.707246727208914e+1869175248056903676161.0longindexeddistThe estimated distance between the two objects. No attempt is made to furnish this with an error estimate.degpos.angDistance5e-050.0002413970.001048660.00709580.04180311doubleindexednullablehdgaia This is the Henry Draper catalog (HD, Cannon & Pickering 1918-1924) as distributed by the Astronomical Data Center in 1989 (Vizier III/135A), with Gaia DR2 source_ids and positions added. The link to modern Gaia DR2 was done through Fabricius et al's match between HD and Tycho 2 (Vizier IV/25), TGAS to match Tycho 2 and Gaia DR1, and Gaia DR2 to match against Gaia DR1.hdgaia.main This is the Henry Draper catalog (HD, Cannon & Pickering 1918-1924) as distributed by the Astronomical Data Center in 1989 (Vizier III/135A), with Gaia DR2 source_ids and positions added. The link to modern Gaia DR2 was done through Fabricius et al's match between HD and Tycho 2 (Vizier IV/25), TGAS to match Tycho 2 and Gaia DR1, and Gaia DR2 to match against Gaia DR1.272150hdHD number for this objectmeta.id;meta.main8165.469999999999136075.5263985.529999999971.0intindexedprimarydmDurchmusterung identifier, taken either from the Bonner Durchmusterung (BD), Cordoba Durchmusterung (CD), or Cape Photographic Durchmusterung (CPD); stars not given in any of them are referenced by their AGK number.meta.id.crosscharnullablera_origOriginal right ascension for equinox J1900.0. Note that this position is only good to about an arcminute.pos.eq.racharnullabledec_origOriginal declination for equinox J1900.0. Note that this position is only good to about an arcminute.pos.eq.deccharnullablera_orig_2000Original right ascension for equinox J2000.0 (precession done by DC staff). Note that this position is only good to about an arcminute.pos.eq.ra0.00095306217.3102173.097344.624359.9911floatnullabledec_orig_2000Original declination for equinox J2000.0 (precession done by DC staff). Note that this position is only good to about an arcminute.pos.eq.dec-89.833-70.8263-11.089661.524889.56961floatnullablemv_meas'0' if the m_v is a measured value, '1' if it's a value inferred from m_pg and the spectral type.meta.codecharm_vPhotovisual magnitude or the star, except for magnitudes >= 20, which are object type flags (see note).magphot.mag;em.opt.V-1.586.338.910.7500.856987floatindexednullablemv_combC if m_v is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise.meta.codecharnullablempg_meas'0' if the m_pg is a measured value, '1' if it's a value inferred from m_v and the spectral type.meta.codecharm_pgPhotographic magnitude or the star, except for magnitudes >= 20, which are object type flags (see note).magphot.mag;em.opt.B-1.5809.511.5500.994984floatnullablempg_combC if m_pg is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise.meta.codecharnullablespectralSpectral type, given in upper and lower case as in the published catalog.src.sptypecharindexednullablepg_intensityPhotographic intensity of the spectrum estimated by Annie Cannon. The faintest spectra which could be classified with certainty were assigned a value of 1, while the densest are given as 10. For stars having two intensities in the published catalog, only the first is given here.meta.code.qual01.03.08.0140.8056476shortnullableremarksRemarks. See note for what the letters mean.meta.codecharnullablen_hdNumber of HD stars matched to a Tycho 2 source by Fabricius et al, 2002A&A...386..709F.meta.number11.01.01.020.9364578shortnullablen_tycNumber of Tycho 2 stars matched to a HD source by Fabricius et al, 2002A&A...386..709F.meta.number11.01.01.020.9364578shortnullablesource_idGaia DR2 source_id matching the HD object through Fabricius' Tycho 2 match and Gaia DR2's tycho2_best_neighbour. For four ambiguous matches, a unique match was randomly chosen (see reference URL).meta.id.cross76321576903683.777458606843629e+174.08509149002637e+186.740768604212051e+1869175049758244692480.9364578longnullablesource_id3Gaia eDR3 source_id matching the HD object through Fabricius' Tycho 2 match and Gaia DR2's tycho2_best_neighbour, and then Gaia eDR3's dr2_best_neighbour.meta.id.cross76321576903683.7773162338312064e+174.0850844806402734e+186.740770681515457e+1869175049758244692480.9364358longnullablegaia_raICRS Right Ascension from Gaia eDR3 (i.e., Epoch J2016)degpos.eq.ra;meta.main0.00043482517.504174.243344.576359.9930.936436doubleindexednullablegaia_decICRS Declination from Gaia eDR3 (i.e., Epoch J2016)degpos.eq.dec;meta.main-89.8312-70.7928-11.563261.272689.56950.936436doubleindexednullablehiicounter A table containing reference data for HII regions. We also give a source code to compute abundances and electron temperatures in HII regions from strong emission lines.hiicounter.data A table containing reference data for HII regions. We also give a source code to compute abundances and electron temperatures in HII regions from strong emission lines.414identIdentifier of the HII region in this catalogmeta.id;meta.main113.389999999999999207.5401.614141.0intlogr3Log of [OIII] R_3 line intensity relative to Hβspect.line.intensity;arith.ratio-1.057-0.274470.7440.995831.0911floatnullablelogr2Log of [OII] R_2 line intensity relative to Hβspect.line.intensity;arith.ratio-0.662-0.453870.2070.545660.6531floatnullablelogn2Log of [NII] N_2 line intensity relative to Hβspect.line.intensity;arith.ratio-1.973-1.762-0.8980.120490.3331floatnullablelogs2Log of [SII] S_2 line intensity relative to Hβspect.line.intensity;arith.ratio-1.509-1.2647-0.6135-0.16639-0.0581floatnullableo_hT_e-based oxygen abundance given as 12+log(O/H)phys.abund;arith.ratio7.097.28128.078.558.761floatnullablen_hT_e-based nitrogen abundance given as 12+log(N/H)phys.abund;arith.ratio5.635.89396.6457.81618.571floatnullablet3Electron temperature derived as given in t3src, reduced to t_3([O III])Kphys.temperature.electron410065391310019461215001floatnullablet3srcLines used for determination of t_3meta.code;phys.temperature.electroncharnullableregion_nameName of the HII region.meta.id;srccharnullablesrcReference to the source of the data quoted.meta.bib.bibcodecharnullablehostalphaICRS RA of host object (from Simbad)pos.eq.ra;meta.main0.4923375.0965164.446294.882354.5610.833333floatindexednullablehostdeltaICRS Dec of host object (from Simbad)pos.eq.dec;meta.main-66.4983-41.37636.1727869.192475.62780.833333floatindexednullablehppunion GAVO's historical photographic plate archive (GHHPA) is a collection of various digitized historical photographic plates. It currently exposes: * the scans of plates of selected Kapteyn special fields obtained at Potsdam * the Palomar-Leiden Trojan surveys, 1960-1977, * a collection of plates obtained at Boyden Station, South Africa, kept at various German observatories. Other plate collections kept by GAVO include the Heidelberg Digitized Astronomical Plates HDAP, ivo://org.gavo.dc/lswscans/res/positions/siap, and the APPLAUSE database from Potsdam.hppunion.main GAVO's historical photographic plate archive (GHHPA) is a collection of various digitized historical photographic plates. It currently exposes: * the scans of plates of selected Kapteyn special fields obtained at Potsdam * the Palomar-Leiden Trojan surveys, 1960-1977, * a collection of plates obtained at Boyden Station, South Africa, kept at various German observatories. Other plate collections kept by GAVO include the Heidelberg Digitized Astronomical Plates HDAP, ivo://org.gavo.dc/lswscans/res/positions/siap, and the APPLAUSE database from Potsdam.1897accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size6837120096433920.0403292160.01544757120.015447571201.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra0.05940231.94028166.321349.57359.470.96679doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec-77.684-76.4629-3.6298417.685631.40480.96679doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure1886719069.141037.448070.148452.31doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.020.96678966intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020000.96679floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median3.6e-073.637e-074.1e-075.3e-076.93e-070.991039floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max3.9e-073.9e-075e-076.6e-079.4e-070.991039floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min3.15e-073.2055e-073.4e-074.6e-075.4e-070.991039floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableobjectObject being observed, Simbad-resolvable formmeta.idcharnullablepub_didDataset identifier assigned by the publisher.meta.ref.urlcharnullabledatalink_urlURL of a datalink document (cutout service, ancillary data) for this dataset.charnullablehsoy HSOY is a catalog of 583'001'653 objects with precise astrometry based on PPMXL and Gaia DR1. Typical formal errors at mean epoch in proper motion are below 1 mas/yr for objects brighter than 10 mag, and about 5 mas/yr at the faint end (about 20 mag). South of -30 degrees, astrometry is significantly worse. HSOY also contains, where available, USNO-B, Gaia, and 2MASS photometry. HSOY's positions and proper motions are given for epoch J2000. The catalog becomes severely incomplete faintwards of 16 mag in the G-band. The mean epochs are typically very close to Gaia's J2015. HSOY still contains about 0.7% spurious close "binaries" (non-matched stars) from the original USNO-B (marked with non-NULL clone). Also, failed matches within Gaia DR1 contribute another 1.5% spurious pairs (marked with non-NULL comp). In both cases, astrometry presumably is sub-standard. More information is available at http://dc.g-vo.org/hsoy.hsoy.main HSOY is a catalog of 583'001'653 objects with precise astrometry based on PPMXL and Gaia DR1. Typical formal errors at mean epoch in proper motion are below 1 mas/yr for objects brighter than 10 mag, and about 5 mas/yr at the faint end (about 20 mag). South of -30 degrees, astrometry is significantly worse. HSOY also contains, where available, USNO-B, Gaia, and 2MASS photometry. HSOY's positions and proper motions are given for epoch J2000. The catalog becomes severely incomplete faintwards of 16 mag in the G-band. The mean epochs are typically very close to Gaia's J2015. HSOY still contains about 0.7% spurious close "binaries" (non-matched stars) from the original USNO-B (marked with non-NULL clone). Also, failed matches within Gaia DR1 contribute another 1.5% spurious pairs (marked with non-NULL comp). In both cases, astrometry presumably is sub-standard. More information is available at http://dc.g-vo.org/hsoy.590000000ipixThe PPMXL object identifier, which in turn is the q3c ipix of the original USNO-B object; for HSOY, only (ipix, comp) is a unique identifier (primary key). The recommended identifier form is 'HSOY ipix.comp', where comp=0 for NULL comps. This is what the SCS generates.meta.id.cross68187852794531.4555397969262336e+174.897678929650011e+186.544739885363848e+1869175110039938228571.0longindexedcompIf non-null this indicates that multiple Gaia objects matched the PPMXL object; this may indicate bona fide multiple stars, but more likely is due to failed matching of Gaia observations at different epochs. In both cases, proper motions must be used with care. The index is artificial, i.e., no primary, secondary, etc, is implied. ipix+comp together are a primary key to hsoy.main.meta.code.multip11.02.02.040.008333711shortnullableraj2000Right Ascension J2000.0, epoch 2000.0degpos.eq.ra;meta.main6e-0620.8815237.901340.5833601doubleindexednullabledej2000Declination J2000.0, epoch 2000.0degpos.eq.dec;meta.main-89.886-70.7159-17.90564.550289.93921doubleindexednullablee_raepraMean error in RA*cos(delta) at mean epochdegstat.error;pos.eq.ra;meta.main2.78e-071.75e-053.11e-054.53e-055.75e-051floatnullablee_deepdeMean error in Dec at mean epochdegstat.error;pos.eq.dec;meta.main2.78e-071.75e-053.14e-054.53e-055.69e-051floatnullablepmraProper Motion in RA*cos(delta)deg/yrpos.pm;pos.eq.ra-0.0026833-3.6267e-05-4.6389e-073.1322e-050.00271881floatnullablepmdeProper Motion in Decdeg/yrpos.pm;pos.eq.dec-0.002712-4.03e-05-7.8056e-073.6792e-050.0027711floatnullablee_pmraMean error in pmRA*cos(delta)deg/yrstat.error;pos.pm;pos.eq.ra5.56e-081.06e-062.11e-066.86e-062.48e-051floatnullablee_pmdeMean error in pmDEdeg/yrstat.error;pos.pm;pos.eq.dec2.78e-081.06e-062.11e-066.86e-062.48e-051floatnullableepraMean Epoch (RA)yrtime.epoch;pos.eq.ra1924.171968.311984.651995.592005.131floatnullableepdeMean Epoch (Dec)yrtime.epoch;pos.eq.dec1922.621968.31984.651995.62005.131floatnullablejmagJ selected default magnitude from 2MASSmagphot.mag;em.IR.J-1.31411.71715.52116.79621.7490.453138floatindexednullablee_jmagJ total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0660.1639.9990.446147floatnullablehmagH selected default magnitude from 2MASSmagphot.mag;em.IR.H-2.23511.0314.96116.28220.1470.453138floatnullablee_hmagH total magnitude uncertaintymagstat.error;phot.mag;em.IR.H00.0220.0780.2139.9980.419335floatnullablekmagK_s selected default magnitude from 2MASSmagphot.mag;em.IR.K-2.66310.78614.75516.23219.8720.453138floatindexednullablee_kmagK_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K00.0210.0890.2459.9990.353952floatnullableb1magB mag from USNO-B, first epochmagphot.mag;em.opt.B-0.6214.7419.4321.0464.880.400937floatnullableb2magB mag from USNO-B, second epochmagphot.mag;em.opt.B-0.4415.2219.2121.665.380.853922floatnullabler1magR mag from USNO-B, first epochmagphot.mag;em.opt.R-1.2213.817.9220.0465.430.793746floatnullabler2magR mag from USNO-B, second epochmagphot.mag;em.opt.R0.1714.2118.2420.965.450.806482floatnullableimagI mag from USNO-Bmagphot.mag;em.opt.I-0.6413.1617.2518.9865.120.73584floatnullablemagsurveysSurveys the USNO-B magnitudes are taken frommeta.codecharnullablenobsNumber of observations contributing to this column (always nobs(ppmxl)+1)meta.number;obs33.06.07.0170.99978745shortnullablegaia_idUnique source identifiermeta.id343598963202.8057349365717197e+174.2738585968976384e+186.723103967053457e+1869175289932832044801.0longindexednullablephot_g_mean_magMean magnitude in the G band from Gaia DR1. Magnitudes for which err_flux/flux>0.1 have been dropped.magphot.mag;em.opt;stat.mean3.3265114.0318.112820.115325.81630.999862floatindexednullablee_phot_g_mean_magEstimated error in Gaia G-band magnitude. This is estimated as 1.09*err_flux/flux which is good as a symmetric 1 σ-error of the magnitude to at least within a few percent when err_flux/flux is smaller than 0.1, as it is for the HSOY objects.s**-1stat.error;phot.mag;em.opt.V5.05882e-050.0005965640.004422870.02065550.1090.999862floatnullablecloneIf 1, more than one PPMXL object matched to this Gaia object (i.e.: proper motion is probably wrong, any apparent duplicity is probably spurious). This is normally due to failed matching of objects from different plates in USNO-B.meta.code.qual11.01.01.010.049893033shortnullableno_sc1 if this object had no match within 3 arcseconds in SuperCosmos at J2000. It is very likely that it is not a real object. NOTE: False is encoded as NULL in the database; to exclude objects without a supercosmos match, write no_sc IS NULL.meta.code.qual0.0shortnullableinflightThe infinite lightcurve is a continuously calculated microlensing lightcurve, simulating the light variation of a quasar due to an intervening star field.inflight.dataThe raw lensing data as well as relative intensities computed for various source profiles.1200000lineDistance indicator in 0.01 Einstein radiipos.distanceintindexeddataBase64 encoded 8-bit image datacharnullablesrcnameName of file this line came frommeta.refcharnullablegauss01Magnification for a Gauss disk source with r=1magphot.mag;arith.difffloatnullablegauss02Magnification for a Gauss disk source with r=2magphot.mag;arith.difffloatnullablegauss04Magnification for a Gauss disk source with r=4magphot.mag;arith.difffloatnullablegauss06Magnification for a Gauss disk source with r=6magphot.mag;arith.difffloatnullablegauss08Magnification for a Gauss disk source with r=8magphot.mag;arith.difffloatnullablegauss10Magnification for a Gauss disk source with r=10magphot.mag;arith.difffloatnullablegauss12Magnification for a Gauss disk source with r=12magphot.mag;arith.difffloatnullablegauss16Magnification for a Gauss disk source with r=16magphot.mag;arith.difffloatnullablegauss20Magnification for a Gauss disk source with r=20magphot.mag;arith.difffloatnullablegauss24Magnification for a Gauss disk source with r=24magphot.mag;arith.difffloatnullablegauss28Magnification for a Gauss disk source with r=28magphot.mag;arith.difffloatnullablegauss32Magnification for a Gauss disk source with r=32magphot.mag;arith.difffloatnullablegauss40Magnification for a Gauss disk source with r=40magphot.mag;arith.difffloatnullablegauss48Magnification for a Gauss disk source with r=48magphot.mag;arith.difffloatnullablethin01Amplification of a thin disk of r=1magphot.mag;arith.diff;meta.mainfloatnullablethin02Magnification for thin disk with r=2magphot.mag;arith.difffloatnullablethin04Magnification for thin disk with r=4magphot.mag;arith.difffloatnullablethin06Magnification for thin disk with r=6magphot.mag;arith.difffloatnullablethin08Magnification for thin disk with r=8magphot.mag;arith.difffloatnullablethin10Magnification for thin disk with r=10magphot.mag;arith.difffloatnullablethin12Magnification for thin disk with r=12magphot.mag;arith.difffloatnullablethin16Magnification for thin disk with r=16magphot.mag;arith.difffloatnullablethin20Magnification for thin disk with r=20magphot.mag;arith.difffloatnullablethin24Magnification for thin disk with r=24magphot.mag;arith.difffloatnullablethin28Magnification for thin disk with r=28magphot.mag;arith.difffloatnullablek2c9vst The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the microlensing program 097.C-0261(A) using the ESO VLT Survey Telescope (VST) was to monitor the superstamp (i.e., the actually downloaded region of K2/C9) in service mode for improving the event coverage and securing some color-information. Due to weather conditions, the majority of images were taken in the red band. These are part of the present release. The exact pointing strategy was adjusted to cover the superstamp with 6 pointings and to contain as many microlensing events from earlier seasons as possible. In addition, a two-point dither was requested to reduce the impact of bad pixels and detector gaps. Consequently, some events were getting more coverage and have been observed with different CCDs. The large footprint of roughly 1 square degree and the complementary weather conditions at Cerro Paranal have lead to the coverage of 147 events (this resource's events table), but ~60 of those were already at baseline.k2c9vst.events The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the microlensing program 097.C-0261(A) using the ESO VLT Survey Telescope (VST) was to monitor the superstamp (i.e., the actually downloaded region of K2/C9) in service mode for improving the event coverage and securing some color-information. Due to weather conditions, the majority of images were taken in the red band. These are part of the present release. The exact pointing strategy was adjusted to cover the superstamp with 6 pointings and to contain as many microlensing events from earlier seasons as possible. In addition, a two-point dither was requested to reduce the impact of bad pixels and detector gaps. Consequently, some events were getting more coverage and have been observed with different CCDs. The large footprint of roughly 1 square degree and the complementary weather conditions at Cerro Paranal have lead to the coverage of 147 events (this resource's events table), but ~60 of those were already at baseline.725event_idEvent name as specified by OGLE (http://ogle.astrouw.edu.pl/ogle4/ews/2015/ews.html) or MOA (http://www.phys.canterbury.ac.nz/moa/). Some event ids actually reference the same object. These have otherwise identical records.meta.id;meta.maincharindexedprimaryraj2000Right ascension of the event source as reported by the OGLE or MOAdegpos.eq.ra;meta.main263.539265.064269.932274.859275.3711doublenullabledej2000Right ascension of the event source as reported by the OGLE or MOAdegpos.eq.dec;meta.main-29.2584-29.0909-27.7676-22.3138-21.07611doublenullablet_alertHJD of alert release.dtime.release2.45669e+062.45721e+062.45752e+062.45764e+062.45766e+061doublenullablet_0Time of largest magnification estimated from a fit assuming a gravitational lens event of pointlike source and lens.dtime.duration;stat.fit2.45679e+062.45723e+062.45753e+062.45765e+062.45941e+061doublenullablet_eEvent timescale (Einstein time assuming a gravitational lens event of pointlike source and lens).dtime.duration0.0492.6035227.18375.561.35003e+061doublenullableu_0Impact parameter in units of Einstein radii.src.impactParam000.2311.83641.2561floatnullablea_0Maximum magnification.phot.flux;arith.ratio1.0311.092524.2834460.96852060.929655floatnullableflagsBitmask for flags: bit 0 -- during campaign; bit 1: In footprint (i.e., Kepler data could be available); bit 2: In superstamp (i.e., Kepler data available).meta.code22.7199999999999997.07.071.0shortk2c9vst.photpoints The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the microlensing program 097.C-0261(A) using the ESO VLT Survey Telescope (VST) was to monitor the superstamp (i.e., the actually downloaded region of K2/C9) in service mode for improving the event coverage and securing some color-information. Due to weather conditions, the majority of images were taken in the red band. These are part of the present release. The exact pointing strategy was adjusted to cover the superstamp with 6 pointings and to contain as many microlensing events from earlier seasons as possible. In addition, a two-point dither was requested to reduce the impact of bad pixels and detector gaps. Consequently, some events were getting more coverage and have been observed with different CCDs. The large footprint of roughly 1 square degree and the complementary weather conditions at Cerro Paranal have lead to the coverage of 147 events (this resource's events table), but ~60 of those were already at baseline.9384accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size30157792.022857.044613.0447301.0longnullabledidLocal dataset identifier for the lightcurve this point belongs to.meta.id;meta.maincharindexednullableevent_idAssociated Eventcharnullableobs_timeTime this photometry corresponds to.dtime.epoch2.45749e+062.45749e+062.45753e+062.45756e+062.45756e+061doublenullablephotSDSS r-band instrumental magnitude (warning: zeropoint may be off several mag).magphot.mag;em.opt.R15.503217.204320.206722.557128.40631doublenullableimageVST image this point was taken from. The raw images are available at http://archive.eso.org/wdb/wdb/eso/eso_archive_main/query?prog_id=097.C-0261(A)meta.ref;meta.filecharnullabledfDifference flux as defined by 2008MNRAS.386L..77Baduphot.flux-105651-43555.728.96013777.14773121doublenullablee_dfError in difference flux.adustat.error;phot.flux65.203797.5333173.61322.863535.9671floatnullablerfReference flux as defined by 2008MNRAS.386L..77Baduphot.flux421.672765.7484975.661692082986841doublenullablee_rfError in reference Fluxadustat.error;phot.flux153.848191.575509.7771185.641237.551floatnullablee_photError in SDSS r-band instrumental magnitude.magstat.error;phot.mag0.001499150.00394050.03743750.339084465.2711floatnullableexp_timeExposure time.stime.duration;obs.exposure60606060601floatnullablefwhmFWHM of the point spread function averaged over all stars on the subimage used.arcsecphys.angSize;instr.det.psf2.1142.948585.154157.022179.44961floatnullablesky_backgroundMedian sky background flux.aduinstr.background98.9249150.865236.323849.8761630.81floatnullablephot_scale_factorScale factor according to 2008MNRAS.386L..77B; if small, photometry was obtained under suboptimal atmospheric transparency.0.07110380.4321640.9721891.003931.113121floatnullablechi2_pxSee 2008MNRAS.386L..77B, sect. 2.1stat.fit.chi200.6315350.8963852.589087.913921floatnullabledxPixel offset of frame wrt. the reference frame, x directionpixelpos.cartesian.x;arith.diff-29.7382-5.58953-0.0292556.1255930.25251floatnullabledyPixel offset of frame wrt. the reference frame, y directionpixelpos.cartesian.y;arith.diff-27.6162-5.46111-0.672526.0649625.06951floatnullablecorr_coeffCoefficients of correction polynomial for frame: TBDfloatnullablek2c9vst.eventsevent_idevent_idk2c9vst.timeseries The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the microlensing program 097.C-0261(A) using the ESO VLT Survey Telescope (VST) was to monitor the superstamp (i.e., the actually downloaded region of K2/C9) in service mode for improving the event coverage and securing some color-information. Due to weather conditions, the majority of images were taken in the red band. These are part of the present release. The exact pointing strategy was adjusted to cover the superstamp with 6 pointings and to contain as many microlensing events from earlier seasons as possible. In addition, a two-point dither was requested to reduce the impact of bad pixels and detector gaps. Consequently, some events were getting more coverage and have been observed with different CCDs. The large footprint of roughly 1 square degree and the complementary weather conditions at Cerro Paranal have lead to the coverage of 147 events (this resource's events table), but ~60 of those were already at baseline.119accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size2000020000.020000.020000.0200001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshift0floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNR0floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.001148230.001190150.001415750.001488040.001512291floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value2.45742e+062.45746e+062.45751e+062.45764e+062.45941e+061doublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent3.96318e+064.27799e+065.77641e+065.77652e+065.77652e+061floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value5.8e-075.8e-075.8e-075.8e-075.8e-071floatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extent1.5e-071.5e-071.5e-071.5e-071.5e-071floatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start5e-075e-075e-075e-075e-071floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop6.5e-076.5e-076.5e-076.5e-076.5e-071floatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Length1122.5473.0171.459999999999981761.0intnullablessa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typecharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharnullablessa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectioncharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcecharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxadustat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatError121.276126.849171.234292.205442.9821floatnullablessa_fluxsyserrorSystematic error in fluxadustat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysError0floatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.Calibrationcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSize0floatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatError0floatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysError0floatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.Calibrationcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolution0floatnullablet_min_mjd(Approximate) earliest timestamp in dataset.dtime.start;obsts:time.start57490.357490.357490.357505.857509.41doubleindexednullablet_max_mjd(Approximate) latest timestamp in dataset.dtime.end;obsts:time.end57551.457555.257557.157557.257557.21doubleindexednullablet_0Time of largest magnification estimated from a fit assuming a gravitational lens event of pointlike source and lens.dtime.duration;stat.fit2.45742e+062.45746e+062.45751e+062.45764e+062.45941e+061doublenullablelamost6 LAMOST, the The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (or Guoshoujing Telescope) is an instrument tailored for producing large number of optical medium- and low-resolution spectra. Here, we publish both the medium (MRS) and low (LRS) resolution spectra from Data Release 6, http://dr6.lamost.org/v2/, to the Virtual Observatory.lamost6.ssa_lrsSSA-compliant metadata for LAMOST DR6 low resolution spectra; this data is also availble through Obscore; the collection name there is LAMOST6 LRS.10000000accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size100000100000.0100000.0100000.01000001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift as estimated by the LAMOST pipeline.src.redshiftssa:Target.Redshift-0.017-0.00037705-2.20152e-050.0007719715.598880.955241floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrMedian signal to noise ratio over all pixel, computed as flux/sqrt(variance)stat.snrssa:Derived.SNR02.17626.966200.1389991floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value55858559165701358154582561doubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcountcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionLAMOST6 MRScharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationRELATIVEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullableobsidUnique identifier for the observation; LAMOST observations typically result in multiple spectra.meta.id;obs10100719009070.59283506073.0642005059.416647162501.0longdesignationTarget Designation (IAU style)meta.idcharnullableplanidIdentifier of the observation planmeta.id;obs.proposalcharnullablespidIdentifier of the Spectragraph that took the source spectrum.meta.id;instr11.09.016.0161.0shortfiberidIdentifier of the fiber used to take the source spectrummeta.id;instr19.0126.0242.02501.0shortra_obsICRS right ascension of the fiber pointing (can be different from ra for bright sources).degpos.eq.ra012.2051118.6341.0383601doublenullabledec_obsICRS declination of the fiber pointingdegpos.eq.dec-9.93339-2.5764627.507956.082583.01521doublenullableobjtypeObject type: star, k2star, fs, rvcandi, galmeta.code.classcharnullablemagtypeDesignation of the bands of the magnitudes in mag_arr; this is not easy to parse by a machine, sorry.meta.codecharnullablemag_arrAn array of derived magnitudes. See mag_types for the bands these magnitudes are intended for.phot.magfloatnullablefibertypeFiber Type of target (one of Obj, Sky, F-std, Unused, PosErr, Dead)meta.code;instrcharnullabletarget_commentVarious comments (e.g., an external target id).meta.notecharnullableoffset_vOffset of the observation from the target coordinate (these are added for bright objects to prevent saturation).arcsecinstr.offset0.260.862.85.38990.0172031floatnullableraICRS right ascension for this object from input cataloguedegpos.eq.ra;meta.main012.2051118.6341.0373601doublenullabledecICRS declination for this object from input cataloguedegpos.eq.dec;meta.main-9.93339-2.5764627.507956.082583.01521doublenullablez_errError in ssa_redshift as estimated by the LAMOST pipeline.stat.error;src.redshift-64.08e-061.67449e-050.0001171e+080.952424floatnullablelamost6.ssa_mrsSSA-compliant metadata for LAMOST DR6 medium resolution spectra; this data is also availble through Obscore; the collection name there is LAMOST6 MRS.5900000accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size100000100000.0100000.0100000.01000001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrMedian signal to noise ratio over all pixel, computed as flux/sqrt(variance)stat.snrssa:Derived.SNR0011.97141.799991floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value58024580275811858268582731doubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start4.91e-074.91e-076.28e-076.28e-076.28e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop5.37e-075.37e-076.87e-076.87e-076.87e-071floatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcountcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionLAMOST6 LRScharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationRELATIVEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolution1.1e-111.1e-111.5e-111.5e-111.5e-111floatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.ResolutionfloatnullablemobsidUnique identifier for the medium resolution spectrum (most of these have multiple observations and include a coadded spectrum).meta.id;meta.maincharssa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullableobsidUnique identifier for the observation; LAMOST observations typically result in multiple spectra.meta.id;obs588902003590109148.0623301220.0666505112.06674162481.0longdesignationTarget Designation (IAU style)meta.idcharnullableplanidIdentifier of the observation planmeta.id;obs.proposalcharnullablespidIdentifier of the Spectragraph that took the source spectrum.meta.id;instr11.08.016.0161.0shortfiberidIdentifier of the fiber used to take the source spectrummeta.id;instr19.0125.0242.02501.0shortra_obsICRS right ascension of the fiber pointing (can be different from ra for bright sources).degpos.eq.ra0.002717414.8771116.07353.5853601doublenullabledec_obsICRS declination of the fiber pointingdegpos.eq.dec-9.19667-1.3948323.701660.571467.70411doublenullableobjtypeObject type: star, k2star, fs, rvcandi, galmeta.code.classcharnullablemagtypeDesignation of the bands of the magnitudes in mag_arr; this is not easy to parse by a machine, sorry.meta.codecharnullablemag_arrAn array of derived magnitudes. See mag_types for the bands these magnitudes are intended for.phot.magfloatnullablefibertypeFiber Type of target (one of Obj, Sky, F-std, Unused, PosErr, Dead)meta.code;instrcharnullabletarget_commentVarious comments (e.g., an external target id).meta.notecharnullableoffset_vOffset of the observation from the target coordinate (these are added for bright objects to prevent saturation).arcsecinstr.offset0.320.52.133.543.640.000876441floatnullableraICRS right ascension for this object from input cataloguedegpos.eq.ra;meta.main0.002717414.8771116.07353.5853601doublenullabledecICRS declination for this object from input cataloguedegpos.eq.dec;meta.main-9.19667-1.3948323.701660.571467.70411doublenullablerv_b0Radial velocity estimated from the B spectrum after continuum removal.km/sspect.dopplerVeloc-599.99-221.88-8.26234.11599.990.723511floatnullablerv_b0_errError in rv_b0.km/sstat.error;spect.dopplerVeloc0.130.381.643.948.660.723511floatnullablerv_r0Radial velocity estimated from the R spectrum after continuum removal.km/sspect.dopplerVeloc-600-118-6.7695.366000.761535floatnullablerv_r0_errError in rv_r0.km/sstat.error;spect.dopplerVeloc0.220.432.37.5920.330.761535floatnullablerv_br0Radial velocity estimated from the B and R spectra after continuum removal.km/sspect.dopplerVeloc-600-90.48-7.7577.23599.980.709411floatnullablerv_br0_errError in rv_br0.km/sstat.error;spect.dopplerVeloc0.130.461.563.438.670.709411floatnullablerv_lasp0Radial velocity estimated from the LAMOST stellar parameter pipeline.km/sspect.dopplerVeloc-494.88-73.04-9.7559.3461.040.211467floatnullablerv_lasp0_errError in rv_lasp0.km/sstat.error;spect.dopplerVeloc0.040.511.032.3399.930.203657floatnullablerv_b1rv_b0 after zero-point correctionkm/sspect.dopplerVeloc-600.87-216.865-2.99239.657606.630.723511floatnullablerv_b1_errError in rv_b1.km/sstat.error;spect.dopplerVeloc0.130.831.854.058.740.723511floatnullablerv_r1rv_r0 after zero-point correctionkm/sspect.dopplerVeloc-602.81-113.718-2.4499.78605.770.761535floatnullablerv_r1_errError in rv_r1.km/sstat.error;spect.dopplerVeloc0.221.32.717.7220.360.761535floatnullablerv_br1rv_br0 after zero-point correctionkm/sspect.dopplerVeloc-600.3-85.28-2.5782.5606.570.709411floatnullablerv_br1_errError in rv_br1.km/sstat.error;spect.dopplerVeloc0.130.941.793.548.730.709411floatnullablerv_lasp1rv_lasp0 after zero-point correctionkm/sspect.dopplerVeloc-488-66.17-3.1865.79467.450.209013floatnullablerv_lasp1_errError in rv_lasp1.km/sstat.error;spect.dopplerVeloc0.040.711.38.8999990.208978floatnullablerv_b_flagFlag for RV extraction in the b band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template.meta.code.qual-128-128.00.00.031.0shortrv_r_flagFlag for RV extraction in the r band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template.meta.code.qual-128-128.00.00.031.0shortrv_br_flagFlag for RV extraction in the br band: 0 – no anomalies; 1 – too many bad pixels; 2 – radial velocity in excess of 450 km/s; 3 – low similarity with best-matched template.meta.code.qual-128-128.00.00.031.0shortcoadd1 if this is a co-added spectrummeta.code00.00.01.011.0shortfibermaskBitmask for fiber problems. See note for the meaning for the bits.meta.code.qual00.00.00.02351.0shortbad_b1 if this is a problematic B spectrum.meta.code00.00.00.011.0shortbad_r1 if this is a problematic R spectrum.meta.code00.00.00.011.0shortlife_td The LIFE Target Star Database contains information useful for the planned `LIFE mission`_ (mid-ir, nulling interferometer in space). It characterizes possible target systems including information about stellar, planetary and disk properties. The data itself is mainly a collection from different other catalogs. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. .. _LIFE mission: https://life-space-mission.com/life_td.disk_basic A list of all basic disk parameters. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 33object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main36403640.963656.03671.0436721.0intindexedprimaryrad_valueBlack body radius.AUphys.size.radius0.2711071.0522117.4933217.747226.4020.424242doublenullablerad_errRadius errorAUstat.error;phys.size.radius0.01006350.2568643.49267129.189142.7820.424242doublenullablerad_qualRadius quality (A:best, E:worst)meta.code.qual;phys.size.radiuscharnullablerad_relRadius relation defining upper / lower limit or exact measurement through '<' ,'>', and '='.phys.size.radius;arith.ratiocharnullablerad_source_idrefIdentifier of the source of the disk parameters.meta.ref239239.0239.0239.02391.0intnullablelife_td.objectobject_idrefobject_idlife_td.h_link This table links subordinate objects (e.g. a planets of a star, or a star in a multiple star system) to their parent objects. Contains only best link for each pair of objects. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 7733parent_object_idrefObject key (unstable, use only for joining to the other tables).meta.id.parent;meta.main1360.839999999999917365.021295.04220361.0intindexedprimarychild_object_idrefObject key (unstable, use only for joining to the other tables).meta.id1222.9199999999999612638.021455.08222171.0intindexedprimarymembershipMembership probability.meta.record100100.0100.0100.01000.01267296intnullableh_link_source_idrefIdentifier of the source of the relationship parameters.meta.ref125180.0197.0915.010291.0intindexedprimarylife_td.ident A list of the object identifiers. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 221142object_idrefObject key (unstable, use only for joining to the other tables).meta.id1210.08559.021266.76999999999222171.0intindexedprimaryidObject identifier.meta.idcharindexedprimaryid_source_idrefIdentifier of the source of the identifier parameter.meta.ref178179.0180.0197.010291.0intindexedprimarylife_td.mes_binary A list of the stellar multiplicitz measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 32636object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1483.010167.521307.95220681.0intindexedprimarybinary_flagBinary flag.meta.code.multipcharindexedprimarybinary_qualBinary quality (A:best, E:worst)meta.code.qualcharnullablebinary_source_idrefIdentifier of the source of the binary_flag parameter.meta.ref180180.0197.0568.05681.0intindexedprimarylife_td.objectobject_idrefobject_idlife_td.mes_h_link This table links subordinate objects (e.g. a planets of a star, or a star in a multiple star system) to their parent objects. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 8422parent_object_idrefObject key (unstable, use only for joining to the other tables).meta.id.parent;meta.main1342.2617053.021298.0220361.0intchild_object_idrefObject key (unstable, use only for joining to the other tables).meta.id1213.011673.021435.11222171.0intmembershipMembership probability.meta.record100100.0100.0100.01000.011636191intnullableh_link_source_idrefIdentifier of the source of the relationship parameters.meta.ref125180.0197.0891.369999999999910291.0intlife_td.mes_mass_pl A list of the planetary mass measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 1611object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main32169.08005.021672.2220321.0intmass_pl_valueMass'jupiterMass'phys.mass0.000190.003710.30460.57514.9151doublenullablemass_pl_err_maxUpper mass error'jupiterMass'stat.error;phys.mass4e-050.00040660.0154124.6878501.5350.883302doublenullablemass_pl_err_minLower mass error'jupiterMass'stat.error;phys.mass4e-050.00040660.014468924.6878501.5350.883302doublenullablemass_pl_qualMass quality (A:best, E:worst)meta.code.qual;phys.masscharnullablemass_pl_sini_flagMass sin(i) flag.meta.code.multipcharnullablemass_pl_source_idrefIdentifier of the source of the mass parameter.meta.ref194501.499999999999941025.01028.010281.0intlife_td.objectobject_idrefobject_idlife_td.mes_mass_st A list of the stellar mass measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 8321object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1302.799999999999958616.016284.199999999999220681.0intindexedprimarymass_st_valueObject mass.solMassphys.mass0.0780.0850.441.296215.41doublenullablemass_st_errObject mass error.solMassstat.error;phys.mass0doublenullablemass_st_qualMass quality (A:best, E:worst)meta.code.qual;phys.masscharnullablemass_st_source_idrefIdentifier of the source of the mass parameter.meta.ref;phys.mass467467.0467.0876.08761.0intindexedprimarylife_td.objectobject_idrefobject_idlife_td.mes_radius_st A list of the stellar radius measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 11120object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1417.148838.016280.0220681.0intindexedprimaryradius_st_valueObject radius.solRadphys.size.radius0.1010.120.4211.37985.058991doublenullableradius_st_errObject radius error.solRadstat.error;phys.size.radius0doublenullableradius_st_qualRadius quality (A:best, E:worst)meta.code.qual;phys.size.radiuscharnullableradius_st_source_idrefIdentifier of the source of the radius parameter.meta.ref;phys.size.radius467467.0467.0876.08761.0intindexedprimarylife_td.objectobject_idrefobject_idlife_td.mes_sep_ang A list of the stellar phys. separation measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 6895object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1376.017784.021300.0220361.0intsep_ang_valueAngular separation of binary.arcsecpos.angDistance00.110.7540.72999.91doublenullablesep_ang_errObject ang. separation error.arcsecstat.error;pos.angDistance0doublenullablesep_ang_obs_dateYear of observation.time.epoch;obs16901832.822006.02023.020251.0intnullablesep_ang_qualAng. separation quality (A:best, E:worst)meta.code.qual;pos.angDistancecharnullablesep_ang_source_idrefIdentifier of the source of the sep_ang parameter.meta.ref;pos.angDistance197197.0197.0197.01971.0intnullablelife_td.objectobject_idrefobject_idlife_td.mes_teff_st A list of the stellar effective temperature measurements. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 16132object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1451.938686.016280.0220681.0intindexedprimaryteff_st_valueObject effective temperature.Kphys.temperature.effective2350274034306180170001doublenullableteff_st_errObject effective temperature error.Kstat.error;phys.temperature.effective0doublenullableteff_st_qualEffective temperature quality (A:best, E:worst)meta.code.qual;phys.temperature.effectivecharnullableteff_st_source_idrefIdentifier of the source of the effective temperature parameter.meta.ref;phys.temperature.effective467467.0877.0878.08781.0intindexedprimarylife_td.objectobject_idrefobject_idlife_td.object A list of the astrophysical objects. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 3672object_idObject key (unstable, use only for joining to the other tables).meta.id;meta.main1111.131836.53561.8736721.0intindexedprimarytypeObject type (sy=multi-object system, st=star, pl=planet and di=disk).src.classcharnullablemain_idMain object identifier.meta.idcharidsAll identifiers of the object separated by '|'.meta.idcharlife_td.planet_basic A list of all basic planetary parameters. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 502object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1063.031709.53405.8536321.0intindexedprimarymass_pl_valueMass'jupiterMass'phys.mass0.000190.00369081.49564.0768514.9150.699537doublenullablemass_pl_err_maxUpper mass error'jupiterMass'stat.error;phys.mass4e-050.00040440.0575826.4356501.5350.628061doublenullablemass_pl_err_minLower mass error'jupiterMass'stat.error;phys.mass4e-050.00040440.05326.4356501.5350.628061doublenullablemass_pl_qualMass quality (A:best, E:worst)meta.code.qual;phys.masscharnullablemass_pl_sini_flagMass sin(i) flag.meta.code.multipcharnullablemass_pl_source_idrefIdentifier of the source of the mass parameter.meta.ref279551.01025.01028.010280.69953674intnullablelife_td.objectobject_idrefobject_idlife_td.provider A list of all the providers for the parameters in the other tables. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 6provider_nameName for the service through which the data was acquired.meta.bib.authorcharindexedprimaryprovider_urlService through which the data was acquired.meta.ref.urlcharnullableprovider_bibcodeReference, bibcode if possible.meta.refcharnullableprovider_accessDate of access to provider.timecharnullablelife_td.source A list of all the sources for the parameters in the other tables. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 1029source_idSource identifier.meta.id131.84515.0998.1610291.0intindexedprimaryrefReference, bibcode if possible.meta.refcharnullableprovider_nameName for the service through which the data was acquired. SIMBAD: service = http://simbad.u-strasbg.fr:80/simbad/sim-tap, bibcode = 2000A&AS..143....9W. ExoMercat: service = http://archives.ia2.inaf.it/vo/tap/projects, bibcode = 2020A&C....3100370A. Everything else is acquired through private communication.meta.bib.authorcharlife_td.star_basic A list of all basic stellar parameters. Note that LIFE's target database is living data. The content – and to some extent even structure – of these tables may change at any time without prior warning. 3137object_idrefObject key (unstable, use only for joining to the other tables).meta.id;meta.main1117.241845.03532.9236391.0intindexedprimarycoo_raRight Ascensiondegpos.eq.ra;meta.main0.0564378.79436182.492348.299359.9641doubleindexednullablecoo_decDeclinationdegpos.eq.dec;meta.main-88.1935-69.232-0.1725370.427185.04121doubleindexednullablecoo_err_angleCoordinate error angledegpos.posAng;pos.errorEllipse;pos.eq090.090.090.01790.9509085shortnullablecoo_err_majCoordinate error major axismasphys.angSize.smajAxis;pos.errorEllipse;pos.eq0.00610.0106460.0276100640000.950909floatnullablecoo_err_minCoordinate error minor axismasphys.angSize.sminAxis;pos.errorEllipse;pos.eq0.00690.0110.025510070000.950909floatnullablecoo_qualCoordinate quality (A:best, E:worst)meta.code.qual;pos.eqcharnullablecoo_source_idrefSource identifier corresponding to the position (coo) parameters.meta.ref124.0220.0220.02201.0intnullablecoo_gal_lGalactical longitude.degpos.galactic.lon0.019142310.7142179.362349.663359.9660.665613doublenullablecoo_gal_bGalactical latitude.degpos.galactic.lat-89.6708-69.4250.74652569.854489.30220.665613doublenullablecoo_gal_source_idrefSource identifier corresponding to the position (coo_gal) parameters.meta.ref10241024.01024.01024.010240.665613intnullablemag_i_valueMagnitude in I filter.phot.mag;em.opt.I-1.682.7299.916517.046123.850.122356doublenullablemag_i_source_idrefSource identifier corresponding to the Magnitude in I filter parameters.meta.ref180180.0180.0180.01800.122355685intnullablemag_j_valueMagnitude in J filter.phot.mag;em.IR.J-2.2524.449489.84216.079125.420.594903doublenullablemag_j_source_idrefSource identifier corresponding to the Magnitude in J filter parameters.meta.ref180180.0180.0180.01800.59490347intnullablemag_k_valueMagnitude in K filter.phot.mag;em.IR.K-3.124.0948.94814.997823.480.586442doublenullablemag_k_source_idrefSource identifier corresponding to the Magnitude in K filter parameters.meta.ref180180.0180.0180.01800.5864417intnullableplx_valueParallax value.maspos.parallax50.005450.56763.7263186.6768.0670.983424doublenullableplx_errParallax uncertainty.masstat.error;pos.parallax0.00970.01510.0374.6810.982467doublenullableplx_qualParallax quality (A:best, E:worst)meta.code.qual;pos.parallaxcharnullableplx_source_idrefSource identifier corresponding to the parallax parameters.meta.ref138.0220.0220.02340.98342365intnullabledist_st_valueObject distance.pcpos.distance1.39.867225.8932.9333.330.652094doublenullabledist_st_errObject distance error.pcstat.error;pos.distance0doublenullabledist_st_qualDistance quality (A:best, E:worst)meta.code.qual;pos.distancecharnullabledist_st_source_idrefIdentifier of the source of the distance parameter.meta.ref10241024.01024.01024.010240.6520936intnullablesptype_stringObject spectral type MK.src.spTypecharnullablesptype_errObject spectral type MK error.stat.error;src.spType0doublenullablesptype_qualSpectral type MK quality (A:best, E:worst)meta.code.qual;src.spTypecharnullablesptype_source_idrefIdentifier of the source of the spectral type MK parameter.meta.ref;src.spType161.0297.0912.010170.44847542intnullableclass_tempObject spectral type MK temperature class.src.spTypecharnullableclass_temp_nrObject spectral type MK temperature class number.src.spTypecharnullableclass_lumObject spectral type MK luminosity class.src.spTypecharnullableclass_source_idrefIdentifier of the source of the spectral type MK classification parameter.meta.ref;src.spType10241024.01024.01024.010240.36444098intnullableteff_st_valueObject effective temperature.Kphys.temperature.effective2350263034306180170000.468463doublenullableteff_st_errObject effective temperature error.Kstat.error;phys.temperature.effective0doublenullableteff_st_qualEffective temperature quality (A:best, E:worst)meta.code.qual;phys.temperature.effectivecharnullableteff_st_source_idrefIdentifier of the source of the effective temperature parameter.meta.ref;phys.temperature.effective467467.0467.0878.08780.46846277intnullableradius_st_valueObject radius.solRadphys.size.radius0.1010.1160.3888051.405775.058990.43019doublenullableradius_st_errObject radius error.solRadstat.error;phys.size.radius0doublenullableradius_st_qualRadius quality (A:best, E:worst)meta.code.qual;phys.size.radiuscharnullableradius_st_source_idrefIdentifier of the source of the radius parameter.meta.ref;phys.size.radius467467.0467.0876.08760.43019015intnullablemass_st_valueObject mass.solMassphys.mass0.0780.0850.371.249655.40.366289doublenullablemass_st_errObject mass error.solMassstat.error;phys.mass0doublenullablemass_st_qualMass quality (A:best, E:worst)meta.code.qual;phys.masscharnullablemass_st_source_idrefIdentifier of the source of the mass parameter.meta.ref;phys.mass467467.0467.0876.08760.36628896intnullablebinary_flagBinary flag.meta.code.multipcharnullablebinary_qualBinary quality (A:best, E:worst)meta.code.qualcharnullablebinary_source_idrefIdentifier of the source of the binary_flag parameter.meta.ref180180.0197.0568.05681.0intnullablesep_ang_valueAngular separation of binary.arcsecpos.angDistance00.110.3504.44999.90.155911doublenullablesep_ang_errObject ang. separation error.arcsecstat.error;pos.angDistance0doublenullablesep_ang_obs_dateYear of observation.time.epoch;obs18911999.02016.02023.020250.1559111intnullablesep_ang_qualAng. separation quality (A:best, E:worst)meta.code.qual;pos.angDistancecharnullablesep_ang_source_idrefIdentifier of the source of the sep_ang parameter.meta.ref;pos.angDistance197197.0197.0197.01970.1559111intnullablelife_td.objectobject_idrefobject_idlotsspol The LOFAR Two Meter Sky Survey LoTSS DR2 (:bibcode:`2022A&A...659A...1S`) obtained radio data from 27% of the northern sky between 120 and 168 MHz in the year 2014 through 2020. This service publishes polarization spectra of extragalactic radio sources (radio galaxies and blazars) and the rotation measures derived from them. We also give redshifts for all sources. The data has a spatial resolution of 20 arcsec.lotsspol.rmtableA table of rotation measures derived from the content of lotsspol.spectra. This is supposed to be in line with RMTable version 1, https://github.com/CIRADA-Tools/RMTable.2461cat_idSource ID in catalogmeta.id;meta.main1186.65611.020336.2206021.0shortraRight Ascension [ICRS] of the polarised emission at epoch (this will often be an one extremity of the radio source).degpos.eq.ra;meta.main0.38575810.8104179.544346.111359.9661doublenullabledecDeclination [ICRS] of the polarised emission at epoch (this will often be an one extremity of the radio source).degpos.eq.dec;meta.main17.306621.757641.01466.287169.04791doublenullabledatalinkDatalink for the spectrummeta.ref.urlcharnullablermRotation measurerad.m**-2phys.polarization.rotMeasure;meta.main-119.078-84.37125.15338.1244115.381floatnullablerm_errTotal error in RMrad.m**-2stat.error;phys.polarization.rotMeasure0.05005360.05038390.05704450.07099740.08481241doublenullablerm_err_snrError in RM from signal to noise ratio onlyrad.m**-2stat.error;phys.polarization.rotMeasure0.00231650.006207470.02746040.05040460.06850661doublenullablepolintPolarized intensityJyphot.flux.density;phys.polarization.linear0.0002490970.0006467460.001685080.01396230.08020311doublenullablepolint_errError in Polarised IntensityJystat.error;phot.flux.density;phys.polarization.linear1.4e-054.4e-057.9e-050.0001870.0008531floatnullablefracpolFractional (linear) polarizationphys.polarization.linear0.0004885260.00194870.01804970.09558860.3165631doublenullablefracpol_errError in fractional polarizationstat.error;phys.polarization.linear7.97101e-068.48044e-050.0006517490.005207210.02763171floatnullablermsf_fwhmFull-width at half maximum of the RMSFrad.m**-2instr.rmsf;stat.fwhm0.8821.1571.1571.1931.4531floatnullablereffreq_polReference frequency for polarizationHzem.freq;phys.polarization1.3405e+081.38571e+081.40646e+081.43061e+081.53789e+081floatnullablelGalactic Longitudedegpos.galactic.lon1.0454149.971130.643195.839357.1261doublenullablebGalactic Latitudedegpos.galactic.lat-45.2886-38.935548.64878.999289.33291doublenullablepos_errPosition uncertaintydegstat.error;pos0.0001112310.0002980110.001255680.002384840.003290381doublenullablebeamdistDistance from beam centre (taken as centre of tile)degpos.angDistance;instr.beam0.030.24181.041.932.760.937424floatnullablecatnameName of catalog this was taken from.meta.notecharnullablecomplex_flagFaraday complexity flagmeta.codecharnullablecomplex_testFaraday complexity metricmeta.notecharnullablerm_methodRM determination methodmeta.notecharnullableionosphereIonospheric correction methodmeta.notecharnullablepol_biasPolarization bias correction methodmeta.notecharnullableflux_typeStokes extraction methodmeta.notecharnullablebeam_majBeam major axisdegpos.angResolution;instr.beam;phys.angSize.smajAxis0.005555560.005555560.005555560.005555560.005555561floatnullablebeam_minBeam minor axisdegpos.angResolution;instr.beam;phys.angSize.sminAxis0.005555560.005555560.005555560.005555560.005555561floatnullablebeam_paBeam position angledegpos.angResolution;instr.beam;pos.posAng90909090901floatnullablereffreq_beamReference frequency for beamHzem.freq;instr.beam000001floatnullableminfreqLowest frequencyHzem.freq;stat.min1.2e+081.2e+081.2e+081.2e+081.2e+081floatnullablemaxfreqHighest frequencyHzem.freq;stat.max1.68e+081.68e+081.68e+081.68e+081.68e+081floatnullablechannelwidthTypical channel widthHzem.freq;instr.bandwidth97600976009760097600976001floatnullablenoise_chanTypical per-channel noise in Q;UJystat.error;instr.det.noise0.0008352720.001282980.001867720.003141480.00502851floatnullabletelescopeName of Telescope(s)instr.telcharnullableint_timeIntegration timestime.duration;obs.exposure28800288002880028800288001floatnullableepoch_mjdMedian epoch of observationdtime.epoch5680556833.25804158796.8588841doublenullableobs_intervalInterval of observationdtime.interval0.3333330.3333330.3333330.3333330.3333331floatnullableleakageInstrumental leakage estimatephys.polarization.linear0.010.010.010.010.011floatnullabledatarefData referencesmeta.bib.bibcodecharnullablenotesNotesmeta.notecharnullablereffreq_iReference frequency for Stokes IHzem.freq;phys.polarization.stokes.I1.44e+081.44e+081.44e+081.44e+081.44e+081floatnullablefieldLoTSS observation pointing namemeta.id;obs.fieldcharnullablexx-pixel coordinate within an individual LoTSS field, ranging from 0 to 3200, for a pixel width of 4.5 arcsecpixelpos.cartesian.x;instr.det7574.81660.02658.99999999999931901.0shortyy-pixel coordinate within an individual LoTSS field, ranging from 0 to 3200, for a pixel height of 4.5 arcsecpixelpos.cartesian.y;instr.det9498.61664.02849.19999999999931981.0shortsnr_rmtools_madSignal to noise ratio based the peak polarized intensity divided by the estimated noise in the Faraday depth spectrum (where the noise is computed using the median deviation from the median of the polarized intensity, and then correcting to be equivalent to a Gaussian sigma).stat.snr;phot.flux;phys.polarization8.4444411.548921.162893.1943249.731doublenullablera_nvssRA of the object in NVSSdegpos.eq.ra0.38459.3513179.898349.758359.9280.369768doublenullabledec_nvssDec of the object in NVSSdegpos.eq.dec17.430121.685640.460565.890969.03190.369768doublenullablenvss_rmRotation measure of the object in NVSSrad.m**-2phys.polarization.rotMeasure-131.4-87.7463.949.665900.369768floatnullablenvss_rm_errError in rotation measure of the object in NVSSrad.m**-2stat.error;phys.polarization.rotMeasure0.31.88.517.573210.369768floatnullablei_nvssIntegrated Stokes I flux density from NVSSmJyphot.flux;phys.polarization.stokes.I10.334.359148.55792.7457098.60.369768floatnullablep_nvssAverage peak polarized intensity from NVSSmJyphot.flux;phys.polarization.stokes.I2.793.277.5443.4229349.760.369768floatnullablepi_nvssPercent polarization from NVSSphys.polarization;arith.ratio0.561.79276.5917.951444.730.369768floatnullableseparation_nvssDifference between NVSS position and LoTSS DR2 positionarcsecpos.angDistance0.2982881.10618.2706443.725259.42710.369768doublenullablelgz_sizeLargest angular size of the sourcearcsecphys.angsize;stat.max23.567757.1309180.74721.6413434.320.236896doublenullablezphotPhotometric redshift derived here from archive photometry (WISE, PanSTARRS, etc; cf. 2021A&A...648A...4D).src.redshift.phot-0.08757360.1143160.6397111.882281e+200.676554doublenullablezphot_errError in zphotstat.error;src.redshift.phot0.004429630.01382750.1040140.9327461e+200.676554doublenullablephot_spec_z_bestNature of z_best: 0: phot, 1: specmeta.code;src.redshift-1-1.00.01.011.0shortlgz_ra_degRA of the host galaxy, mainly from NED.degpos.eq.ra0.3847510.7954180.731346.189359.9660.880943doublenullablelgz_dec_degDec of the host galaxy, mainly from NED.degpos.eq.dec17.314821.761141.11666.282669.04770.880943doublenullablez_bestBest redshift available from the literature, typically from NED.src.redshift0.005850.09114380.5851.662683.424590.791955doublenullablenum_in_fieldNumber of polarized sources in the originating pointing.meta.number;src23.08.017.0281.0shortmedrmMedian RM in the originating pointing.rad.m**-2phys.polarization.rotMeasure;stat.median-110.63-81.395.1336.59697.11floatnullablemadrmMedian absolute deviation of RM in the originating pointing.rad.m**-2stat.mad;phys.polarization.rotMeasure0.090.6783.0414.58441.381floatnullablemedfpolMedian degree of polarization in the originating pointing (percent).phys.polarization;stat.median0.170.461.94.97.821floatnullablemadfpolMedian absolute deviation of degree of polarization in the originating pointing (percent).stat.mad;phys.polarization0.040.151.083.527.431floatnullablera_centreRA of field centredegpos.eq.ra;obs.field0.0312510.5632179.577345.655359.6991doublenullabledec_centreDec of field centredegpos.eq.dec;obs.field18.111121.120441.182467.006567.76511doublenullablenchanNumber of channels used in RM derivationmeta.number;em.bin259429.8450.0479.07031.0intnullablesource_name_dr2Official source name assigned by the International LOFAR Telescope ILT.meta.idcharnullablera_dr2LoTSS DR2 RA of the centroid of the total radio intensity using pyBDSF.degpos.eq.ra0.38444910.8018180.007346.159359.9660.993092doublenullabledec_dr2LoTSS DR2 Dec of the centroid of the total radio intensity using pyBDSF.degpos.eq.dec17.305221.754541.025566.290669.04830.993092doublenullablee_ra_dr2Error in ra_dr2degstat.error;pos.eq.ra0.0002324580.002409110.05295172.6641839.64080.992686doublenullablee_dec_dr2Error in dec_dr2degstat.error;pos.eq.dec0.000424910.002566150.05517632.6869638.55890.992686doublenullabletotal_flux_dr2Total radio flux at 144 MHz from pyBDSF.Jyphot.flux;em.radio0.001804480.03282980.3750784.0140928.07690.993092doublenullablee_total_flux_dr2Error in total_flux_dr2Jystat.error;phot.flux;em.radio0.0001034610.0004480760.002329550.01521070.1938510.992686doublenullablemaj_dr2Semimajor axis of the radio emissionarcsecphys.angSize.smajAxis6.339427.2997726.8432126.478330.2860.759447doublenullablemin_dr2Semiminor axis of the radio emissionarcsecphys.angSize.sminAxis5.450296.543879.2802125.776977.21080.759447doublenullablepa_dr2Position angle of the radio emission, north over westdegpos.posAng0.2822196.5844985.6607174.394179.8490.759447doublenullablel144Spectral luminosity at 144 MHz in the rest frame of the sourceW.Hz**-1phys.luminosity2.25463e+223.38959e+245.18412e+261.17556e+285.46758e+280.787485doublenullablelinearsize_kpcProjected largest linear sizekpcphys.size6.6167568.4241423.9482194.024558.050.606258doublenullablerrmThe residual RM after subtraction of the average Galactic RM within an aperture of radius 1 degree (see the grm column).rad.m**-2phys.polarization.rotMeasure;src.net-44.4383-7.06386-0.1525175.8592841.21051doublenullablegrmAverage Galactic RM within an aperture of radius 1 degree from the Garching Faraday rotation sky v2.rad.m**-2phys.polarization.rotMeasure-118.973-82.04665.3865339.0822104.2891doublenullablegrmerrError in grm.rad.m**-2stat.error;phys.polarization.rotMeasure0.08923670.1223640.3110271.43982.594161doublenullablebzcat_nameBlazar source name in the ROMA-BZCAT catalogue (2015Ap&SS.357...75M)meta.id.crosscharnullablelotsspol.spectraSpectrally resolved polarisation; for pre-derived rotation measures, see lotsspol.rmtable. The spectral behaviour of the LoTSS Stokes I data are presently unreliable and not included here. However, one can use the stokes_i column in lotsspol.rmtable in combination with an assumed radio spectral index to produce fractional polarization spectra.2461ssa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value5680556833.25804158796.8588841doublenullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start1.511891.794741.794741.81921.957221floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop2.492822.492822.492822.492822.492821floatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Length259429.8450.0479.07031.0intnullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent28800288002880028800288001floatnullablessa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.ClasscharnullableaccrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size100000100000.0100000.0100000.01000001.0longnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablecat_idRunning number of the sourcemeta.id;meta.main1186.65611.020336.2206021.0longfreqThe spectral coordinateHzem.freqdoublenullablestokesiPer-frequency Stokes polarization coefficients ImJy/beamphys.polarization.stokes.Idoublenullablestokesi_errorError in stokesimJy/beamstat.error;phys.polarization.stokes.IdoublenullablestokesqPer-frequency Stokes polarization coefficients QmJy/beamphys.polarization.stokes.Qdoublenullablestokesq_errorError in stokesqmJy/beamstat.error;phys.polarization.stokes.QdoublenullablestokesuPer-frequency Stokes polarization coefficients UmJy/beamphys.polarization.stokes.Udoublenullablestokesu_errorError in stokesumJy/beamstat.error;phys.polarization.stokes.Udoublenullablegalactic_locationssa_location expressed in galactic coordinates (do not use for querying: there's no index on this).pos;pos.galacticdoublenullablelotsspol.ssameta The LOFAR Two Meter Sky Survey LoTSS DR2 (:bibcode:`2022A&A...659A...1S`) obtained radio data from 27% of the northern sky between 120 and 168 MHz in the year 2014 through 2020. This service publishes polarization spectra of extragalactic radio sources (radio galaxies and blazars) and the rotation measures derived from them. We also give redshifts for all sources. The data has a spatial resolution of 20 arcsec.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassRadiocharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value5680556833.25804158796.8588841doublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent28800288002880028800288001floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start1.511891.794741.794741.81921.957221floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop2.492822.492822.492822.492822.492821floatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Length259429.8450.0479.07031.0intnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.freqcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitHzcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphys.polarization.stokescharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.UnitJycharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionLoTSS DR2charnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentFEROScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcepointedcharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationRELATIVEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablemagic The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. This service re-publishes the data with homogeneized in flux units (given here in 'erg/(s.cm2)'). Photon energy values in are transfomred to frequencies.magic.main The MAGIC project observes the VHE sky (GeV~TeV) through Cherenkov radiation events. The project is operating since 2004 and with the support from the Spain-VO team they provide data access through a VO-SSAP and web services. This service re-publishes the data with homogeneized in flux units (given here in 'erg/(s.cm2)'). Photon energy values in are transfomred to frequencies.95accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_referencecharnullablereference_doicharnullableebl_correctedshortra_j2000Right Ascensiondegpos.eq.radoubledec_j2000Declinationdegpos.eq.decdoublemwsc MWSC presents a list of 3006 Milky Way Stellar Clusters (MWSC), found in the 2MAst (2MASS with Astrometry) catalogue. The target list was compiled on the basis of present-day lists of open, globular and candidate clusters. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, mean cluster proper motions, distances, reddenings, ages, tidal parameters, and sometimes radial velocities.mwsc.mainA list of milky way stellar cluster candidates and objects, together with the notes and parameters from confirmed objects for the original publication.3784recnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharindexedprimarynameNGC, IC or other common designationmeta.idcharnullableconfirmation_flagIs this object a stellar cluster? 'dupe' indicates the object coincides with another cluster.charobject_typeObject typesrc.classcharnullableot_certainTrue if the object type is confirmed, false if object type has candidate status.meta.code;src.classbooleannullablesourceSource for MWSC list and input parametersmeta.refcharnullablesource_typeObject type from sourcesrc.classcharnullablen_starNumber of stars in MWSC sky area.meta.number00.011195.054257.1799999999716431931.0intraj2000Adopted cluster centre in RA J2000.0degpos.eq.ra;meta.main0.067519.4204167.11343.301359.7720.794397doublenullabledej2000Adopted cluster centre in Dec J2000.0degpos.eq.dec;meta.main-83.445-64.7943-12.325563.774585.2550.794397doublenullableglonGalactic longitudedegpos.galactic.lon0.0088.31210.733351.439359.7640.794397doublenullableglatGalactic latitudedegpos.galactic.lat-89.386-18.2523-0.34616.457384.4930.794397doublenullablercoreAngular radius of the coredegphys.angSize;src0.0090.010.0180.050.50.794397floatnullablercenterAngular radius of the central partdegphys.angSize;src0.020.0350.070.249252.510.794397floatnullablerclusterAngular radius of the clusterdegphys.angSize;src0.040.0650.130.484256.20.794397floatindexednullablepmraAverage proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra;stat.mean-1.12361e-05-2.92736e-06-5.90278e-071.10833e-069.94444e-060.794397floatnullablepmdeAverage proper motion in Declinationdeg/yrpos.pm;pos.eq.dec;stat.mean-1.27778e-05-2.21625e-06-4.05556e-072.03111e-067.61111e-060.794397floatnullablee_pmError of proper motiondeg/yrstat.error;pos.pm;pos.eq.ra;stat.mean8.33333e-095.55556e-081.52778e-074.02778e-078.88889e-070.794397floatnullablervAverage radial velocitykm/sspect.dopplerVeloc;pos.heliocentric;stat.mean-411.4-123.815-4.57113.6474940.25185floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric;stat.mean0.010.12.414.7138570.203488floatnullablen_rvNumber of stars used for RVkm/smeta.number;spect.dopplerVeloc;pos.heliocentric;stat.mean11.02.023.2799999999999731060.1915962intnullablen1s_coreNumber of most probable (1sigma) members within R(core)meta.number01.03.018.01470.7943975intnullablen1s_centerNumber of most probable (1sigma) members within R(center); these are the stars used to compute the average proper motion.meta.number28.030.0185.84999999999999500.7943975intnullablen1s_clusterNumber of most probable (1sigma) members within R(cluster)meta.number717.081.0513.042620.7943975intnullabledistDistance from the Sunpcpos.distance;pos.heliocentric87502.052069.58921.35825350.794397floatindexednullablecol_ex_optColour excess in (B-V)magphot.color.excess;phot.color;em.opt.B;em.opt.V00.0310.572.0823.7270.794397floatnullabledist_modApparent distance modulus in Ksmagphot.mag.distMod4.6988.568411.815.034219.610.794397floatnullablecol_ex_jColour excess in (J-Ks)magphot.color.excess;phot.color;em.ir.J;em.ir.K00.0150.27411.790.794397floatnullablecol_ex_hColour excess in (J-H)magphot.color.excess;phot.color;em.ir.J;em.ir.H00.010.1830.6671.1940.794397floatnullabledelta_hCorrection to H mag of fitted isochrone, empirically introduced to achieve a better fit in the Ks vs. J-H CMD. (see 2012A&A...543A.156K).magphot.mag;arith.diff-0.12-0.0425500.050.120.794397floatnullablelogtLogarithm of average agelog(yr)time.age;stat.mean66.28.6410.110.10.794397floatindexednullablee_logtError in logarithm of average agelog(yr)stat.error;time.age0.0010.0030.040.173920.3430.16834floatnullablentNumber of stars used for log(T) calculationmeta.number01.03.031.6499999999999771490.22357294intnullablercKing core radiuspcphys.size.radius0.080.31.246.62239.10.782505floatnullablee_rcError of King core radiuspcstat.error;phys.size.radius0.030.090.322.31424.090.782505floatnullablertKing tidal radiuspcphys.size.radius0.843.0568.5836.212178.830.782505floatnullablee_rtError of King tidal radiuspcstat.error;phys.size.radius0.140.542.2810.692137.370.782505floatnullablekingkKing normalization factor (a measure of the central density of the cluster, see 2007A&A...468..151Ppc**-2stat.fit.param0.010.245.0950.8552384.030.781977floatnullablee_kingkError of King normalization factorpc**-2stat.error;stat.fit.param0.010.081.1312.4908197.690.781448floatnullablefe_hMetallicity [Fe/H]; this is copied from 2013arXiv1309.4325C or 2012A&A...539A.125D. Data for globular clusters is taken from the revised Harris (1996) catalogue, edition 2010, or newly determined.phys.abund.Fe-2.155-1.887-0.3340.2014290.1280.102273floatindexednullablee_fe_hError of Metallicitystat.error;phys.abund.Fe0.010.010.0950.20.30.0486258floatnullablen_fe_hNumber of objects in [Fe/H] calculation.meta.number11.010.0134.38000000000015800.08192389shortnullablenote_textThe text of the note for an object.meta.notecharnullablemwsc.starsData on cluster stars.64000000recnoMWSC number of the cluster containing the star.meta.id;meta.maincharindexedraj2000Stellar Right Ascension J2000.0, epoch 2000.0degpos.eq.ra;meta.main-2.1703632.2117226.028335.425360.6561doubleindexednullabledej2000Stellar Declination J2000.0, epoch 2000.0degpos.eq.dec;meta.main-83.9275-64.5364-25.542762.115886.10781doubleindexednullablemagbB magnitude in Johnson system.magphot.mag;em.opt.B-31.0821417.920.1300.647789floatnullablemagvV magnitude in Johnson system.magphot.mag;em.opt.V-32.63612.716.618.332.70.647825floatindexednullablemagjMagnitude in the 2MASS J bandmagphot.mag;em.ir.J-0.72611.33114.93516.61420.121floatindexednullablee_magjError in the magnitude in the 2MASS J bandmagstat.error;phot.mag;em.ir.J0.030.030.0520.158.8871floatnullablemaghMagnitude in the 2MASS H bandmagphot.mag;em.ir.H-1.51410.34914.18415.91918.7191floatnullablee_maghError in the magnitude in the 2MASS H bandmagstat.error;phot.mag;em.ir.H0.030.030.0570.1778.9041floatnullablemagksMagnitude in the 2MASS Ks bandmagphot.mag;em.ir.K-1.8249.87313.94415.60219.8651floatnullablee_magksError in the magnitude in the 2MASS Ks bandmagstat.error;phot.mag;em.ir.K0.030.030.0680.2228.8871floatnullablepmraStellar proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra-0.000302042-1.24222e-05-5.19444e-071.34056e-050.0004374530.783847floatnullablepmdeStellar proper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.000308794-1.48278e-05-5.77778e-071.16083e-050.0002758190.783847floatnullablee_pmError of stellar proper motiondeg/yrstat.error;pos.pm;pos.eq.ra4.16667e-071.02778e-061.58056e-064.56111e-063.73944e-050.783847floatnullablervStellar radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-158.6-56-2.959.745289.30.00012444floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric0.090.23.510900.000108126floatnullableqflg2MASS JHK photometric quality flagmeta.code.qual;photcharnullablerflg2MASS photometric read flagmeta.refcharnullablebflg2MASS photometric blend flagmeta.codecharnullabletwomassidUnique identifier in 2MASS (pts_key)meta.id.cross98046197431.05711607583.01287762235.1913399380741.0intasccIdentifier in ASCC 2.5meta.id.cross22109137.961506411.02351212.1226032250.0042021875intnullablespectralSpectral type and luminosity classsrc.spTypecharnullabler_clAngular distance from cluster centredegpos.angDistance0.00010.07840.33582.84976.70721floatnullablep_spatProbability of membership from spatial propertiesstat.probability000111floatindexednullablep_kinProbability of membership from kinetic propertiesstat.probability000.06050.968511floatindexednullablep_jksProbability of membership from J, Ks photometrystat.probability000.0856111floatindexednullablep_jhProbability of membership from J, H photometrystat.probability000.1634111floatnullablemwsc.mainrecnorecnomwsce14a MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/formmwsce14a.main MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/form782recnoMWSC sequential number (cluster catalog number).meta.id;meta.maincharindexedprimarynameNGC, IC or other common designationmeta.idcharnullableconfirmation_flagIs this object a stellar cluster? 'dupe' indicates the object coincides with another cluster.charobject_typeObject typesrc.classcharnullableot_certainTrue if the object type is confirmed, false if object type has candidate status.meta.code;src.classbooleannullablesourceSource for MWSC list and input parametersmeta.refcharnullablesource_typeObject type from sourcesrc.classcharnullablen_starNumber of stars in MWSC sky area.meta.number00.011195.054257.1799999999716431931.0intraj2000Adopted cluster centre in RA J2000.0degpos.eq.ra;meta.main0.067519.4204167.11343.301359.7720.794397doublenullabledej2000Adopted cluster centre in Dec J2000.0degpos.eq.dec;meta.main-83.445-64.7943-12.325563.774585.2550.794397doublenullableglonGalactic longitudedegpos.galactic.lon0.0088.31210.733351.439359.7640.794397doublenullableglatGalactic latitudedegpos.galactic.lat-89.386-18.2523-0.34616.457384.4930.794397doublenullablercoreAngular radius of the coredegphys.angSize;src0.0090.010.0180.050.50.794397floatnullablercenterAngular radius of the central partdegphys.angSize;src0.020.0350.070.249252.510.794397floatnullablerclusterAngular radius of the clusterdegphys.angSize;src0.040.0650.130.484256.20.794397floatindexednullablepmraAverage proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra;stat.mean-1.12361e-05-2.92736e-06-5.90278e-071.10833e-069.94444e-060.794397floatnullablepmdeAverage proper motion in Declinationdeg/yrpos.pm;pos.eq.dec;stat.mean-1.27778e-05-2.21625e-06-4.05556e-072.03111e-067.61111e-060.794397floatnullablee_pmError of proper motiondeg/yrstat.error;pos.pm;pos.eq.ra;stat.mean8.33333e-095.55556e-081.52778e-074.02778e-078.88889e-070.794397floatnullablervAverage radial velocitykm/sspect.dopplerVeloc;pos.heliocentric;stat.mean-411.4-123.815-4.57113.6474940.25185floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric;stat.mean0.010.12.414.7138570.203488floatnullablen_rvNumber of stars used for RVkm/smeta.number;spect.dopplerVeloc;pos.heliocentric;stat.mean11.02.023.2799999999999731060.1915962intnullablen1s_coreNumber of most probable (1sigma) members within R(core)meta.number01.03.018.01470.7943975intnullablen1s_centerNumber of most probable (1sigma) members within R(center); these are the stars used to compute the average proper motion.meta.number28.030.0185.84999999999999500.7943975intnullablen1s_clusterNumber of most probable (1sigma) members within R(cluster)meta.number717.081.0513.042620.7943975intnullabledistDistance from the Sunpcpos.distance;pos.heliocentric87502.052069.58921.35825350.794397floatindexednullablecol_ex_optColour excess in (B-V)magphot.color.excess;phot.color;em.opt.B;em.opt.V00.0310.572.0823.7270.794397floatnullabledist_modApparent distance modulus in Ksmagphot.mag.distMod4.6988.568411.815.034219.610.794397floatnullablecol_ex_jColour excess in (J-Ks)magphot.color.excess;phot.color;em.ir.J;em.ir.K00.0150.27411.790.794397floatnullablecol_ex_hColour excess in (J-H)magphot.color.excess;phot.color;em.ir.J;em.ir.H00.010.1830.6671.1940.794397floatnullabledelta_hCorrection to H mag of fitted isochrone, empirically introduced to achieve a better fit in the Ks vs. J-H CMD. (see 2012A&A...543A.156K).magphot.mag;arith.diff-0.12-0.0425500.050.120.794397floatnullablelogtLogarithm of average agelog(yr)time.age;stat.mean66.28.6410.110.10.794397floatindexednullablee_logtError in logarithm of average agelog(yr)stat.error;time.age0.0010.0030.040.173920.3430.16834floatnullablentNumber of stars used for log(T) calculationmeta.number01.03.031.6499999999999771490.22357294intnullablercKing core radiuspcphys.size.radius0.080.31.246.62239.10.782505floatnullablee_rcError of King core radiuspcstat.error;phys.size.radius0.030.090.322.31424.090.782505floatnullablertKing tidal radiuspcphys.size.radius0.843.0568.5836.212178.830.782505floatnullablee_rtError of King tidal radiuspcstat.error;phys.size.radius0.140.542.2810.692137.370.782505floatnullablekingkKing normalization factor (a measure of the central density of the cluster, see 2007A&A...468..151Ppc**-2stat.fit.param0.010.245.0950.8552384.030.781977floatnullablee_kingkError of King normalization factorpc**-2stat.error;stat.fit.param0.010.081.1312.4908197.690.781448floatnullablefe_hMetallicity [Fe/H]; this is copied from 2013arXiv1309.4325C or 2012A&A...539A.125D. Data for globular clusters is taken from the revised Harris (1996) catalogue, edition 2010, or newly determined.phys.abund.Fe-2.155-1.887-0.3340.2014290.1280.102273floatindexednullablee_fe_hError of Metallicitystat.error;phys.abund.Fe0.010.010.0950.20.30.0486258floatnullablen_fe_hNumber of objects in [Fe/H] calculation.meta.number11.010.0134.38000000000015800.08192389shortnullablenote_textThe text of the note for an object.meta.notecharnullablemwsce14a.stars MWSC-e14a ("MWSC extension 2014a") is a catalogue of 139 new open clusters at high Galactic latitudes (\|b\|>20 deg) including lists of candidate members. It extends the Kharchenko et al. 'Catalog of Milky Way Star Clusters'. The target list was compiled as density enhancements found in the 2MASS point source catalogue. For confirmed clusters we determined a homogeneous set of astrophysical parameters such as membership, angular radii of the main morphological parts, proper motion, distance, reddening, age, and tidal parameters. .. _Catalog of Milky Way Star Clusters: http://dc.g-vo.org/mwsc/q/clu/form519163recnoMWSC number of the cluster containing the star.meta.id;meta.maincharindexedraj2000Stellar Right Ascension J2000.0, epoch 2000.0degpos.eq.ra;meta.main-2.1703632.2117226.028335.425360.6561doubleindexednullabledej2000Stellar Declination J2000.0, epoch 2000.0degpos.eq.dec;meta.main-83.9275-64.5364-25.542762.115886.10781doubleindexednullablemagbB magnitude in Johnson system.magphot.mag;em.opt.B-31.0821417.920.1300.647789floatnullablemagvV magnitude in Johnson system.magphot.mag;em.opt.V-32.63612.716.618.332.70.647825floatindexednullablemagjMagnitude in the 2MASS J bandmagphot.mag;em.ir.J-0.72611.33114.93516.61420.121floatindexednullablee_magjError in the magnitude in the 2MASS J bandmagstat.error;phot.mag;em.ir.J0.030.030.0520.158.8871floatnullablemaghMagnitude in the 2MASS H bandmagphot.mag;em.ir.H-1.51410.34914.18415.91918.7191floatnullablee_maghError in the magnitude in the 2MASS H bandmagstat.error;phot.mag;em.ir.H0.030.030.0570.1778.9041floatnullablemagksMagnitude in the 2MASS Ks bandmagphot.mag;em.ir.K-1.8249.87313.94415.60219.8651floatnullablee_magksError in the magnitude in the 2MASS Ks bandmagstat.error;phot.mag;em.ir.K0.030.030.0680.2228.8871floatnullablepmraStellar proper motion in RA*cos(DE)deg/yrpos.pm;pos.eq.ra-0.000302042-1.24222e-05-5.19444e-071.34056e-050.0004374530.783847floatnullablepmdeStellar proper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.000308794-1.48278e-05-5.77778e-071.16083e-050.0002758190.783847floatnullablee_pmError of stellar proper motiondeg/yrstat.error;pos.pm;pos.eq.ra4.16667e-071.02778e-061.58056e-064.56111e-063.73944e-050.783847floatnullablervStellar radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-158.6-56-2.959.745289.30.00012444floatnullablee_rvError of RVkm/sstat.error;spect.dopplerVeloc;pos.heliocentric0.090.23.510900.000108126floatnullableqflg2MASS JHK photometric quality flagmeta.code.qual;photcharnullablerflg2MASS photometric read flagmeta.refcharnullablebflg2MASS photometric blend flagmeta.codecharnullabletwomassidUnique identifier in 2MASS (pts_key)meta.id.cross98046197431.05711607583.01287762235.1913399380741.0intasccIdentifier in ASCC 2.5meta.id.cross22109137.961506411.02351212.1226032250.0042021875intnullablespectralSpectral type and luminosity classsrc.spTypecharnullabler_clAngular distance from cluster centredegpos.angDistance0.00010.07840.33582.84976.70721floatnullablep_spatProbability of membership from spatial propertiesstat.probability000111floatindexednullablep_kinProbability of membership from kinetic propertiesstat.probability000.06050.968511floatindexednullablep_jksProbability of membership from J, Ks photometrystat.probability000.0856111floatindexednullablep_jhProbability of membership from J, H photometrystat.probability000.1634111floatnullablemwsce14a.mainrecnorecnoohmaserA all-sky compilation of galactic stellar sources observed for OH maser emission in the transitions at 1612, 1665, and 1667 MHz. The database contains OH maser observations selected from the literature . These observations belong to more than 6000 different objects. The database consists of three tables: The main table ("masers"), interferometric followup observations ("maps") and monitoring programs ("monitor").ohmaser.bibrefsBibliographic and other metadata on the sources of the data in the masers table.314ref_keyInternal key for the papercharindexedprimarybibcodeBibliographic reference to the data sourcemeta.bibcharnullablemodificationsModifications applied to data given in papercharnullablecommentsCompilators' CommentscharnullabletextrefHuman-readable reference to workcharnullabledet1612Sources detected at 1612 MHz00.02.0333.39999999999948120.19426751intnullablendet1612Sources not detected at 1612 MHz00.01.0224.1999999999999618800.19426751intnullabledet1665Sources detected at 1665 MHz00.02.047.92999999999991320.15286624intnullablendet1665Sources not detected at 1665 MHz00.07.0200.849999999999972440.14649682intnullabledet1667Sources detected at 1667 MHz00.04.0100.789999999999942100.1656051intnullablendet1667Sources not detected at 1667 MHz00.09.0171.772140.15923567intnullablecoosrcSource of coordinates given in databasecharnullableinputtablesTables evaluated from cited papercharnullableohmaser.mapsTable of interferometric measurements included.271measure_noUnique measurement identifiermeta.id;meta.main1410.626837.025691.379999999997341791.0intsource_noUnique, artificial source identifiermeta.code1222.626038.025500.0341741.0intsource_nameName of the observed source. The name given in the reference is usually kept.meta.idcharraj2000Selected best RA, J2000degpos.eq.ra;meta.main0.027341739.2583268.065334.999359.7671doublenullabledej2000Selected best Dec, J2000degpos.eq.dec;meta.main-87.3389-62.369-2.5805360.941186.63691doublenullablefrequencyObserved frequencyMHzem.freq16121612.01612.01667.016671.0intnullableref_keyInternal key for the originating paper, see ohmasers.bibrefs.meta.bibcharnullableinstrumentName of the interferometer usedmeta.id;instrcharnullableresolutionSpatial resolution of the observationmasinstr.param214300505680000.937269floatnullablenon_det_flag< if observation is a non-detection.meta.codecharnullablermsRMS sensitivity of the observationJyinstr.sensitivity0.0020.0050.030.530.535055floatnullablen_mapsNumber of maps obtained between obs_date_start and obs_date_endmeta.number;obs11.01.06.091.0shortnullableobs_date_startDate of the first observation, Julian years.yrtime.start;obs1968.781973.261981.162004.082011.650.99631doublenullableobs_date_endDate of last observation, Julian yearsyrtime.end;obs1969.031973.261981.162005.252011.650.99631doublenullablet_resApproximate time resolution of obs_date_*yrtime.resolution0.0050.0050.0050.110.99631floatnullableohmaser.maserssource_nosource_noohmaser.masersMaser data proper.13655measure_noUnique measurement identifiermeta.id;meta.main1410.626837.025691.379999999997341791.0intsource_noUnique, artificial source identifiermeta.code1222.626038.025500.0341741.0intflagNon-null if this measurement is considered the best available at a particular frequency. Lower means higher confidence.meta.code11.01.03.030.7250824shortnullablesource_nameName of the observed source. The name given in the reference is usually kept.meta.idcharfrequencyObserved frequencyMHzem.freq16121612.01612.01667.016671.0161216651667intnullablespec_typeS -- Single peak of maser emission; D -- Double peak of maser emission; I -- Irregular spectral profile, multiple emission peaks.meta.code;src.spTypecharnullablera_rawJ2000 RApos.eq.racharnullablede_rawJ2000 Decpos.eq.deccharnullableveloc_blueVelocity of the blue-shifted maser peak. For single-peak masers it contains the line velocity.km/sphys.veloc.expansion;pos.bodyrc-374-148.480.3127.645365.20.362944floatnullableveloc_redVelocity of the red-shifted maser peak in km/s. It contains the line velocity for a single peak maser if it corresponds to the red-shifted peak in other observations.km/sphys.veloc.expansion;pos.bodyrc-336.2-123.90822.1151.963319.60.298792floatnullableveloc_centralRadial velocity of the central star. If veloc_central is not given in the reference, it is calculated.km/sphys.veloc.expansion;pos.bodyrc-355.1-1389.4137.508365.20.370926floatnullableveloc_shellOutflow Velocity of the shell. If vexp is not given in the reference it is calculated.km/sphys.veloc.expansion;pos.bodyrc-48.81.413.82487.50.300037floatnullableveloc_errUncertainty of velocity values. Taken from the velocity resolution of the observation. It is actually a lower limit of the uncertainty, because the lines are usually much broader than velocity resolution of the observing equipment.km/sstat.error;phys.veloc.expansion;pos.bodyrc00.10.91.52.270.945441floatnullableflux_dens_flagNULL -- flux density columns contain detections; < -- non-detection at level flux density blue (3 sigma); > -- flux density blue contains a lower limit for the flux; = -- source only gives fluxes; . -- flux density blue contains probable detection; : -- flux density red contains probable detection; & -- both flux densities contain probable detectionsmeta.codecharnullableflux_dens_blueFlux Density of the blue-shifted maser peak. For single-peak masers it contains its flux density.Jyphot.flux.density;em.radio.1500-3000MHz-3.220.020.27.6042419210.977664floatnullableflux_dens_redFlux Density of the red-shifted maser peak. It contains the flux density for a single peak maser, if it corresponds to the red-shifted peak in other observations.Jyphot.flux.density;em.radio.1500-3000MHz-1.330.0380.6927.2852597.280.295643floatnullableint_flux_redIntegrated flux of red peak1e-22W.m**-2phot.flux.density;em.radio.1500-3000MHz0.0020.0220.63926.0034238.10.0407177floatnullableint_flux_blueIntegrated flux of blue peak1e-22W.m**-2phot.flux.density;em.radio.1500-3000MHz-0.3120.025650.54825.19221152.40.048041floatnullableref_keyInternal key for the originating paper, see ohmasers.bibrefs.meta.bibcharnullablerapubRA of object, from sourcedegpos.eq.ra0.027341739.2598268.065334.999359.7671floatnullabledepubDec of object, from sourcedegpos.eq.dec-87.3389-62.369-2.5794460.941686.63691floatnullableraj2000Selected best RA, J2000degpos.eq.ra;meta.main0.027341739.2583268.065334.999359.7671doubleindexednullabledej2000Selected best Dec, J2000degpos.eq.dec;meta.main-87.3389-62.369-2.5805360.941186.63691doubleindexednullablemapurlURL to information on an interferometric followup observation for this object.meta.ref.urlcharnullablemonitorurlURL to information on a monitor programme for this object.meta.ref.urlcharnullableohmaser.bibrefsref_keyref_keyohmaser.monitorTable of measurements included from monitoring programs.180measure_noUnique measurement identifiermeta.id;meta.main1410.626837.025691.379999999997341791.0intsource_nameName of the observed source. The name given in the reference is usually kept.meta.idcharsource_noUnique, artificial source identifiermeta.code1222.626038.025500.0341741.0intraj2000Selected best RA, J2000degpos.eq.ra;meta.main0.027341739.2583268.065334.999359.7671doublenullabledej2000Selected best Dec, J2000degpos.eq.dec;meta.main-87.3389-62.369-2.5805360.941186.63691doublenullablefrequencyObserved frequencyMHzem.freq16121612.01612.01667.016671.0intnullableref_keyInternal key for the originating paper, see ohmasers.bibrefs.meta.bibcharnullableobs_date_startDate of the first observation, Julian years.yrtime.start;obs1968.781973.261981.162004.082011.650.99631doublenullableobs_date_endDate of last observation, Julian yearsyrtime.end;obs1972.331972.58198820082013.351doublenullablet_resApproximate time resolution of obs_date_*yrtime.resolution0.0050.0050.0050.110.99631floatnullablemax_flux_dens_flag< if max_flux_dens_peak is a 3σ upper limit.meta.codecharnullablemax_flux_dens_peakMaximal flux density observed (or 3σ upper limit)Jyphot.flux.density;em.radio;stat.max0.060.122414.15298.5096070.566667floatnullablemin_flux_dens_flag< if min_flux_dens_peak is a 3σ upper limit.meta.codecharnullablemin_flux_dens_peakMinimal flux density observed (or 3σ upper limit)Jyphot.flux.density;em.radio;stat.min0.30.4047.7212.724425.20.472222floatnullableohmaser.maserssource_nosource_nopcc This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.pcc.main This is a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope. Additionally, we used archival Subaru multiband imaging data in order to measure aperture colors and to perform a morphological classification. The catalog reaches its 50 per cent completeness limit at an absolute V-band luminosity of -12 mag and a V-band surface brightness of 26 mag arcsec^-2 . In addition to the published table, this service also contains cutout images of the objects investigated.object_nameIdentifier from Wittman et al (2019).meta.id;meta.maincharindexedprimaryraICRS Right Ascension from WHT imagedegpos.eq.ra;meta.main49.235549.275249.662249.985150.00891doubleindexednullabledecICRS Declination from WHT imagedegpos.eq.dec;meta.main41.195741.245141.491641.741341.76931doubleindexednullablemagIntegrated V-band apparent magnitude corrected for extinction.magphot.mag;em.opt.V14.0818.711622.5424.0124.31doublenullableerr_magError in integrated apparent magnitude for sources fitted with GALFIT (i.e., pflag = 1 .. 8; NULL otherwise)magstat.error;phot.mag;em.opt.V000.030.130.630.909509floatnullabler_50Half-light radius in the V band..arcsecphys.angsize0.120.120.713.329215.231floatnullableerr_r_50Error in half-light radius in the V band.arcsecstat.error;phys.angsize00.010.040.251.150.845319floatnullablemu50Effective V band surface brightness within R_50 corrected for extinctionmag.arcsec**-2phot.mag.sb15.8520.1522.9625.3926.751floatnullableerr_mu50Error in the effective surface brightness propagated from err_mag and err_r_50mag.arcsec**-2stat.error;phot.mag.sb00.010.130.6710.845319floatnullablesersic_indexSérsic index, upper limit constrained to 4 (cf. paper, sect. 4.3)stat.fit.param0.050.090.823.508441floatnullableerr_sersic_indexError in Sérsic index for sources fitted with GALFIT with free N parameter (pflag = 1)stat.error;stat.fit.param00.010.191.6823.710.581387floatnullableb_aAxis ratio in the V band for sources fitted with GALFIT (pflag = 1 .. 8)phys.angsize;arith.ratio0.10.140.66110.909509floatnullableerr_b_aError in axis ratio for sources fitted with GALFIT with free B/A parameter (pflag = 1 - 4)stat.error;phys.angsize;arith.ratio000.050.280.930.827294floatnullablepaPosition Angle for sources fitted with GALFIT and b_a < 0.9 [North/Up=0, East/Left=90]; from V band.degpos.posang-89.9-82.9-0.983.928900.740298floatnullableerr_paError in position angle.degstat.error;pos.posang00.25.132.92889.30.740298floatnullablea_vV-band galactic foreground extinction.magphys.absorption;em.opt.V0.390.410.450.490.561floatnullablepflagPhotometry processing flag (see note).meta.code11.01.09.091.0shortresflag1 if there were significant residuals after substracting GALFIT model, 0 otherwise. This is only given for sources fitted with GALFIT (i.e., pflag = 1 .. 8)meta.code.qual00.00.01.010.90950894shortnullablebgflagBackground fitted with: ...0: Galfit; ...1: SExtractor with BACK_SIZE = 256 pixel background map, ...2: like 1, but BACK_SIZE = 32 pixelmeta.code00.00.02.021.0shortg_r_1Subaru g-r for aperture 1, color corrected for extinction. (r_aper1 = 1 R50 for sources with R50 > 4 pixels, r_aper1 = 4 pixels for sources with R50 <= 4 pixels)magphot.color;em.opt.V;em.opt.R-0.610.10.781.672.260.992091floatnullableerr_g_r_1Error in g-r for aperture 1magphot.color;em.opt.V;em.opt.R00.010.080.3410.992091floatnullabler_z_1Subaru r-z for aperture 1, color corrected for extinction. (r_aper1 = 1 R50 for sources with R50 > 4 pixels, r_aper1 = 4 pixels for sources with R50 <= 4 pixels)magphot.color;em.opt.R;em.opt.I-0.620.220.71.833.390.988413floatnullableerr_r_z_1Error in r-z for aperture 1magphot.color;em.opt.R;em.opt.I00.010.090.50.990.988413floatnullableg_r_2Subaru g-r for aperture 2, color corrected for extinction. (only for sources with R50 > 4 pixels, where r_aper2 = 2 R50)magphot.color;em.opt.V;em.opt.R-0.730.230.661.49411.940.304212floatnullableerr_g_r_2Error in g-r for aperture 2magphot.color;em.opt.V;em.opt.R00.020.120.730.980.304212floatnullabler_z_2Subaru r-z for aperture 2, color corrected for extinction. (only for sources with R50 > 4 pixels, where r_aper2 = 2 R50)magphot.color;em.opt.R;em.opt.I-0.20.240.541.311.860.290418floatnullableerr_r_z_2Error in r-z for aperture 2magphot.color;em.opt.R;em.opt.I0.010.020.150.8510.290418floatnullableg_r_flag1 if g-r photometry possibly comtaminated through bleeding trails of bright stars within 3 arcsec, 0 otherwisemeta.code.qual00.00.01.010.99209124shortnullabler_z_flag1 if r-z photometry possibly comtaminated through bleeding trails of bright stars within 3 arcsec, 0 otherwisemeta.code.qual00.00.01.010.98841274shortnullablea_gg-band galactic foreground extinction.magphys.absorption;em.opt.V0.480.510.550.60.690.992091floatnullablea_rr-band galactic foreground extinction.magphys.absorption;em.opt.R0.330.350.380.420.480.992459floatnullablea_zz-band galactic foreground extinction.magphys.absorption;em.opt.I0.180.20.210.230.260.988413floatnullablemorphologyMorphological classificationsrc.classcharnullablenucleationRemark on nucleationsrc.classcharnullablecutout_linkLink to a FITS cutout for this source from an r-band mosaic. See datalink for additional retrieval options.meta.ref.urlcharnullableplcA catalogue of candidate stars for observing astrometric microlensing using Gaia.plc.dataThe final candidate table with estimates of minimal distances, epochs, etc.8932sourceSource of the data of the lensmeta.codecharnullablesrcidId of lensing objectmeta.id;meta.maincharnullablelensalphaJ2000 PPMX alpha of lensdegpos.eq.ra;meta.main0.24841348.6085244.351318.941359.8851doubleindexednullablelensdeltaJ2000 PPMX delta of lensdegpos.eq.dec;meta.main-88.0467-71.3738-39.957155.319686.76541doubleindexednullablelensalphaerrError of lens alphadegstat.error;pos.eq.ra;meta.main2.77778e-074.16667e-062.11111e-054.41667e-050.00013751floatnullablelensdeltaerrError of lens deltadegstat.error;pos.eq.dec;meta.main2.77778e-074.16667e-062.11111e-054.36111e-050.00013751floatnullablelenspmalphaLens PM in alpha, cos(delta) applieddeg/yr-0.000508269-0.0001031337.08194e-060.0001120840.0005558331floatnullablelenspmdeltaLens PM in deltadeg/yr-0.000545278-0.000114666-1.43334e-059.67491e-050.0005390441floatnullablelenspmalphaerrError of Lens PM in alphadeg/yr01.08297e-063.83333e-061.35949e-057.38753e-051floatnullablelenspmdeltaerrError of Lens PM in deltadeg/yr08.33333e-072.52778e-068.86111e-062.21111e-051floatnullablelensmagPPMX catalogue magnitude of lensmag011.167915.05618.251499.91floatnullablelensrmagPPMX Ru mag of lensmag0.0998.514.33718.919.80.319861floatnullablelensbmagLens B mag as in PPMXmag4.28.34417.0521.121.80.0891178floatnullablelensvmagLens V mag as in PPMXmag06.33710.49713.917614.760.0258621floatnullablelensjmagLens J mag as in PPMXmag3.087.3165312.092515.50116.960.297582floatnullablelenshmagLens H mag as in PPMXmag2.846.7415211.63215.416327.770.297582floatnullablelenskmagLens K mag as in PPMXmag2.796.5823911.40814.929217.260.297582floatnullableobalphaJ2000 USNO alpha of lensed objectdeg0.24915648.608244.35318.94359.8861doublenullableobdeltaJ2000 USNO delta of lensed objectdeg-88.0475-71.374-39.956655.318986.76511doublenullableobalphaerrPositional error of lensed object in alphadeg2.78e-071.83e-053.69e-054.53e-054.53e-051floatnullableobdeltaerrPositional error of lensed object in deltadeg2.78e-071.83e-053.69e-054.53e-054.53e-051floatnullableobpmalphaObject PM in alphadeg/yr-0.00024123-7.31901e-05-5.1667e-077.20873e-050.000314981floatnullableobpmdeltaObject PM in deltadeg/yr-0.00031425-9.4e-05-6.5972e-076.94153e-050.00038971floatnullableobpmalphaerrError of Object PM in alphadeg/yr1.39e-071.08e-064.47e-068e-069.03e-061floatnullableobpmdeltaerrError of Object PM in deltadeg/yr1.39e-071.08e-064.47e-068e-069.03e-061floatnullableobbUSNO-B B mag magnitude of lensed4.112.918.6421.48500.863524floatnullableobrUSNO-B R mag magnitude of lensed3.5611.3217.7821500.947156floatnullableobiUSNO-B I mag magnitude of lensed3.6410.6316.8118.82500.605016floatnullableobj2MASS J mag magnitude of lensed3.0829.19615.056516.69117.7750.268697floatnullableobh2MASS H mag magnitude of lensed2.848.4691914.35816.142317.50.268697floatnullableobk2MASS K mag magnitude of lensed2.798.2123714.01816.170417.0670.268697floatnullablemindateEstimated time of closest approach (julian year)yr19501978.092012.882028.521001floatnullablemindateerrError in estimation of time of closest approachyr0.04204410.2029311.0927338.46484.86724e+101floatnullablemindistEstimated minimal distancedeg09.76927e-060.0002025640.0008782090.003277041floatnullablemindisterrError in estimation of minimal distancedeg6.55068e-062.98734e-057.24038e-050.0002352652.791031floatnullableconfirmed1 if lensing event confirmedbooleanplts This service publishes plate scans of the Palomar-Leiden Troian surveys conducted between 1960 and 1977. The surveys led to the discovery of more than 2,000 asteroids (1,800 with orbital information), with another 2,400 asteroids, including 19 Trojans, found after further analysis of the plates. Note that because of the large size of the plates, in this service each original plate is contained in two parts, marked with "_1" and "_2", respectively. The central parts of the two parts overlap.plts.data This service publishes plate scans of the Palomar-Leiden Troian surveys conducted between 1960 and 1977. The surveys led to the discovery of more than 2,000 asteroids (1,800 with orbital information), with another 2,400 asteroids, including 19 Trojans, found after further analysis of the plates. Note that because of the large size of the plates, in this service each original plate is contained in two parts, marked with "_1" and "_2", respectively. The central parts of the two parts overlap.699accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size627727680772384320.0772384320.01544757120.015447571201.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra0.05940230.46402611.5676356.407359.471doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec-11.4021-6.011963.3308728.172330.93051doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdVOX:Image_MJDateObs37201.337201.441043.443437.543438.51doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median4.1e-074.1e-074.1e-075.3e-075.3e-071floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max5e-075e-075e-076.6e-076.6e-071floatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min3.3e-073.3e-073.3e-074.6e-074.6e-071floatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableplatenumPlate IDmeta.idcharnullableplatepartScan index. Since the scanner used to digitise the plate was physically smaller than the plates, each plate scan consists of two parts. This number is either 1 or 2 correspondingly.meta.id.part11.01.02.021.0shortwfpdb_idPlate identifier as in the WFPDBmeta.idcharnullableexposureEffective exposure timestime.duration;obs.exposure2406007202400432001floatnullableobsnotesObservation Notesmeta.notecharnullableemulsionEmulsion of the original plateinstr.plate.emulsioncharnullablepub_didPublisher data set id; this is an identifier for the dataset in question and can be used to retrieve the data through, e.g., datalink.meta.id;meta.maincharnullableobjectSpecial object on platemeta.idcharindexednullablepolcatsmc An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.polcatsmc.data An optical polarimetric catalog for the Small Magelanic Cloud (SMC) is presented. It gives intrinsic and observed polarizations in the V-band for a total of 7207 stars located in the Northeast and Wing sections of the SMC and part of the Magellanic Bridge.7207ctObject running numbermeta.id;meta.main1217.179999999999983604.06990.8272071.0intraj2000Object Right Ascension ICRSdegpos.eq.ra;meta.main15.001715.051816.823430.324732.50431doubleindexednullabledej2000Object Declination ICRSdegpos.eq.dec;meta.main-74.6845-74.4829-72.6133-71.851-71.8081doubleindexednullablepol_obsObserved polarization in percent of total flux, obtained by determining the Q and U stokes parameters from V photometry in four different angles.0.0270.207180.9633.416645.1481floatnullablee_pol_obsError in observed polarization including pixel noise. The error is given in percent of the total flux.0.0010.0050.0860.627821.551floatnullablepa_pol_obsPosition angle of the observed polarizationdeg0.0712.67106.87170.87179.971floatnullablepol_intIntrinsic polarisation in per cent of total flux, obtained by substracting the foreground polarization due to Milky Way dust from the observed polarization pol_obs. See paper, chapter 3, for details on foreground determination.0.05240.1777220.96613.439665.40770.910087floatnullablee_pol_intError on the intrinsic polarisation, including errors on observed polarisation and the estimate of the polarization due to forground dust.0.01580.01730.08670.6288721.55020.910087floatnullablepa_pol_intPosition angle of the intrinsic polarisationdeg0.046.697.06173.623179.930.910087floatnullablevmagV band magnitude obtained by summing up the flux of the image pair in one frame and calibrating against several published catalogs (see Table 3 in the paper).magphot.mag;em.opt.V9.689914.532717.899519.508920.69861floatnullablee_vmagError in V band magnitude, including photon noise and dispersion in the magnitude calibration.magstat.error;phot.mag;em.opt.V0.00040.02190.11040.25020.27071floatnullableppakm31 These observations cover five star-forming regions in the Andromeda galaxy (M31) with optical integral field spectroscopy. Each has a field of view of roughly 1 kpc across, at 10pc physical resolution. In addition to the calibrated data cubes, we provide flux maps of the Hβ, [OIII]5007, Hα, [NII]6583, [SII]6716 and [SII]6730 line emission. Line fluxes have not been corrected for dust extinction. All data products have associated error maps.ppakm31.cubes Spectral cubes of the fields. Look for these with full metadata in the ivoa.obscore table, obs_collection 'ppakm31 cubes'.5accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Sizelongnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.size19.09.097.017226641.0longnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1020.1413209.025341.7143600.982073doublenullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9161-63.4054-18.958256.480589.9880.982073doublenullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime-6146.555450.156458.35814959214.20.620126doublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime-6146.5562865762658738.163023.50.620108doublenullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit1.23881e-173.184e-074.8e-078.6e-071.837720.996148floatnullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit1.23881e-153.6e-076.99e-071.12e-062.492820.996148floatnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins111.01.01.0382430.9981014intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins211.01.01.0382430.9981014intnullableppakm31.maps Extracted narrow-band images.30accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsRepresentative date of observation. In reality, data contributing to this observation has typically been obtained over about a month.dtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablefieldInternal designation of the field being observed.charnullablecube_idIVOA publisher DID of the originating cube.meta.ref.ivoidcharnullablecube_linkDatalink URL for the cube this line was extracted from. This can be used to access the cube using datalink.charnullableprdust A 3D map of interstellar dust reddening, covering three quarters of the sky (declinations greater than -30 degrees) out to a distance of several kiloparsecs. The map is based on high-quality stellar photometry of 800 million stars from Pan-STARRS 1 and 2MASS. The map is available for five HEALPix levels (6 through 10), published here as separate tables, map6 through map10. A union of the coverage is provided as map_union. Use its coverage column to match against other tables. See http://argonaut.rc.fas.harvard.edu/ for more details.prdust.map10 The HEALPix map for order 10 (nside=1024); the pixel scale is about 3.4'. In ADQL, all array indices are 1-based.2200000healpixThe healpix (of order 10) of which the extinction data is given. This is in Galactic l, b.pos.healpix066092.05854354.010482060.0115343351.0intindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.code01.01.01.011.0shortdm_reliable_minMinimum reliable distance modulus.mag4.1487.3948.5489.4521floatnullabledm_reliable_maxMaximum reliable distance modulus.mag5.10212.35614.16715.241floatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.number1066.0184.0897.015561.0intnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.number264.0178.0860.013921.0intnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.number047.0142.0588.09691.0intnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullableprdust.map6 The HEALPix map for order 6 (nside=64); the pixel scale is about 55'. In ADQL, all array indices are 1-based.74healpixThe healpix (of order 6) of which the extinction data is given. This is in Galactic l, b.pos.healpix1278713168.7437925.045124.62451361.0intindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.code11.01.01.011.0shortdm_reliable_minMinimum reliable distance modulus.mag5.1185.917857.10610.16881floatnullabledm_reliable_maxMaximum reliable distance modulus.mag7.6398.2339510.93351floatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.number1012.1958.5183.150000000000031951.0intnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.number910.054.5173.100000000000021911.0intnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.number07.189999999999999542.5157.480000000000021771.0intnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullableprdust.map7 The HEALPix map for order 7 (nside=128); the pixel scale is about 27'. In ADQL, all array indices are 1-based.410healpixThe healpix (of order 7) of which the extinction data is given. This is in Galactic l, b.pos.healpix5103152559.02164678.5180450.331804991.0intindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.code11.01.01.011.0shortdm_reliable_minMinimum reliable distance modulus.mag5.1435.621866.6029.431481floatnullabledm_reliable_maxMaximum reliable distance modulus.mag4.5928.6709111.19151floatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.number1014.095.0217.459999999999922371.0intnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.number714.090.5209.02261.0intnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.number09.080.5189.459999999999922091.0intnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullableprdust.map8 The HEALPix map for order 8 (nside=256); the pixel scale is about 14'. In ADQL, all array indices are 1-based.192156healpixThe healpix (of order 8) of which the extinction data is given. This is in Galactic l, b.pos.healpix2146048576.65192118.5694463.357219311.0intindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.code11.01.01.011.0shortdm_reliable_minMinimum reliable distance modulus.mag3.7765.7376.7697.571floatnullabledm_reliable_maxMaximum reliable distance modulus.mag5.85614.06215.30716.0851floatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.number10125.0181.0264.02941.0intnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.number1113.0167.0244.02751.0intnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.number0104.0153.0225.02571.0intnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullableprdust.map9 The HEALPix map for order 9 (nside=512); the pixel scale is about 6.9'. In ADQL, all array indices are 1-based.1100000healpixThe healpix (of order 9) of which the extinction data is given. This is in Galactic l, b.pos.healpix1432661010.821440316.02830307.179999999728835161.0intindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.code01.01.01.011.0shortdm_reliable_minMinimum reliable distance modulus.mag4.0836.537.6238.5051floatnullabledm_reliable_maxMaximum reliable distance modulus.mag4.67812.35714.39815.4211floatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.number1059.0132.0448.07471.0intnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.number056.0125.0430.07271.0intnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.number051.0115.0394.06211.0intnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullableprdust.map_unionThis is a view of the dust maps in the five orders, generated by splitting the larger pixels from the higher orders into HEALPixes of order 10. This means, in particular, that the spatial resolution for all pixels with original_order!=10. Use this for convenient joins to other tables.healpixThe healpix (in galactic l, b) for which this data applies. This is of the order given in the hpx_order column, and thus it's not usually useful for querying. Query against the coverage column instead.pos.healpixintindexedprimarycoverageArea (as order-10-healpix interval) covered by this healpix.phys.angAreaintindexednullableconverged1 if the line-of-sight reddening fit converged, 0 otherwise.meta.codeshortdm_reliable_minMinimum reliable distance modulus.magfloatnullabledm_reliable_maxMaximum reliable distance modulus.magfloatnullablen_starsNumber of stars used to fit the line-of-sight reddening.meta.numberintnullablen_goodThe number of stars in the sightline with good convergence, and which passed a cut on Bayesian evidence (termed "good" stars).meta.numberintnullablen_dwarfsThe number of "good" stars which are inferred to be Main-Sequence stars.meta.numberintnullablegrdiagnosticGelman-Rubin convergence diagnostic in each HEALpix; a HEALpix can be considered good if diagnostic is below 1.2.floatnullablebest_fitThe best-fit (maximum proability density) line-of-sight reddening, in units of SFD-equivalent E(B-V), in each distance bin; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags.magphys.absorptionfloatnullablesamples18 samples of E(B-V) in each distance bin drawn from the MCMC chain; the bins are 4 .. 19 mag of distance modulus, spaced 0.5 mags. This information can be used to estimate the reliability of best_fit (e.g., a standard deviation).magphys.absorption;src.samplefloatnullablehpx_orderThe HEALPix order healpix is given for. The dust map is not regularly sampled, which is why orders vary over the sky. For querying, it is simpler to look at coverage than at healpix+order.meta.number;pos.healpixshortrave The RAdial Velocity Experiment (RAVE) contains stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, chemical abundances and distances. Observations between 2003 and 2013 were used to build the five RAVE data releases.rave.dr2 The second data release of RAVE contains spectroscopic radial velocities for 49327 stars in the Milky-Way southern hemisphere using the 6dF instrument at the AAO. Stellar parameters are published for a set of 21121 stars belonging to the second year of observation. This data collection has been superceded by RAVE data release 3 (`table rave.dr </__system__/dc_tables/show/tableinfo/rave.dr3>`_ in the data center). The data published here comprises all original RAVE data. Columns in the data release that resulted from crossmatching were left out. For details, see 2008MNRAS.391..793S.51829nameTarget designationmeta.id;meta.maincharnullablealtnameTarget alternative designationmeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.002041678.64914188.417349.012359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-84.9345-74.5354-28.1774-3.150911.570971doubleindexednullableglonGalactic longitudedegpos.galactic.lon3.3430410.6975277.171349.142359.4651floatnullableglatGalactic latitudedegpos.galactic.lat-88.2274-75.9196-28.643351.764859.7411floatnullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-578.3-59789.8595.71floatnullablee_rvHRV errorkm/sstat.error00.71.86.485.81floatnullablepmraProper motion in RAmas/yrpos.pm;pos.eq.ra-0.000214389-1.38889e-055.55556e-081.45278e-050.0005138890.998572floatnullablee_pmraError in proper motion in RAmas/yrstat.error;pos.pm;pos.eq.ra03.88889e-077.77778e-073.58333e-060.0002328610.998572floatnullablepmdeProper motion in Declinationmas/yrpos.pm;pos.eq.dec-0.000245167-1.61667e-05-1.19444e-067.77778e-060.000233750.998572floatnullablee_pmdeError in proper motion in Declinationmas/yrstat.error;pos.pm;pos.eq.dec03.88889e-077.77778e-073.27778e-060.0002495830.998572floatnullablepmsrcSource of proper motion (0 - no PM; 1 - Tycho-2; 2 - Supercosmos; 3 - STARNET 2.0; 4 - GSC1.2x2MASS; 5 - UCAC-2)meta.ref;pos.pm;pos.eq.dec12.03.05.091.0shortnullableimagInput catalog I magnitudemagphot.mag;em.opt.I4.839.1110.7811.9613.021floatnullableobsdateDate of observationdtime.epoch;obscharnullablefieldName of RAVE fieldmeta.id;obs.fieldcharnullableplatePlate number usedmeta.id;instr.param11.01.02.021.0shortfiberFiber numbermeta.id16.076.0146.01501.0shortteffEffective TemperatureKphys.temperature.effective00.00.06818.159999999996271451.0intnullableloggGravityphys.gravity0004.75.091floatnullablem_h_uncalUncalibrated [M/H]phys.abund.Fe-2.48-0.8200.250.51floatnullablealfa_fealpha enhancement [{alpha}/Fe]phys.abund0000.280.41floatnullablem_hCalibrated [M/H], Sun=1phys.abund.Fe-2.05-0.3900.41.011floatnullablechi2chi squarestat.fit.chi20003679.62423501doublenullablesnrCorrected signal to noisestat.snr00077.7150.41floatnullabletdccTonry-Davis correlation coefficientstat.fit.param09.831.588.8156.11floatnullablehcpHeight of correlation peakstat.correlation00.520.910.980.991floatnullablewcpWidth of correlation peakkm/sstat.correlation04759.5109.4164011floatnullablezeropointZero point correction appliedkm/sarith.zp-19.2-3.5-0.53.858.21floatnullablehrvskyMeasured heliocentric radial velocity of skykm/sspect.dopplerVeloc;obs.field;pos.heliocentric-149-7.1-0.47.6248.81floatnullablee_hrvskyError HRV of skykm/sstat.error00.83.112.7752.91floatnullabletdccskySky Tonry-Davis correlation coefficientstat.fit.param00.46.72858.71floatnullablesnrspecSpectra signal to noise ratiostat.snr-102.622.269.4272.41floatnullablezp1Entire plate zero point correction flag [dispersion around correction <1 (A), 1..2 (B), 2..3 (C), >3 km/s (D); E - less than 15 fibers available.]meta.codecharnullablezp250 fibers group to which the fiber belongs zero point correction flagmeta.codecharnullablegapwarningFiber is close to a 15 fibers gapmeta.codebooleanqualSpectra quality flag [a - asymmetric Ca lines; c - cosmic ray pollution; e - emission line spectra; n - noise dominated spectra; l - no lines visible; w - weak lines; g - strong ghost; t - bad template fit; s - strong residual sky emission; cc - bad continuum; r - red part of the spectra shows problem; b - blue part of the spectra shows problem; p - possible binary/doubled lined; x - peculiar object;]meta.code.qualcharnullablerave.dr3 The third data release of RAVE contains spectroscopic radial velocities for 83072 stars in the Milky-Way southern hemisphere using the 6dF instrument at the AAO. This data collection has been superceded by RAVE data release 4 (`table rave.dr </__system__/dc_tables/show/tableinfo/rave.main>`_ in the data center). Columns in the data release that resulted from crossmatching were left out. For details, see 2011AJ....141..187S.83072nameTarget designationmeta.id;meta.maincharnullablealtnameTarget alternative designationmeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416710.0457190.701349.204359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-85.3074-74.3527-29.389-3.22561.570971doubleindexednullableglonGalactic longitudedegpos.galactic.lon0.000277.46166275.244351.722359.9971floatnullableglatGalactic latitudedegpos.galactic.lat-88.2274-75.5354-25.375651.57959.7411floatnullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-976.672-63.37036.61788.9365967.8871floatnullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentric00.6571.76.70987299.2151floatnullablepmraProper motion in RAdeg/yrpos.pm;pos.eq.ra-0.000214389-1.30556e-05-1.66667e-071.38333e-05277.750.989262floatnullablee_pmraError in proper motion in RAdeg/yrstat.error;pos.pm;pos.eq.ra03.05556e-077.77778e-073.44444e-06277.750.989262floatnullablepmdeProper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.000245167-1.53611e-05-1.11111e-067.25e-06277.750.989262floatnullablee_pmdeError in proper motion in Declinationdeg/yrstat.error;pos.pm;pos.eq.dec03.05556e-077.5e-073.08333e-06277.750.989262floatnullablepmsrcSource of proper motion (see note)meta.ref;pos.pm;pos.eq.dec01.05.06.060.98926234shortnullableimagInput catalog I magnitudemagphot.mag;em.opt.I-27.49.1410.8411.9613.021floatnullableobsdateDate of observationyrtime.epoch;obscharnullablefieldName of RAVE fieldmeta.id;obs.fieldcharnullableplatePlate number usedmeta.id;obs.field11.02.02.021.0shortfiberFiber numbermeta.id17.080.0146.01501.0shortteffEffective TemperatureKphys.temperature.effective34973894.135557.07721.0469350.50163716intnullableloggGravityphys.gravity0.041.073.994.895.110.501637floatnullablemetMetallicity [m/H]phys.abund.Fe-2.35-0.99-0.270.240.50.501637floatnullablealphaalpha enhancement [{alpha}/Fe]phys.abund000.070.280.40.501637floatnullablechi2Chi square of continuum fitstat.fit.chi2329.4435.1566041466.8277598.40.692809doublenullablesnr2DR2 signal to noise ratiostat.snr2.49.8431.1683.61167.080.663003floatnullablesnrPre-flux calibration signal to noisestat.snr68.629.583.5163.20.692809floatnullabletdccTonry-Davis R correlation coefficientstat.fit.param010.234.190.6687164.811floatnullablehcpHeight of correlation peakstat.correlation00.540.910.9790.991floatnullablewcpWidth of correlation peakkm/sstat.correlation048.562.278113.662683.1931floatnullablezeropointZero point correction appliedkm/sarith.zp-30.3-3.578-0.52.943.7511floatnullablehrvskyMeasured heliocentric radial velocity of skykm/sspect.dopplerVeloc;obs.field;pos.heliocentric-149.009-7.23-0.47.46115248.8040.999856floatnullablee_hrvskyError HRV of skykm/sstat.error00.8943.18812.5451752.9480.999904floatnullabletdccskySky Tonry-Davis correlation coefficientstat.fit.param00.66.8527.3558.710.999856floatnullablesnrspecSpectrum signal to noise ratiostat.snr-105.622.268.9300.70.988239floatnullablezp1Entire plate zero point correction flag (see note)meta.codecharnullablequalSpectrum quality flag (see note)meta.code.qualcharnullablemaskflagFraction of spectrum unaffected by continuum problems (see note)meta.code.qual0.030.891110.692785floatnullablerave.dr4The RAVE object catalog, data release 4. Note that columns with names ending in _k originate from the stellar parameters pipeline, those with names ending in _c come from the chemical pipeline, those with name ending in _sparv come from the radial velocity pipeline. Names ending in _n_k indicate calibrated values.482194nameTarget designationmeta.id;meta.maincharindexedprimaryaltnameRAVE target designationmeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416710.8708185.699348.023359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-87.5159-77.5138-36.1694-3.0444127.74051doubleindexednullableglonGalactic longitudedegpos.galactic.lon0.000277.05174277.426353.107359.9991doublenullableglatGalactic latitudedegpos.galactic.lat-89.8798-74.4171-21.109346.624873.63471doublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-1000.54-68.17287.49195.12481001.311floatindexednullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentric0.2730.5741.187.273448.7441floatnullableobsdateObservation date.dtime.epoch;obs52740528955461756101562811doublenullablefield_nameName of RAVE field (RA/DE)meta.id;obs.fieldcharnullableplate_numberNumber of field plate [1..3]meta.id;obs.field11.02.03.031.0shortfiber_numberNumber of optical fiber used to obtain the spectrum [1,150].meta.number;instr.setup18.076.0146.01501.0shortteff_kEffective temperature from the stellar parameter pipeline.Kphys.temperature.effective3000380048587049.2780000.932867floatnullablee_teff_kError in the effective temperature from the stellar parameter pipeline.Kstat.error;phys.temperature.effective62629527711660.932867floatnullablelogg_kLog gravity as determined by the stellar pipeline.phys.gravity00.493.184.85.50.932867floatnullablee_logg_kError in logg_k.stat.error;phys.gravity0.090.120.20.521.260.932867floatnullablemet_kMetallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5-1.57-0.470.3510.932867floatnullablemet_n_kCalibrated metallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-7.709-1.18775-0.197750.2055390.349750.932867floatnullablee_met_kError in metallicity [m/H] from the stellar parameter pipeline.stat.error;phys.abund.Z0.060.080.10.261.140.932867floatnullablesnr_kSignal to noise value for the stellar parameter pipeline.stat.snr011509620310.932867floatindexednullablealgo_conv_kQuality flag for stellar parameter pipeline [0..4].meta.code.qual000440.932867floatnullablealAbundance of Al [Al/H]phys.abund-1.84-0.67-0.070.471.10.585961floatnullableal_nNumber of spectral lines used for the computation of Al abundance.phys.abund02.02.02.020.6493859intnullablesiAbundance of Si [Si/H]phys.abund-2.34-0.73-0.040.511.10.631192floatnullablesi_nNumber of spectral lines used for the computation of Si abundance.phys.abund04.013.016.0330.6493859intnullablefeAbundance of Fe [Fe/H]phys.abund.Fe-2.71-0.94-0.230.321.040.616267floatnullablefe_nNumber of spectral lines used for the computation of Fe abundance.phys.abund116.036.054.0890.6493859intnullabletiNumber of spectral lines used for the computation of Ti abundance.phys.abund-2.67-0.71-0.10.521.10.516039floatnullableti_nNumber of used spectral lines for calculation of Ti abundance.phys.abund01.010.025.0390.6493859intnullableniAbundance of Ni [Ni/H]phys.abund-1.67-0.85-0.160.591.10.236625floatnullableni_nNumber of spectral lines used for the computation of Ni abundance.phys.abund00.00.04.060.6493859intnullablemgAbundance of Mg [Mg/H]phys.abund-2.04-0.76-0.160.381.10.621534floatnullablemg_nNumber of spectral lines used for the computation of Mg abundance.phys.abund01.03.05.070.6493859intnullablejmag2MASS J magnitudemagphot.mag;em.IR.J-2.98911.82815.54816.84322.8431floatindexednullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0690.1679.9990.953595floatnullablehmag2MASS H magnitudemagphot.mag;em.IR.H-4.00711.06314.90816.27824.2920.999999floatnullablee_hmag2MASS H total magnitude uncertaintymagstat.error;phot.mag;em.IR.H0.010.0220.0790.2139.9990.909418floatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.K-4.37810.73314.66516.20520.5320.999998floatnullablee_kmag2MASS K_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K0.0110.0210.0860.2439.9990.770189floatnullablechisq_cχ² of the Chemical Pipelinestat.fit.chi2382.6542.1723.91718.21e+060.649386floatnullableid_2mass2MASS Target designationmeta.idcharnullableid_denisDENIS Target designationmeta.idcharnullableid_usnob1USNOB1 Target designationmeta.idcharnullableid_tycho2TYCHO2 target designationmeta.idcharnullableid_ucac4UCAC4 target designationmeta.idcharnullableid_ppmxlPPMXL target designation.meta.id11529489412846565331.3073282239178688e+184.819919694503959e+186.775420030134535e+1869175240734767787700.99372864longnullableparallaxParallax (from 2014MNRAS.437..351B)maspos.parallax0.069520.2489971.546899.73911540.30.80451floatnullablee_parallaxError Parallax (from 2014MNRAS.437..351B)masstat.error;pos.parallax0.002028760.05666440.5582122.97427688.0430.80451floatnullabledist_binneyDistance (from 2014MNRAS.437..351B)kpcpos.distance0.0007883120.1154620.7820914.2611714.4870.80451floatnullablee_distError in Distance (from 2014MNRAS.437..351B)kpcstat.error;pos.distance0.0003843470.03653540.2753821.054085.415810.80451floatnullabledistance_modulusDistance modulus (from 2014MNRAS.437..351B)phot.mag.distMod-5.740335.165069.2763413.086615.79770.80451floatnullablee_distance_modulusDistance modulus (from 2014MNRAS.437..351B)stat.error;phot.mag.distMod0.02265240.3581630.6153731.405245.641650.80451floatnullablelog_avExtinction (from 2014MNRAS.437..351B)phys.absorption-3.32378-1.5398-0.7748930.02653070.807970.80451floatnullablee_log_avError in extinction (from 2014MNRAS.437..351B)stat.error;phys.absorption1.06153e-050.1276110.3426950.4401491.009130.80451floatnullablemin_dists20 minimum distances to the base spectrum given by alphabetic codes from 2012ApJS..200...14M.charnullablecorrelation_coeffTonry & Davis R correlation coefficientstat.fit.param0.048.8251.55103.46201.871floatnullablepeak_heightHeight of the correlation peak.stat.correlation0.0010.4810.9510.9830.991floatnullablepeak_widthWidth of the correlation peak.stat.correlation8.52251.315863.753103.3011434.41floatnullableskyhrvMeasured heliocentry radial velocity of the sky.km/sspect.dopplerVeloc;obs.field;pos.heliocentric-297.286-9.744-0.20711.451254.7950.995029floatnullablee_skyhrvError in the measured heliocentric velocity of the sky.km/sstat.error;spect.dopplerVeloc;obs.field;pos.heliocentric00.9715.2517.259995.5430.995037floatnullabletdccskyTonry & Davis R Sky correlation coefficient.stat.fit.param00.23.7425.299.660.995027floatnullablecorrection_rvZero point correction applied to the radial velocity solutions (see 2011AJ....141..187S).km/sarith.zp-36.953-3.533-0.5192.30543.7511floatnullablezeropoint_flagQuality flag for Zero point correctionmeta.codecharnullableteff_sparvEffective temperature as determined by the radial velocity pipeline.Kphys.temperature.effective2580358749347154508240.945928floatnullablelogg_sparvLog gravity as determined by the radial velocity pipeline.phys.gravity00.73.184.865.50.945928floatnullablealpha_sparvMetallicity as determined by the radial velocity pipeline.phys.abund.Z000.070.310.450.945928floatnullableageLogarithm of age (from 2014MNRAS.437..351B)log(a)time.age7.178949.035659.7410810.003810.080.80451floatnullablee_ageError in Age (from 2014MNRAS.437..351B)log(a)stat.error;time.age0.003448430.06653730.2718180.4821661.138460.80451floatnullablemassMass (from 2014MNRAS.437..351B)solMassphys.mass0.163050.7686651.179511.9294714.40940.80451floatnullablee_massError Mass (from 2014MNRAS.437..351B)solMassstat.error;phys.mass0.001984930.05007570.2106540.8409945.440660.80451floatnullablerave.mainThe RAVE object catalog of radial velocities, surface gravities, and chemical parameters for about 500000 stars, data release 5. We have removed almost all fields originating from crossmatches (as this is intended for use within our TAP service, where users can do the crossmatches themselves). Also, some obviously buggy columns (e.g., footprint_flag) were dropped. Note that columns with names ending in _k originate from the stellar parameters pipeline, those with names ending in _c come from the chemical pipeline. Columns ending in _n_k indicate calibrated values.520629rave_obs_idUnique Identifier for RAVE objects: Observation Date, Fieldname, Fibernumbermeta.id;meta.maincharindexedprimaryraveidMain RAVE identifiermeta.idcharnullableraj2000Right ascension (J2000.0)degpos.eq.ra;meta.main0.0020416711.6986187.976347.739359.9951doubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.main-87.5159-77.45-36.6149-3.1733327.74051doubleindexednullableglonGalactic longitudedegpos.galactic.lon0.000276.99548278.956353.304359.9991doublenullableglatGalactic latitudedegpos.galactic.lat-89.8798-73.9055-19.208346.573773.63471doublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentric-2938.4-70.2027.2697.01132667.081floatindexednullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentric00.5751.1898.1281239.511floatnullableobsdateObservation date.dtime.epoch;obs52741529195464656124563861doublenullablefield_nameName of RAVE field (RA/DE)meta.id;obs.fieldcharnullableplate_numberNumber of field plate [1..3]meta.id;obs.field11.02.03.031.0shortfiber_numberNumber of optical fiber used to obtain the spectrum [1,150].meta.number;instr.setup18.077.0127.01271.0shortteff_kEffective temperature from the stellar parameter pipeline.Kphys.temperature.effective300038004849704780000.952949floatnullablee_teff_kError in the effective temperature from the stellar parameter pipeline.Kstat.error;phys.temperature.effective4949742349810.952949floatnullablelogg_kLog gravity as determined by the stellar pipeline.phys.gravity00.493.174.825.50.952949floatnullablee_logg_kError in logg_k.stat.error;phys.gravity0.080.10.160.471.010.952949floatnullablemet_kMetallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5-1.62-0.470.410.952949floatnullablemet_n_kCalibrated metallicity [m/H] from the stellar parameter pipeline.phys.abund.Z-5.78-1.26-0.20.450.950.952949floatnullablee_met_kError in metallicity [m/H] from the stellar parameter pipeline.stat.error;phys.abund.Z0.070.080.10.211.030.952949floatnullablesnr_kSignal to noise value for the stellar parameter pipeline.stat.snr010499520310.952949floatindexednullablealgo_conv_kQuality flag for stellar parameter pipeline [0..4].meta.code.qual000440.952949floatnullablealAbundance of Al [Al/H]phys.abund-3.06-0.66-0.040.541.10.687691floatnullableal_nNumber of spectral lines used for the computation of Al abundance.phys.abund02.02.02.020.76315intnullablesiAbundance of Si [Si/H]phys.abund-3.09-0.680.010.551.090.729871floatnullablesi_nNumber of spectral lines used for the computation of Si abundance.phys.abund05.013.017.0270.7631538intnullablefeAbundance of Fe [Fe/H]phys.abund.Fe-3.02-0.89-0.160.391.10.722071floatnullablefe_nNumber of spectral lines used for the computation of Fe abundance.phys.abund116.041.056.0810.76315intnullabletiNumber of spectral lines used for the computation of Ti abundance.phys.abund-3.02-0.67-0.030.641.10.622731floatnullableti_nNumber of used spectral lines for calculation of Ti abundance.phys.abund02.013.034.0400.76315intnullableniAbundance of Ni [Ni/H]phys.abund-1.63-0.79-0.060.691.10.332246floatnullableni_nNumber of spectral lines used for the computation of Ni abundance.phys.abund00.02.04.060.76315intnullablemgAbundance of Mg [Mg/H]phys.abund-2.99-0.73-0.140.41.090.708921floatnullablemg_nNumber of spectral lines used for the computation of Mg abundance.phys.abund-22.04.05.060.7631538intnullablejmag2MASS J magnitudemagphot.mag;em.IR.J-2.98911.82815.54816.84322.8431floatindexednullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.J0.0150.0230.0690.1679.9990.953595floatnullablehmag2MASS H magnitudemagphot.mag;em.IR.H-4.00711.06314.90816.27824.2920.999999floatindexednullablee_hmag2MASS H total magnitude uncertaintymagstat.error;phot.mag;em.IR.H0.010.0220.0790.2139.9990.909418floatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.K-4.37810.73314.66516.20520.5320.999998floatnullablee_kmag2MASS K_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.K0.0110.0210.0860.2439.9990.770189floatnullablechisq_cχ² of the Chemical Pipelinestat.fit.chi20.1824.51156.51880.551e+060.76315floatnullableid_2mass2MASS Target designationmeta.idcharnullableid_denisDENIS Target designationmeta.idcharnullableid_usnob1USNOB1 Target designationmeta.idcharnullableid_tycho2TYCHO2 target designationmeta.idcharnullableid_ucac4UCAC4 target designationmeta.idcharnullableid_ppmxlPPMXL target designation.meta.id11529489412846565331.3112217555738726e+184.840295169519e+186.770253335717306e+1869175240734767787700.9986728longnullableparallaxParallax (from 2014MNRAS.437..351B)maspos.parallax0.0430.2371.5539.1521042.570.904763floatnullablee_parallaxError Parallax (from 2014MNRAS.437..351B)masstat.error;pos.parallax00.0540.5132.908266.0380.904763floatnullabledist_binneyDistance (from 2014MNRAS.437..351B)kpcpos.distance11257614512231060.904763floatnullablee_distError in Distance (from 2014MNRAS.437..351B)kpcstat.error;pos.distance041269116483700.904763floatnullabledistance_modulusDistance modulus (from 2014MNRAS.437..351B)phot.mag.distMod-5.0065.3239.23213.20216.8190.904763floatnullablee_distance_modulusDistance modulus (from 2014MNRAS.437..351B)stat.error;phot.mag.distMod0.0030.3530.6051.4036.7240.904763floatnullablelog_avExtinction (from 2014MNRAS.437..351B)phys.absorption-2.981-1.536-0.7990.0731.0610.904763floatnullablee_log_avError in extinction (from 2014MNRAS.437..351B)stat.error;phys.absorption00.1250.3460.4580.9180.904763floatnullablemin_dists20 minimum distances to the base spectrum given by alphabetic codes from 2012ApJS..200...14M.charnullablestddev_rvStandard deviation in HRV from 10 resampled spectrakm/sstat.stdev;spect.dopplerVeloc;pos.heliocentric00.1930.5954.771917.960.948952floatnullablemad_rvMedian absolute deviation in HRV from 10 resampled spectrakm/sstat.fit.residual;spect.dopplerVeloc;pos.heliocentric;stat.median00.1510.4623.6821451.920.940474floatnullablestddev_teff_kStandard deviation in Teff_K from 10 resampled spectraKstat.stdev;phys.temperature.effective08.6353395.7115452.971653.870.836511floatnullablemad_teff_kMedian absolute deviation in Teff_K from 10 resampled spectraKstat.fit.residual;phys.temperature.effective;stat.median00.980680.97394.3841977.10.754896floatnullablestddev_logg_kStandard deviation in Teff_K from 10 resampled spectrastat.stdev;phys.gravity00.030.240.943.170.836511floatnullablemad_logg_kMedian absolute deviation in metallicity from 10 resampled spectrastat.fit.residual;phys.abund.Z;stat.median00.010.20.854.510.754896floatnullablestddev_met_kStandard deviation in metallicity from 10 resampled spectrastat.stdev;phys.abund.Z00.020.130.483.290.836511floatnullablechisq_kχ² of the Stellar Parameter Pipelinestat.fit.chi24.18.816.175.21.88259e+070.952949floatnullableteff_irEffective temperature from infrared flux methodKphys.temperature.effective340037434936675196980.960811floatnullablee_teff_irError in the effective temperature from infrared flux methodKstat.error;phys.temperature.effective30491183536000.960811floatnullableir_directInfrared temperature method: IRFM -- Temperature derived from infrared flux method; CTRL -- Temperature computed via color-Teff relations; NO -- No temperature derivation possiblemeta.codecharnullablealpha_cAlpha-enhancement from chemical pipeline (log solar ratio; 'dex')phys.abund-9.99-9.990.090.451.170.763008floatnullablefrac_cFraction of spectrum used for calculation of abundancesstat.value00.921110.78943floatnullableav_schlegelTotal Extinction in V-band from 1998ApJ...500..525Smagphys.absorption0.0060.0380.2191.41303349.1740.844171floatnullablen_gauss_fitNumber of components required for multi-Gaussian distance modulus fit.meta.number11.02.03.030.9596238shortnullablegauss_mean_1Gaussian number 1 in the estimated PDF of the object distance, width.stat.fit.param-4.8294.8529.09813.198817.1450.959624floatnullablegauss_frac_1Gaussian number 1 in the estimated PDF of the object distance, weight.stat.fit.param0.3380.5110.859110.959624floatnullablegauss_mean_2Gaussian number 2 in the estimated PDF of the object distance, width.stat.fit.param-4.8206.0711.64216.9260.959624floatnullablegauss_frac_2Gaussian number 2 in the estimated PDF of the object distance, weight.stat.fit.param000.1350.4840.50.959624floatnullablegauss_mean_3Gaussian number 3 in the estimated PDF of the object distance, width.stat.fit.param-4.732005.12718.5880.959624floatnullablegauss_frac_3Gaussian number 3 in the estimated PDF of the object distance, weight.stat.fit.param0000.0340.330.959624floatnullablerep_flagTrue if the object was observed multiple timesmeta.code.qualbooleancluster_flagTrue if this was a targeted cluster observationmeta.code.qualbooleanid_tgasTGAS target designationmeta.id.cross168706316942082.4299709766774426e+185.433330854338756e+186.818433543826135e+1869174937058300416000.47942585longnullablesasmirala The Subarcsecond mid-infrared (MIR) atlas of local active galactic nuclei (AGN) is a collection of all available N- and Q-band images obtained at ground-based 8-meter class telescopes with public archives (Gemini/Michelle, Gemini/T-ReCS, Subaru/COMICS, and VLT/VISIR). It includes in total 895 images, of which 60% are perviously unpublished. These correspond to 253 local AGN with a median redshift of 0.016. The atlas contains the uniformly processed and calibrated images and nuclear photometry obtained through Gauss and PSF fitting for all objects and filters. This also includes measurements of the nuclear extensions. In addition, the classifications of extended emission (if present) and derived nuclear monochromatic 12 and 18 micron continuum fluxes are available. Finally, flux ratios with the circumnuclear MIR emission (measured by Spitzer) and total MIR emission of the galaxy (measured by IRAS) are presented.sasmirala.objectsBasic object properties and nuclear 12 and 18 micron continuum fluxes/ratios.253nameCommon object namemeta.id;meta.main1H 0419-5771RXS J112716.6+1909142MASX J03565655-40414532MASX J09180027+04250663C 1053C 1203C 1353C 2273C 2643C 2733C 2853C 293C 2933C 3053C 3173C 3213C 3273C 333C 3533C 3823C 390.33C 4033C 4243C 4453C 4493C 4523C 4593C 783C 933C 984C +73.08Ark 120Cen ACircinusCygnus AESO 103-35ESO 121-28ESO 138-1ESO 141-55ESO 198-24ESO 209-12ESO 253-3ESO 263-13ESO 286-19ESO 297-18ESO 323-32ESO 323-77ESO 33-2ESO 362-18ESO 416-2ESO 420-13ESO 428-14ESO 5-4ESO 500-34ESO 506-27ESO 511-30ESO 548-81ESO 602-25Fairall 49Fairall 51Fairall 9Fornax AH 0557-385H1143-182Hydra AI Zw 1IC 1459IC 3639IC 4329AIC 4518WIC 5063IC 883III Zw 35NIRAS 00188-0856IRAS 01003-2238IRAS 04103-2838IRAS 05189-2524IRAS 08572+3915IRAS 09149-6206IRAS 11095-0238IRAS 13349+2438IRAS 15250+3609LEDA 13946LEDA 170194LEDA 178130LEDA 549777M51aM81M87MCG-1-13-25MCG-1-24-12MCG-1-5-47MCG-2-8-14MCG-2-8-39MCG-3-34-64MCG-5-23-16MCG-6-30-15MR 2251-178Mrk 1014Mrk 1018Mrk 1239Mrk 266NEMrk 266SWMrk 3Mrk 304Mrk 509Mrk 520Mrk 573Mrk 590Mrk 841Mrk 897Mrk 915Mrk 926Mrk 937NGC 1052NGC 1068NGC 1097NGC 1144NGC 1194NGC 1275NGC 1365NGC 1386NGC 1433NGC 1553NGC 1566NGC 1614NGC 1667NGC 1808NGC 2110NGC 235ANGC 253NGC 2623NGC 2992NGC 3081NGC 3094NGC 3147NGC 3166NGC 3169NGC 3185NGC 3227NGC 3281NGC 3312NGC 3368NGC 3379NGC 3393NGC 34NGC 3486NGC 3521NGC 3607NGC 3623NGC 3627NGC 3628NGC 3660NGC 3690ENGC 3690WNGC 3718NGC 3783NGC 3982NGC 3998NGC 4051NGC 4074NGC 4111NGC 4138NGC 4151NGC 4235NGC 424NGC 4258NGC 4261NGC 4278NGC 4303NGC 4374NGC 4388NGC 4395NGC 4418NGC 4438NGC 4457NGC 4472NGC 4501NGC 4507NGC 454ENGC 4579NGC 4593NGC 4594NGC 4636NGC 4698NGC 4736NGC 4746NGC 4785NGC 4941NGC 4945NGC 4992NGC 5005NGC 5033NGC 5135NGC 5252NGC 5258NGC 526ANGC 5273NGC 5347NGC 5363NGC 5427NGC 5506NGC 5548NGC 5643NGC 5728NGC 5813NGC 5866NGC 5953NGC 5995NGC 612NGC 613NGC 6221NGC 6240NNGC 6240SNGC 6251NGC 6300NGC 676NGC 6810NGC 6814NGC 6860NGC 6890NGC 7130NGC 7172NGC 7212NGC 7213NGC 7314NGC 7469NGC 7479NGC 7496NGC 7552NGC 7582NGC 7590NGC 7592WNGC 7626NGC 7674NGC 7679NGC 7743NGC 788NGC 985PG 0026+129PG 0052+251PG 0844+349PG 2130+099PKS 1417-19PKS 1814-63PKS 1932-46PKS 2158-380PKS 2354-35Pictor ASuperantennae SUGC 12348UGC 5101Z 41-20charindexedprimaryraj2000Right Ascension J2000.0degpos.eq.ra;meta.main2.5416714.097184.74349.342359.2531doubleindexednullabledej2000Declination J2000.0degpos.eq.dec;meta.main-86.6319-62.3425-1.3911159.790682.53781doubleindexednullableprodlinkLink to a web page with images, bibliography, and other details on the source.charnullablezRedshiftsrc.redshift-0.00010.0016680.01610.1343840.35711floatnullabledDistanceMpc3.27.8871.7651.2419671floatnullableclsOptical classification (References for the collected optical AGN classifications are given in App. B of 2014MNRAS.439.1648A)src.classcharnullableu_agnClassification as AGN uncertain?meta.codebooleanbatidBAT ID from 9-month catalog (from Winter et al, 2009, 2009ApJ...690.1322W)meta.id15.482.0151.61540.3201581intnullablen_extNuclear morphology at subarcsecond resolutionmeta.code;src.morph-o?circ.ellip.spir.comp.charnullablelim12True if 12 µm flux was not detected. flu12 is a 3-sigma upper level in this case.meta.code;phot.fluxbooleanflu12Nuclear subarcsecond-scale monochromatic flux density at restframe 12 µmmJyphot.flux.density;em.IR1.63.15664.5963.37210205.81floatnullableerr121-σ uncertainty of the 12 µm continuum fluxmJystat.error;phot.flux;em.IR0.51.30918.7222.0273567.20.806324floatnullablelim18True if 18 µm flux was not detected. flu18 is a 3-sigma upper level in this case.meta.code;phot.fluxbooleanflu18Nuclear subarcsecond-scale monochromatic flux density at restframe 18 µmmJyphot.flux.density;em.IR2245.605362.953539.5619950.20.268775floatnullableerr181-σ uncertainty of the 18 µm continuum fluxmJystat.error;phot.flux;em.IR17.2435.7391.61466.50.241107floatnullablephotparLink to detailed information on the photometry sources.meta.ref;photchardunrSize constraint on the nuclear unresolved emission in pc, which is set equal to the minimum PSF FWHM (major axis) measured for the objectpcphys.size;src514124123121351floatnullablermedFlux ratio of nuclear to intermediate scale; the in Spitzer/IRS unresolved flux component is used as measure for the intermediate-scale emission.phot.flux;arith.ratio0.020.060.721.14221.40.84585floatnullablerlarFlux ratio of nuclear to large scale; the IRAS 12 µm flux is used as measure for the large-scale emission.phot.flux;arith.ratio0.00080.003390.30521.377121.82460.833992floatnullablepathcompInterally usedcharnullablesasmirala.photparPhotometric parameters for all nuclear measurements.901nameCommon object namemeta.id;meta.main1H 0419-5771RXS J112716.6+1909142MASX J03565655-40414532MASX J09180027+04250663C 1053C 1203C 1353C 2273C 2643C 2733C 2853C 293C 2933C 3053C 3173C 3213C 3273C 333C 3533C 3823C 390.33C 4033C 4243C 4453C 4493C 4523C 4593C 783C 933C 984C +73.08Ark 120Cen ACircinusCygnus AESO 103-35ESO 121-28ESO 138-1ESO 141-55ESO 198-24ESO 209-12ESO 253-3ESO 263-13ESO 286-19ESO 297-18ESO 323-32ESO 323-77ESO 33-2ESO 362-18ESO 416-2ESO 420-13ESO 428-14ESO 5-4ESO 500-34ESO 506-27ESO 511-30ESO 548-81ESO 602-25Fairall 49Fairall 51Fairall 9Fornax AH 0557-385H1143-182Hydra AI Zw 1IC 1459IC 3639IC 4329AIC 4518WIC 5063IC 883III Zw 35NIRAS 00188-0856IRAS 01003-2238IRAS 04103-2838IRAS 05189-2524IRAS 08572+3915IRAS 09149-6206IRAS 11095-0238IRAS 13349+2438IRAS 15250+3609LEDA 13946LEDA 170194LEDA 178130LEDA 549777M51aM81M87MCG-1-13-25MCG-1-24-12MCG-1-5-47MCG-2-8-14MCG-2-8-39MCG-3-34-64MCG-5-23-16MCG-6-30-15MR 2251-178Mrk 1014Mrk 1018Mrk 1239Mrk 266NEMrk 266SWMrk 3Mrk 304Mrk 509Mrk 520Mrk 573Mrk 590Mrk 841Mrk 897Mrk 915Mrk 926Mrk 937NGC 1052NGC 1068NGC 1097NGC 1144NGC 1194NGC 1275NGC 1365NGC 1386NGC 1433NGC 1553NGC 1566NGC 1614NGC 1667NGC 1808NGC 2110NGC 235ANGC 253NGC 2623NGC 2992NGC 3081NGC 3094NGC 3147NGC 3166NGC 3169NGC 3185NGC 3227NGC 3281NGC 3312NGC 3368NGC 3379NGC 3393NGC 34NGC 3486NGC 3521NGC 3607NGC 3623NGC 3627NGC 3628NGC 3660NGC 3690ENGC 3690WNGC 3718NGC 3783NGC 3982NGC 3998NGC 4051NGC 4074NGC 4111NGC 4138NGC 4151NGC 4235NGC 424NGC 4258NGC 4261NGC 4278NGC 4303NGC 4374NGC 4388NGC 4395NGC 4418NGC 4438NGC 4457NGC 4472NGC 4501NGC 4507NGC 454ENGC 4579NGC 4593NGC 4594NGC 4636NGC 4698NGC 4736NGC 4746NGC 4785NGC 4941NGC 4945NGC 4992NGC 5005NGC 5033NGC 5135NGC 5252NGC 5258NGC 526ANGC 5273NGC 5347NGC 5363NGC 5427NGC 5506NGC 5548NGC 5643NGC 5728NGC 5813NGC 5866NGC 5953NGC 5995NGC 612NGC 613NGC 6221NGC 6240NNGC 6240SNGC 6251NGC 6300NGC 676NGC 6810NGC 6814NGC 6860NGC 6890NGC 7130NGC 7172NGC 7212NGC 7213NGC 7314NGC 7469NGC 7479NGC 7496NGC 7552NGC 7582NGC 7590NGC 7592WNGC 7626NGC 7674NGC 7679NGC 7743NGC 788NGC 985PG 0026+129PG 0052+251PG 0844+349PG 2130+099PKS 1417-19PKS 1814-63PKS 1932-46PKS 2158-380PKS 2354-35Pictor ASuperantennae SUGC 12348UGC 5101Z 41-20charnullableraj2000Right Ascension J2000.0degpos.eq.ra;meta.main2.5416714.097184.74349.342359.2531doublenullabledej2000Declination J2000.0degpos.eq.dec;meta.main-86.6319-62.3425-1.3911159.790682.53781doublenullablefilterFilter namemeta.id;instr.filtercharnullableaccrefAccess key for the datameta.ref.urlAccess.ReferencecharnullableprodlinkLink to a web page with images, bibliography, and other details on the source.charnullablew_obsFilter central wavelength (observing frame)umem.wl.central;instr.filter7.78.5911.618.7219.51floatnullablehwidthFilter half-width-half-maximumuminstr.bandwidth0.10.160.422.642.641floatnullableinstrInstrument used to obtain the datameta.id;instrcharnullablepfovPixel size of field of viewarcsec/pixphys.angSize;instr.pixel0.0750.0750.0750.1330.1331floatnullableexptimeTotal exposure time on-sourcestime.duration;obs.exposure563362320870731floatnullablemodeChop and nod modeinstr.setupcharnullablecthrowChop throwarcsecinstr.param58816301floatnullablecangleChop angledeginstr.param-350-9003364261floatnullablerotaInstrument rotation angle, west of north.deginstr.param;pos.posAng-303-200901401floatnullableproidObservation program IDmeta.id;obscharnullablecalnameCalibrator star namemeta.id;obs.calibcharnullablecalmjdMJD of observation of calibrator stardtime.epoch;obs.calib52975.153275.754724.255593.455727.10.970033floatnullabledateobsMJD of observationdtime.epoch;obs52975.153194.25472055584.555727.11doublenullableconvfConversion factor measured from the CalibrationmJy/ctphot.calib0.00650.009090.052841.1225510.03241floatnullableeconvf1-sigma uncertainty of the Conversion factormJy/ctstat.error;phot.calib6e-050.000110.000850.0256411floatnullablecalfluCalibrator star fluxmJyphot.flux;obs.calib1374.32518.958761.141990.21.0716e+060.970033floatnullablelimgaussIf True, the object was not detected using Gauss fitting or no matching calibrator star was available. In that case, F_Gauss represents a 3-sigma upper limit.meta.codebooleanfgaussNuclear flux measured through Gauss fittingmJyphot.flux;em.IR26.3145.38189.766926.41floatnullableefgauss1-sigma uncertainty in nuclear flux measured through Gauss fittingmJystat.error;phot.flux;em.IR0.20.79210.2331.785902.30.849057floatnullablelimpsfIf True, the object was not detected using PSF fitting or no matching calibrator star was available. In that case, F_PSF represents a 3-sigma upper limit.meta.codebooleanfpsfNuclear flux measured through PSF fittingmJyphot.flux;em.IR1.64.8107.76307.331349.51floatnullableefpsf1-sigma uncertainty in nuclear flux measured through PSF fittingmJystat.error;phot.flux;em.IR0.20.710.45337.89526490.82131floatnullablecalfmaCalibrator Star major axis FWHMarcsecphys.angSize;obs.calib0.260.30.40.710.970033floatnullablecalfmiCalibrator Star minor axis FWHMarcsecphys.angSize;obs.calib0.240.270.360.580.970.970033floatnullablecalpaCalibrator Star position angle, north over eastdegpos.posAng;obs.calib011.191031701790.970033floatnullablefwhmmaMajor axis FWHM (constrained to <=1arcsec) of the Gaussian fit of the target objectarcsecphys.angSize;src0.260.320.46110.802442floatnullablefwhmmiMinor axis FWHM (constrained to <=1arcsec) of the Gaussian fit of the target objectarcsecphys.angSize;src0.190.280.390.7810.802442floatnullablepaPosition Angle, north over east, of the Gaussian fit of the target objectdegpos.posAng;src07.32941751800.802442floatnullablesmakced The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED_) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with `resulting decompositions`_ and other properties of the galaxies in the sample. .. _SMAKCED: http://smakced.net .. _resulting decompositions: http://smakced.net/data.htmlsmakced.mainSMAKCED infrared images and derived properties of early-type dwarf galaxies in the Virgo cluster.119accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size83952008395200.016807680.020107411.199999996248313601.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra182.344183.888187.375191.729192.561doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec3.67787.4744212.162816.134818.19731doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsApproximate observation date (essentially, month and year should be about right). NULL for archival materialdtime;obs.exposure55211552115530156001560010.806723doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median1.651e-061.651e-061.651e-061.651e-061.651e-061floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max1.85e-061.85e-061.85e-061.85e-061.85e-061floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min1.44e-061.44e-061.44e-061.44e-061.44e-061floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableobjectCommon name of the observed galaxy.meta.id;meta.maincharraj2000ICRS RA of galaxy center from asymmetry centering (unless specified otherwise in remarks).degpos.eq.ra;meta.main182.343183.894187.379191.731192.561doublenullabledej2000ICRS Declination of galaxy center from asymmetry centering (unless specified otherwise in remarks).degpos.eq.dec;meta.main3.682227.4768112.155816.127218.19671doublenullableexptimeTotal integration time for the object (sum of exposure times of all images stacked; note that different telescopes were in use).stime.duration;obs.exposure360424.8378011100133201floatnullableseeingEstimate for the seeing at observation time.arcsecinstr.obsty.seeing0.590.67540.911.71.991floatnullablesnrSignal to noise ratio for a pixel at 2 r_e.stat.snr0.20.31.312.00490.90.840336floatnullablehmagTotal H-band magnitude of the galaxyphot.mag;em.ir.H9.579.891611.7212.673812.861floatnullabler_eEffective radius of the galaxy (semi-major axis of half-light aperture in H).arcsecphys.angSize2.66.11816.229.61246.81floatnullableb_aAxis raio at 2 r_ephys.angSize;arith.ratio0.290.320.680.970.981floatnullableconcentrationConcentration index 5 log_80/r_20 as in 2000AJ....119.2645Bphys.size;arith.ratio2.322.60543.093.82363.951floatnullablerho10Local projected number density of cluster galaxies. (see Appendix D in the source)log(deg**-2)src.density0.991.352.042.54922.691floatnullableremarksMorphological features from 2006AJ....132.2432L and other remarksmeta.notecharnullablemoreinfoBibcodes of papers containing more information.meta.refcharnullablestructgroupStructural Group (see 2012ApJ...745L..24J) resulting from the decomposition.meta.code.classcharnullablesimp_mIntegrated H-band brightness, simple modelmagphot.mag;em.ir.H9.569.984111.7712.612712.950.773109floatnullablesimp_rcHalf-light radius, simple modelarcsecphys.angSize;src3.96.2315.7529.40535.60.773109floatnullablesimp_nSérsic index, simple modelstat.fit.param0.720.831.482.92854.040.773109floatnullablesimp_b_aAxis ratio, simple modelphys.angSize;arith.ratio0.440.46730.7550.96270.980.773109floatnullableinner_mIntegrated H-band brightness, inner componentmagphot.mag;em.ir.H11.0111.47413.23515.193216.760.420168floatnullableinner_rcHalf-light radius, inner componentarcsecphys.angSize;src1.41.9885.714.94218.90.420168floatnullableinner_nSérsic index, inner componentstat.fit.param0.650.75351.143.25783.540.420168floatnullableinner_b_aAxis ratio, inner componentphys.angSize;arith.ratio0.350.40820.720.930.970.420168floatnullableouter_mIntegrated H-band brightness, global/outer componentmagphot.mag;em.ir.H9.9310.441211.8113.01213.310.546219floatnullableouter_rcHalf-light radius, global/outer componentarcsecphys.angSize;src5.87.84419.635.51252.20.546219floatnullableouter_nSérsic index, global/outer componentstat.fit.param0.270.465212.05363.020.546219floatnullableouter_b_aAxis ratio, global/outer componentphys.angSize;arith.ratio0.430.45920.730.960.960.546219floatnullablesimpdec_rffResidual flux fraction (2006ApJ...644...30B) for the single decompositionstat.fit.goodness-0.078-0.041920.0120.068320.2230.663866floatnullablesimpdec_eviExcess variance index (2011MNRAS.411.2439H) for single decompositionstat.fit.goodness-0.19-0.147660.0762.450345.850.663866floatnullablefinaldec_rffResidual flux fraction (2006ApJ...644...30B) for the final decompositionstat.fit.goodness-0.047-0.025450.0090.023580.0290.487395floatnullablefinaldec_eviExcess variance index (2011MNRAS.411.2439H) for final decompositionstat.fit.goodness-0.126-0.122450.05251.639122.5870.487395floatnullablecompmorphAdditional information on decomposition.meta.note;src.morphcharnullabletenpc A catalogue of 541 nearby (within 10pc of the sun) stars, brown dwarfs, and confirmed exoplanets in 336 systems, as well 21 candidates, compiled from SIMBAD and several other sources. Where available, astrometry and photometry from Gaia eDR3 has been inserted.tenpc.main A catalogue of 541 nearby (within 10pc of the sun) stars, brown dwarfs, and confirmed exoplanets in 336 systems, as well 21 candidates, compiled from SIMBAD and several other sources. Where available, astrometry and photometry from Gaia eDR3 has been inserted.562nb_objRunning number for object, ordered by increasing distancemeta.id;meta.mainshortnb_sysRunning number for system, ordered by increasing distancemeta.id.parentshortsystem_nameName of the systemmeta.id.parentcharnullableobj_catOne of Star (*), LM (low mass star), BD (brown dwarf), WD (white dwarf), or Planetmeta.code.class*LMLM?BDBD?WDWD?Planetcharnullableobj_nameAdopted name of the objectmeta.idcharnullableraRight ascension at epoch (ICRS)degpos.eq.ra;meta.maindoubleindexednullabledecDeclination at epoch (ICRS)degpos.eq.dec;meta.maindoubleindexednullableepochEpoch for ra and decyrtime.epochfloatnullableparallaxTrigonometric parallaxmaspos.parallax.trigdoublenullableparallax_errorParallax uncertaintymasstat.error;pos.parallaxdoublenullableparallax_bibcodeReference for the parallax; missing values here mean the parallax is taken from another member of the systemmeta.bib;pos.parallaxcharnullablepmraProper motion in right ascensionmas/yrpos.pm;pos.eq.radoublenullablepmra_errorProper motion uncertainty in right ascensionmas/yrstat.error;pos.pm;pos.eq.radoublenullablepmdecProper motion in declinationmas/yrpos.pm;pos.eq.decdoublenullablepmdec_errorProper motion uncertainty in declinationmas/yrstat.error;pos.pm;pos.eq.decdoublenullablepm_bibcodeReference for the proper motion; missing values here mean that the proper motion was taken from another member of the systemmeta.ref;pos.pm;pos.eq.racharnullablervLine-of-sight velocitykm/sspect.dopplerVelocfloatnullablerv_errorLine-of-sight velocity uncertaintykm/sstat.error;spect.dopplerVelocfloatnullablerv_bibcodeReference for the line-of-sight velocitymeta.ref;spect.dopplerVeloccharnullablesp_typeSpectral typesrc.sptypecharnullablesp_bibcodeReference for spectral typemeta.ref;src.sptypecharnullablesp_methodMethod used to derive the spectral typemeta.codecharnullableg_codeSource of the value of the G magnitude (see note)meta.code;phot.mag;em.opt.Vshortnullablemag_gGaia G band magnitude measured (when g_code is 2 or 3)magphot.mag;em.opt.Vdoublenullablemag_g_estimateEstimated Gaia G band magnitude (when g_code is not 2 or 3)magphot.mag;em.opt.Vfloatnullablemag_gbpGaia BP band magnitudephot.mag;em.opt.Bdoublenullablemag_grpGaia RP band magnitudephot.mag;em.opt.Rdoublenullablemag_uMagnitude in Umagphot.mag;em.opt.Ufloatnullablemag_bMagnitude in Bmagphot.mag;em.opt.Bfloatnullablemag_vMagnitude in Vmagphot.mag;em.opt.Vfloatnullablemag_rMagnitude in Rmagphot.mag;em.opt.Rfloatnullablemag_iMagnitude in Imagphot.mag;em.opt.Ifloatnullablemag_jMagnitude in Jmagphot.mag;em.ir.Jfloatnullablemag_hMagnitude in Hmagphot.mag;em.ir.Hfloatnullablemag_kMagnitude in Kmagphot.mag;em.ir.Kfloatnullablesystem_bibcodeReference for multiplicity or exoplanetsmeta.refcharnullableexoplanet_countNumber of confirmed exoplanetsmeta.numbershortnullablegaia_dr2Gaia DR2 identifiermeta.id.crosslongnullablegaia_edr3Gaia DR3 identifiermeta.id.crosslongnullablesimbad_nameName resolved by SIMBADmeta.id.crosscharnullablecommon_nameCommon namemeta.idcharnullablegjGliese and Jahreiß catalogue identifiermeta.id.crosscharnullablehdHenry Draper catalogue identifiermeta.id.crosscharnullablehipHipparcos catalogue identifiermeta.id.crosscharnullablecommentAdditional comments on exoplanets, multiplicity, etcmeta.notecharnullabletoss This service provides oscillator strengths and transition probabilities. Mainly based on experimental energy levels, these were calculated with the pseudo-relativistic Hartree-Fock method including core-polarization corrections.toss.dataA table of transitions, their species, and their properties.930656wavelengthWavelength of the transition.mem.wlssldm:Line.wavelength.valuedoubleindexedlinenameTerse descriptor of the linemeta.id;em.linessldm:Line.titlecharchemical_elementElement transitioningphys.atmol.elementssldm:Line.species.nameCuZnGaGeSeKrSrZrMoTcTeIXeBacharindexednullableinitial_nameName of the level the atom or molecule starts in.phys.atmol.initial;phys.atmol.levelssldm:Line.initialLevel.namecharnullablefinal_nameName of the level the atom or molecule ends up in.phys.atmol.final;phys.atmol.levelssldm:Line.finalLevel.namecharnullableinitial_level_energyEnergy of the level the atom or molecule starts in.Jphys.energy;phys.atmol.initial;phys.atmol.leveldoublenullablefinal_level_energyEnergy of the level the atom or molecule ends up in.Jphys.energy;phys.atmol.final;phys.atmol.leveldoublenullablepubThe publication this value originated from.meta.bibcharnullableid_statusIdentification status of the linemeta.codecharnullableion_stageIonisation stagephys.atmol.ionStagecharindexednullablec_wavelengthConventional wavelength of the transition. This is the air wavelength between 2000 and 20000 Angstrom, the vacuum wavelength otherwise.Angstromem.wl;phys.atmol.transitiondoubleindexednullablepar_initParity of the init level of the transitionphys.atmol.parityeocharj_initAngular momentum quantum number of the init level of the transition.phys.atmol.qnfloatnullablepar_finalParity of the final level of the transitionphys.atmol.parityeocharj_finalAngular momentum quantum number of the final level of the transition.phys.atmol.qnfloatnullablelog_gfCalculated HRF log(gf) (g -- statistical weight of the lower level; f -- oscillator strength)phys.atmol.wOscStrength-9.871.57floatnullablegaTransition probability times the statistical weight of the upper level1e9s**-1phys.atmol.transProbfloatnullablecfCancellation factor as defined by 1981tass.book.....Cfloatnullabletoss.line_tap This table contains line metadata computed a pseudo-relativistic Hartree-Fock method including core-polarization corrections. Its schema follows the first Working Draft of LineTAP.ivo://ivoa.net/std/linetap#lines-1.0titleHuman-readable line designation.meta.idcharindexedvacuum_wavelengthVacuum wavelength of the transitionAngstromem.wldoubleindexedvacuum_wavelength_errorTotal error in vacuum_wavelengthAngstromstat.error;em.wldoublenullablemethodMethod the wavelength was obtained with (XSAMS controlled vocabulary)meta.code.classobservedtheoryritzcharnullableelementElement name for atomic transitions, NULL otherwise.phys.atmol.elementcharindexednullableion_chargeTotal charge (ionisation level) of the emitting particle.phys.electChargeintindexedmass_numberNumber of nucleons in the atom or moleculephys.atmol.weightintnullableupper_energyEnergy of the upper stateJphys.energy;phys.atmol.initialdoublenullablelower_energyEnergy of the lower stateJphys.energy;phys.atmol.finaldoublenullableinchiInternational Chemical Identifier InChI.meta.id;phys.atmol;meta.maincharinchikeyThe InChi key (hash) generated from inchi.meta.id;phys.atmolchareinstein_aEinstein A coefficient of the radiative transition.phys.atmol.transProbdoublenullablexsams_uriA URI for a full XSAMS description of this line.meta.refcharnullableline_referenceReference to the source of the line data; this could be a bibcode, a DOI, or a plain URI.meta.refcharwfpdb The Wide-Field Plate Database (WFPDB_) contains the descriptive information for the astronomical wide-field (>1°) photographic observations stored in numerous archives all over the world. The total number of these observations, obtained since the end of the 19th century with more then 200 instruments (telescopes) is about 2 550 000 from 509 archives. The WFPDB is continually being updated, providing currently access to the information for about 640 000 plates from 117 plate archives (30% of the estimated total number of wide-field plates) .. _WFPDB: http://www.skyarchive.org/wfpdb.archives A table of plate archives included in the WFPDB or scheduled for inclusion, as well as the properties of the instruments used to take the data.509instr_idWFPDB-internal instrument designationmeta.id;instrcharnullablearchive_idWFPDB-internal archive designation, consisting of the instrument id, the archive code, and the site code.meta.id;meta.maincharindexedprimarywfpdb_statusInclusion status of plates from this archive: * - at disposal in SSADC, not yet converted in computer-readable form, ** - in preparation in SSADC, converted in computer readable form, *** - included in the WFPDB and available on-line.meta.codecharnullableinstr_nameOriginal name of the instrument as used by the relevant observatorymeta.id;instrcharnullablearchive_locationLocation of the plate archivemeta.id;instr.obstycharnullablearch_partCode for a sub-archive when an instrument's archive is split across several sitesintinst_nameName of the hosting institutioncharnullablesite_codeCode for the instrument site when the instrument was operated from several locations.meta.idcharsite_nameObservatory sitemeta.id;instr.obstycharnullablecountryCountry the observatory is located in.meta.id;pos.earthcharnullablempc_numberMinor Planet Center observatory codemeta.id;instr.obstyintnullabletime_zoneTime difference to Greenwichhtime;arith.difffloatnullablelongGeographical longitude of the observatory.degpos.earth.lonfloatnullablelatGeographical latitude of the observatory.degpos.earth.latfloatnullablealtitudeAltitude of the observatory.mpos.earth.altitudefloatnullablen_tubesNumber of telescope tubes.meta.number;instr.telcharnullableapertureClear aperture of the telescope.mphys.size;instr.telfloatnullablediameterDiameter of the primary mirror or the objective lensmfloatnullablefocal_lengthFocal length of the telescopeminstr.tel.focalLengthfloatnullableplate_scalePlate scalearcsec/mmfloatnullableinst_typeInstrument type: Ast-astrograph, Cam-camera, FEC-fish eye camera, Men-meniscus, RCr-Ritchey-Chretien, Rfl-reflector, Rfr- refractor, Sch-Schmidtcharnullableang_sizeMaximum angular size of the field of view.degphys.angsize;instr.fovfloatnullableop_beginYear telescope operations started.yrtime.epochfloatnullableop_endYear telescope operations ended.yrtime.epochfloatnullabledet_typeDetector used: blank--plate, F--film, X--film and platemeta.code;instrcharnullablen_directNumber of direct plates in the archive.meta.number;obsintnullablen_prismNumber of prism plates in the archive.meta.number;obsintnullablecontactName of the contact person.charnullablewfpdb.main WFPDB's table of plates, including position observed and the epoch of observation.609884instr_idWFPDB instrument identifier. TDB: Foreign keymeta.id;instrcharindexednullablewfpdbidWFPDB identifier of the plate, consisting of an observatory identifier, the instrument aperture, an instrument suffix, a plate number, and a suffix to it.meta.id;meta.maincharindexedprimaryraj2000Right ascension of the plate center (ICRS)degpos.eq.ra;meta.mainfloatindexednullabledej2000Declination of the plate center (ICRS)degpos.eq.dec;meta.mainfloatindexednullablecoord_problemQuality flag for the coordinates (empty means no known problems)meta.notecharnullableepochEpoch of observation start (UT)yrtime.epoch1858.882189.01doubleindexednullabletime_problemQuality flag for the epoch (empty means no known problems)meta.notecharnullableobjectObject or field name as given by observermeta.id;srcunicodeCharindexednullableobject_typeType of the target objectsrc.classcharindexednullablemethodMethod of observationinstr.setupcharnullableexptimeExposure time (for multiple exposures, this is for the first exposure; for the others, see notes)stime.duration;obs.exposurefloatnullableemulsionEmulsion typeinstr.plate.emulsioncharnullablefilterFilter typemeta.id;instr.filtercharnullablewavebandSpectral Bandinstr.bandpasscharindexednullablexsizeWidth of the platecmphys.size;instr.detfloatnullableysizeHeight of the platecmphys.size;instr.detfloatnullableobserverName(s) of the persons having performed the observation.obs.observerunicodeCharnullablenotesVarious longer remarksmeta.noteunicodeCharnullablequalityQuality-related information in free text.meta.noteunicodeCharnullableavailabilityFree text on how to find the plate.meta.notecharnullabledigitizationInformation on possible ways to access plate scans in free text.meta.noteunicodeCharnullablewfpdb.archivesinstr_idinstr_idmcextinct A catalogue of E(V-I) extinction values is presented for 3174 (LMC) and 693 (SMC) fields within the Magellanic Clouds. The extinction values were computed by determining the (V-I) colour difference of the red clump from Optical Gravitational Microlensing Experiment (OGLE III) observations in the V and I bands and theoretical values for unreddend red clump colours.mcextinct.exts Extinction values within certain areas in the Magellanic clouds.3867bboxBounding box for the extinction datapos.outline;obs.fielddoublenullablecenteralphaArea center RA ICRSdegpos.eq.ra;meta.main5.3051710.347779.30488.743294.52271floatindexednullablecenterdeltaArea center Declination ICRSdegpos.eq.dec;meta.main-74.6606-73.7765-69.919-67.6284-66.72681floatindexednullableev_iReddening (color difference between observation and theory, V-I)magphot.color.excess;em.opt.V;em.opt.I-0.010.020.070.180.431floatnullablesig_ev_iDifferential reddening calculated as FWHM of the red clump star distributionmagstat.stdev;phot.color.excess0.0610.0680.09150.14150.21951floatnullablempc Complete Asteroid Data from the Minor Planet Center (MPC), updated once per month. The MPC operates at the Smithsonian Astrophysical Observatory under the auspices of Division III of the International Astronomical Union (IAU); for the upstream data, see https://www.minorplanetcenter.net/data. The MPC Orbit database contains orbital elements of minor planets that have been published in the Minor Planet Circulars, the Minor Planet Orbit Supplement and the Minor Planet Electronic Circulars.mpc.epn_core The EPN-TAP 2.0 version of the complete asteroid data from the Minor Planet Center (MPC), updated once per month. The MPC operates at the Smithsonian Astrophysical Observatory under the auspices of Division III of the International Astronomical Union (IAU). The MPC Orbit database contains orbital elements of minor planets that have been published in the Minor Planet Circulars, the Minor Planet Orbit Supplement and the Minor Planet Electronic Circulars.ivo://ivoa.net/std/epntap#table-2.0granule_uidInternal table row index, which must be unique within the table. Can be alphanumeric.meta.idchargranule_gidCommon to granules of same type (e.g. same map projection, or geometry data products). Can be alphanumeric.meta.idcharobs_idAssociates granules derived from the same data (e.g. various representations/processing levels). Can be alphanumeric, may be the ID of original observation.meta.id;obschardataproduct_typeThe high-level organization of the data product, from a controlled vocabulary (e.g., 'im' for image, sp for spectrum). Multiple terms may be used, separated by # characters.meta.code.classimmaspdsscprpfvomocutscacisvevcharnullabletarget_nameStandard IAU name of target (from a list related to target class), case sensitivemeta.id;srcunicodeCharnullabletarget_classType of target, from a controlled vocabulary.src.classasteroiddwarf_planetplanetsatellitecometexoplanetinterplanetary_mediumsampleskyspacecraftspacejunkstarcalibrationcharnullabletime_minAcquisition start time (in JD), as UTC at time_refpositiondtime.start;obsdoublenullabletime_maxAcquisition stop time (in JD), as UTC at time_refpositiondtime.end;obsdoublenullabletime_sampling_step_minSampling time for measurements of dynamical phenomena, lower limit.stime.resolution;stat.mindoublenullabletime_sampling_step_maxSampling time for measurements of dynamical phenomena, upper limitstime.resolution;stat.maxdoublenullabletime_exp_minIntegration time of the measurement, lower limit.stime.duration;obs.exposure;stat.mindoublenullabletime_exp_maxIntegration time of the measurement, upper limitstime.duration;obs.exposure;stat.maxdoublenullablespectral_range_minSpectral range (frequency), lower limit.Hzem.freq;stat.mindoublenullablespectral_range_maxSpectral range (frequency), upper limitHzem.freq;stat.maxdoublenullablespectral_sampling_step_minSpectral sampling step, lower limit.Hzem.freq;spect.binSize;stat.mindoublenullablespectral_sampling_step_maxSpectral sampling step, upper limitHzem.freq;spect.binSize;stat.maxdoublenullablespectral_resolution_minSpectral resolution, lower limit.spect.resolution;stat.mindoublenullablespectral_resolution_maxSpectral resolution, upper limitspect.resolution;stat.maxdoublenullablec1minRight Ascension (ICRS), lower limit.degpos.eq.ra;stat.mindoublenullablec1maxRight Ascension (ICRS), upper limitdegpos.eq.ra;stat.maxdoublenullablec2minDeclination (ICRS), lower limit.degpos.eq.dec;stat.mindoublenullablec2maxDeclination (ICRS), upper limitdegpos.eq.dec;stat.maxdoublenullablec3minDistance from coordinate origin, lower limit.AUpos.distance;stat.mindoublenullablec3maxDistance from coordinate origin, upper limitAUpos.distance;stat.maxdoublenullables_regionObsCore-like footprint, valid for celestial, spherical, or body-fixed framespos.outline;obs.fieldcharnullablec1_resol_minResolution in the first coordinate, lower limit.degpos.angResolution;stat.mindoublenullablec1_resol_maxResolution in the first coordinate, upper limitdegpos.angResolution;stat.maxdoublenullablec2_resol_minResolution in the second coordinate, lower limit.degpos.angResolution;stat.mindoublenullablec2_resol_maxResolution in the second coordinate, upper limitdegpos.angResolution;stat.maxdoublenullablec3_resol_minResolution in the third coordinate, lower limit.AUpos.resolution;stat.mindoublenullablec3_resol_maxResolution in the third coordinate, upper limitAUpos.resolution;stat.maxdoublenullablespatial_frame_typeFlavor of coordinate system, defines the nature of coordinates. From a controlled vocabulary, where 'none' means undefined.meta.code.class;pos.framecelestialbodycartesiancylindricalsphericalnonecharnullableincidence_minIncidence angle (solar zenithal angle) during data acquisition, lower limit.degpos.incidenceAng;stat.mindoublenullableincidence_maxIncidence angle (solar zenithal angle) during data acquisition, upper limitdegpos.incidenceAng;stat.maxdoublenullableemergence_minEmergence angle during data acquisition, lower limit.degpos.emergenceAng;stat.mindoublenullableemergence_maxEmergence angle during data acquisition, upper limitdegpos.emergenceAng;stat.maxdoublenullablephase_minPhase angle during data acquisition, lower limit.degpos.phaseAng;stat.mindoublenullablephase_maxPhase angle during data acquisition, upper limitdegpos.phaseAng;stat.maxdoublenullableinstrument_host_nameStandard name of the observatory or spacecraftmeta.id;instr.obstycharnullableinstrument_nameStandard name of instrumentmeta.id;instrcharnullablemeasurement_typeUCD(s) defining the data, with multiple entries separated by hash (#) characters.meta.ucdcharnullableprocessing_levelDataset-related encoding, or simplified CODMAC calibration levelmeta.calibLevelintcreation_dateDate of first entry of this granuletime.creationcharnullablemodification_dateDate of last modification (used to handle mirroring)time.processingcharnullablerelease_dateStart of public access periodtime.releasecharnullableservice_titleTitle of resource (an acronym really, will be used to handle multiservice results)meta.titlecharnullablealt_target_nameProvides alternative target name if more common (e.g. comets); multiple identifiers can be separated by hashesmeta.id;srcunicodeCharnullablemagnitudeAbsolute Magnitude of the asteroid, i.e., the magnitude of the asteroid at a distance of 1 AU when viewed at a phase angle of 0°.magphys.magAbsfloatnullableslope_parameterSlope Parameter G. It describes how the magnitude of the asteroid varies as a function of changing illumination (phase angle)src.morph.paramfloatnullableorb_epochEpoch of the orbit (julian years)yrtime.epochdoublenullablemean_anomalyMean anomaly at the epochdegsrc.orbital.meanAnomalyfloatnullablearg_perihelArgument of Perihelion, J2000.0degsrc.orbital.periastronfloatnullablelong_ascLongitude of ascending node, J2000.0degsrc.orbital.nodefloatnullableinclinationInclination of the orbit to the ecliptic, J2000.0degsrc.orbital.inclinationfloatnullableeccentricityEccentricity of the orbitsrc.orbital.eccentricityfloatnullablemean_motionMean Daily Motiondeg/dpos.pm;arith.diff;phys.velocfloatnullablesemi_major_axisOrbital semimajor axisAUphys.size.smajAxisfloatnullableuncertainty_parameterQuality code (0 is best) as per http://www.minorplanetcenter.org/iau/info/UValue.html. Or: E -- the orbital eccentricity was assumed; D -- for one-opposition orbits this means a double (or multiple) designation is involved; F -- an e-assumed double (or multiple) designation is involved.meta.code.errorcharnullablen_obsNumber of Observationsmeta.number;obsintnullablen_oppNumber of Oppositionsmeta.numberintarc_lengthLength of observed arcs for single-opposition orbits.dtime.intervalshortnullablerms_fitRMS Residual of orbital fitarcsecstat.fit.residualfloatnullableperturbersInformation on orbit perturbers; see table note.meta.notecharnullablecomputerIdentifies the computer of the orbitmeta.notecharnullableorbit_classOrbit family this object belongs to (note that the classification is based on cuts in osculating element space and is not 100% reliable.src.classcharnullableorbit_flagsAdditional classification flag(s) as comma-separated human-readable phrasessrc.classcharnullablefirst_obsDiscovery year for multi-opposition orbits.yrtime.epochshortnullablelast_obsDate of last observationyrtime.epoch;obsfloatnullablebib_referenceOrigin of the datameta.bibcharnullablempc.mpcorb Complete Asteroid Data from the Minor Planet Center (MPC), updated once per month. The MPC operates at the Smithsonian Astrophysical Observatory under the auspices of Division III of the International Astronomical Union (IAU); for the upstream data, see https://www.minorplanetcenter.net/data. The MPC Orbit database contains orbital elements of minor planets that have been published in the Minor Planet Circulars, the Minor Planet Orbit Supplement and the Minor Planet Electronic Circulars.1200000designationAsteroid number or provisional designation.meta.id;meta.maincharnullablemagAbsolute Magnitude of the asteroid, i.e., the magnitude of the asteroid at a distance of 1 AU when viewed at a phase angle of 0°.magphys.magAbsfloatindexednullableslopeSlope Parameter G. It describes how the magnitude of the asteroid varies as a function of changing illumination (phase angle)src.morph.paramfloatnullableorb_epochEpoch of the orbit (julian years)yrtime.epochdoublenullablemean_anomalyMean anomaly at the epochdegsrc.orbital.meanAnomalyfloatnullablearg_perihelArgument of Perihelion, J2000.0degsrc.orbital.periastronfloatnullablelong_ascLongitude of ascending node, J2000.0degsrc.orbital.nodefloatnullableinclinationInclination of the orbit to the ecliptic, J2000.0degsrc.orbital.inclinationfloatnullableeccentricityEccentricity of the orbitsrc.orbital.eccentricityfloatnullablemean_motionMean Daily Motiondeg/dpos.pm;arith.diff;phys.velocfloatnullablesemimaj_axOrbital semimajor axisAUphys.size.smajAxisfloatindexednullableuncertainty_parameterQuality code (0 is best) as per http://www.minorplanetcenter.org/iau/info/UValue.html. Or: E -- the orbital eccentricity was assumed; D -- for one-opposition orbits this means a double (or multiple) designation is involved; F -- an e-assumed double (or multiple) designation is involved.meta.code.errorcharnullablebib_referenceOrigin of the datameta.bibcharnullablen_obsNumber of Observationsmeta.number;obsintnullablen_oppNumber of Oppositionsmeta.numberintarc_lengthLength of observed arcs for single-opposition orbits.dtime.intervalshortnullablefirst_obsDiscovery year for multi-opposition orbits.yrtime.epochshortnullablerms_fitRMS Residual of orbital fitarcsecstat.fit.residualfloatnullableperturbersInformation on orbit perturbers; see table note.meta.notecharnullablecomputerIdentifies the computer of the orbitmeta.notecharnullableorbit_classOrbit family this object belongs to (note that the classification is based on cuts in osculating element space and is not 100% reliable.src.classcharnullableorbit_flagsAdditional classification flag(s) as comma-separated human-readable phrasessrc.classcharnullablenameHuman-readable designation of the Asteroid.meta.idunicodeCharindexednullablelast_obsDate of last observationyrtime.epoch;obsfloatnullableusnobThe USNO-B catalog is an all-sky catalog of about 1e9 objects including their proper motions, based on scans of several sky surveys conducted between 1950 and the late 1990ies.usnob.dataThe USNO-B 1.0 catalogue with Barron's spurious detections removed.1100000000raj2000Right Ascension at Eq=J2000, Ep=J2000degpos.eq.ra;meta.main019.9241238.043341.1753601doubleindexednullabledej2000Declination at Eq=J2000, Ep=J2000degpos.eq.dec;meta.main-89.9516-70.6605-15.760565.048589.93931doubleindexednullablee_radegMean error on RAdeg*cos(DEdeg) at Epochdegstat.error;pos.eq.ra05.27778e-063.69444e-050.00027750.00027751floatnullablee_dedegMean error on DEdeg at Epochdegstat.error;pos.eq.dec05.27778e-063.63889e-050.00027750.00027751floatnullableepochMean epoch of observationyrtime.epoch19501966.51980.719932049.91floatnullablepmraProper motion in RAdeg/yrpos.pm;pos.eq.ra-0.00272167-2.22222e-0501.72222e-050.002678331floatnullablepmdeProper motion in DEdeg/yrpos.pm;pos.eq.dec-0.002555-2.16667e-0502.16667e-050.002729441floatnullablemuprTotal Proper Motion probabilitystat.fit.goodness0000.90.91floatnullablee_pmraMean error on pmRAdeg/yrstat.error;pos.pm;pos.eq.ra2.77778e-072.77778e-071.66667e-063.27778e-050.00027750.264193floatnullablee_pmdeMean error on pmDEdeg/yrstat.error;pos.pm;pos.eq.dec2.77778e-072.77778e-071.66667e-063.52778e-050.00027750.261385floatnullablefit_raMean error on RA fitdegstat.error2.77778e-052.77778e-055.55556e-050.000250.000250.800957floatnullablefit_deMean error on DE fitdegstat.error2.77778e-052.77778e-055.55556e-050.000250.000250.792568floatnullablendetNumber of detectionsmeta.number02.04.05.051.0shortflagsFlags on objectmeta.codecharnullableb1magFirst blue magnitude (B1)magphot.mag;em.opt.B0.3114.9819.4821.0684.950.360581floatnullableb1sB1 Survey codemeta.idABCDcharindexednullableb1fB1 Field number in surveymeta.id;obs.field150.0496.0922.09370.3580957shortindexednullableb1sgB1 Star/galaxy separation, A=Galaxy, L=Starsrc.class.starGalaxycharnullableb1xiB1 Residual in X directiondegstat.fit.residual;pos.cartesian.x0000.0002833330.003744440.358096floatnullableb1etaB1 Residual in Y directiondegstat.fit.residual;pos.eq.dec;arith.diff0000.0003055560.003461110.358096floatnullabler1magFirst red magnitude (R1)magphot.mag;em.opt.R0.1213.8317.9820.1850.738815floatnullabler1sR1 Survey codemeta.idABCDcharindexednullabler1fR1 Field number in surveymeta.id;obs.field139.0335.0919.09370.7363305shortindexednullabler1sgR1 Star/galaxy separation, A=Galaxy, L=Starsrc.class.starGalaxycharnullabler1xiR1 Residual in X directiondegstat.fit.residual;pos.cartesian.x0000.0002083330.003388890.73633floatnullabler1etaR1 Residual in Y directiondegstat.fit.residual;pos.eq.dec;arith.diff0000.0002138890.003577780.73633floatnullableb2magSecond blue magnitude (B2)magphot.mag;em.opt.B0.0415.1419.3121.65850.820628floatnullableb2sB2 Survey codemeta.idcharindexednullableb2fB2 Field number in surveymeta.id;obs.field144.0389.0819.08980.81814367shortindexednullableb2sgB2 Star/galaxy separation, A=Galaxy, L=Starsrc.class.starGalaxycharnullableb2xiB2 Residual in X directiondegstat.fit.residual;pos.cartesian.x0000.0002833330.003216670.818144floatnullableb2etaB2 Residual in Y directiondegstat.fit.residual;pos.eq.dec;arith.diff0000.0003027780.003655560.818144floatnullabler2magSecond red magnitude (R2)magphot.mag;em.opt.R0.1314.0718.3920.9850.877989floatnullabler2sR2 Survey codemeta.idcharindexednullabler2fR2 Field number in surveymeta.id;obs.field145.0393.0825.08980.87550414shortindexednullabler2sgR2 Star/galaxy separation, A=Galaxy, L=Starsrc.class.starGalaxycharnullabler2xiR2 Residual in X directiondegstat.fit.residual;pos.cartesian.x0000.0002555560.003102780.875504floatnullabler2etaR2 Residual in Y directiondegstat.fit.residual;pos.eq.dec;arith.diff0000.0002722220.003677780.875504floatnullableimagInfrared (N) magnitudemagphot.mag;em.opt.I0.2113.0717.3519.03850.714414floatnullablei_sI Survey codemeta.idcharindexednullableifI Field number in surveymeta.id;obs.field245.0394.0842.08980.7119295shortindexednullableisgI Star/galaxy separation, A=Galaxy, L=Starsrc.class.starGalaxycharnullableixiI Residual in X directiondegstat.fit.residual;pos.cartesian.x0000.0002777780.0033750.711929floatnullableietaI Residual in Y directiondegstat.fit.residual;pos.eq.dec;arith.diff0000.0002888890.003352780.711929floatnullableusnob.platecorrsPlate corrections to USNO-B 1.0 based on a crossmatch with PPMX7194surveySurvey identifier, see long docsmeta.idABCDEFGHIXcharfieldField number in surveymeta.id;obs.field127.620000000000005444.0887.010371.0shortdaMean offset in alphadegpos.eq.ra;arith.diff-0.000539976-5.11083e-052.10587e-050.0001243080.001875260.999861floatnullableddMean offset in deltadegpos.eq.dec;arith.diff-0.00015169-7.26503e-05-2.59859e-054.66571e-050.0001638260.999861floatnullablentotalNumber of objects in estimatemeta.number0489.789999999999961504.07343.26163241.0intusnob.platesPlate data for the source plates of USNO-B8855fieldField number in surveymeta.id;obs.field127.620000000000005444.0887.010371.0shortplatePlate number in USNO-Bmeta.id;obs.field;meta.maincharnullablesurveySurvey identifier, see long docsmeta.idABCDEFGHIXcharindexedepochPlate epochyrtime.epochcharnullableemulsionEmulsioninstr.plate.emulsioncharnullablefilterFiltermeta.id;instr.filtercharnullableexposureLength of exposurestime.duration;obs.exposure018036007200108001floatnullableusnocode2-char plate code given in the plate cataloguemeta.id;obs.fieldcharnullablealpha1950Field center alpha for B1950degpos.eq.ra010180.0193503601floatnullabledelta1950Field center decl for B1950degpos.eq.dec-90-704.9988372.5289901floatnullablealpha2000Field center alpha for J2000degpos.eq.ra;meta.main0.3240657.67832178.887347.166359.1681floatindexednullabledelta2000Field center decl for J2000degpos.eq.dec;meta.main-89.7216-69.86984.7640972.729189.79961floatindexednullablesrcSource file for this recordmeta.ref;meta.filecharnullablealphamin1950degpos.eq.ra;stat.min010.3554180.896349.726358.7060.895765floatnullablealphamax1950degpos.eq.ra;stat.max0.253829.25548179.785349.4693600.895765floatnullabledeltamin1950degpos.eq.dec;stat.min-90-68.38396.7120971.474185.29350.895765floatnullabledeltamax1950degpos.eq.dec;stat.max-86.1554-62.313413.048178.0648900.895765floatnullableusnob.ppmxcrossA crossmatch between USNO-B 1.0 and PPMX.18000000ipixq3c ipix value of USNO-B objectmeta.id8976072396271.758775736454438e+173.528987594054219e+186.566351331851216e+1869166012618704412511.0longindexedppmxidPPMX id of matching objectmeta.id;meta.maincharindexednullableusnob.spuriousSpurious detections in USNO-B 1.0 as established by Barron et al, 2008AJ....135..414B.18000000raRA of spurious detectiondegpos.eq.ra;meta.main0.00020555610.4049161.404351.0413601doubleindexednullabledecDec of spurious detectiondegpos.eq.dec;meta.main-89.8459-75.779-12.745972.37189.56631doubleindexednullableusnob.twomasscrossA crossmatch between USNO-B 1.0 and 2MASS.360000000ipixq3c ipix value of USNO-B objectmeta.id8976072396271.758775736454438e+173.528987594054219e+186.566351331851216e+1869166012618704412511.0longindexedtwomassid2MASS id of matching objectmeta.id;meta.maincharindexednullableapplause APPLAUSE DR3 contains images and metadata from 24 plate collections in Hamburg, Bamberg, Potsdam, Tautenburg and Tartu, a total of 101138 scans of 70276 photographic plates. The present table contains metadata records for singly exposed plates with astrometric solutions in APPLAUSE (about 44000). It is mainly intended as a basis for publishing suitable APPLAUSE plates in the Obscore schema through the TAP service in GAVO's Heidelberg Data Center. A TAP service with more complete metadata and, in particular, extracted sources, is available at https://www.plate-archive.org/tap.applause.mainA redux of the calibrated subset of APPLAUSE to the obscore schema, with constant columns removed.44370obs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.sizelongnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classcharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameterfloatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharindexednullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.valuefloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttimedoubleindexednullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptimedoubleindexednullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extentfloatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimitfloatindexednullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimitfloatindexednullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.namecharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.namecharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins1intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins2intnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriodfloatnullablepreviewURL for a preview of the imagemeta.ref.url;meta.previewcharnullableemulsionEmulsion of the original plate (from observatory log).instr.plate.emulsioncharnullablefilterFilter used (from observatory log).meta.id;instr.filter;meta.maincharnullableseriesPlate seriesmeta.idcharnullablearchive_idArchive identification number (see plate-archive.org for the key)meta.idintplate_numPlate number in archivemeta.record;instr.platecharnullablewfpdb_idPlate identification in the Wide-Field Plate Databasemeta.id.crosscharnullablecasa_lines This is a rendering of the `CASA Offline Splatalogue`_ in a draft LineTAP, mainly intended to enable verification of the standard. This is not recommended for production yet. In particular, many InChIs are known wrong, and we have skipped several hundred lines because we did have no InChIs for their species at all. .. _CASA Offline Splatalogue: https://safe.nrao.edu/wiki/bin/view/ALMA/CASA_Offline_Splat_listcasa_lines.line_tap This is a rendering of the `CASA Offline Splatalogue`_ in a draft LineTAP, mainly intended to enable verification of the standard. This is not recommended for production yet. In particular, many InChIs are known wrong, and we have skipped several hundred lines because we did have no InChIs for their species at all. .. _CASA Offline Splatalogue: https://safe.nrao.edu/wiki/bin/view/ALMA/CASA_Offline_Splat_listivo://ivoa.net/std/linetap#lines-1.0333480titleHuman-readable line designation.meta.idcharvacuum_wavelengthVacuum wavelength of the transitionAngstromem.wldoublevacuum_wavelength_errorTotal error in vacuum_wavelengthAngstromstat.error;em.wldoublenullablemethodMethod the wavelength was obtained with (XSAMS controlled vocabulary)meta.code.classobservedtheoryritzcharnullableelementElement name for atomic transitions, NULL otherwise.phys.atmol.elementcharnullableion_chargeTotal charge (ionisation level) of the emitting particle.phys.electChargeintmass_numberNumber of nucleons in the atom or moleculephys.atmol.weightintnullableupper_energyEnergy of the upper stateJphys.energy;phys.atmol.initialdoublenullablelower_energyEnergy of the lower stateJphys.energy;phys.atmol.finaldoublenullableinchiInternational Chemical Identifier InChI.meta.id;phys.atmol;meta.maincharinchikeyThe InChi key (hash) generated from inchi.meta.id;phys.atmolchareinstein_aEinstein A coefficient of the radiative transition.phys.atmol.transProbdoublenullablexsams_uriA URI for a full XSAMS description of this line.meta.refcharnullableline_referenceReference to the source of the line data; this could be a bibcode, a DOI, or a plain URI.meta.refcharnrao_formulaChemical formula in NRAO's argot.meta.id;phys.molcharnullablecommon_nameCommon name of the molecule.meta.id;phys.molcharnullablequantnrResolved Quantum Number as per http://www.cv.nrao.edu/php/splat/QuantumCode.htmlphys.atmol.configurationcharnullabledipole_momentMolecule dipole moment Sij μ²Dfloatnullableglots The global TAP schema collects information on tables and columns from known TAP servers. This facilitates locating queriable data by physics (via UCD) or keywords (via description). Note that this shouldn't really be necessary as all information present here should be exposed through Registry records. However, in reality data providers currently are much more liable to give column metadata in their tap_schema than in their Registry records. Hence, for the time being, we maintain this service by harvesting tap_schemas about monthly.glots.columnsA table of columns within the tables listed in glots.tables.ivoidIVOA identifier of providing servicecharindexedprimarytable_nameFully qualified table namecharindexedprimarycolumn_nameColumn namecharindexedprimarydescriptionBrief description of columncharindexednullableunitUnit in VO standard formatcharnullableucdUCD of column (some services still have 1.0 UCDs).charindexednullableutypeUtype of columncharnullabledatatypeADQL datatypecharnullable"size"Length of variable length datatypesintnullableprincipalIs column principal?charnullableindexedIs there an index on this column?intnullablestdIs this a standard column?charnullableglots.tablesivoidivoidtable_nametable_nameglots.servicesA table of TAP services harvested from the registry (and some spoon-fed).ivoidIVOA identifier of providing servicecharindexedprimaryaccessurlBase URL of TAP endpointcharnullablenextharvestNext scheduled harvest of datacharnullableharvestintervalApproximate interval of harvestdintnullablelastsuccessLast successful harvest of this servicecharnullableglots.tablesA table of tables accesible through the TAP services known to glots.services.ivoidIVOA identifier of providing servicecharindexedprimarytable_nameFully qualified table namecharindexedprimarytable_descBrief description of the tableunicodeCharindexednullableutypeutype if the table corresponds to a data modelcharnullableglots.servicesivoidivoidobscode List of Observatory Codes assigned by the Minor Planet Center (MPC). The codes are used in cataloguing astrometric observations of small bodies in the solar system. A code is unique for a certain location and consists of three digits or one letter and two digits. In this representation, we give the observatory code, the geocentric coordinates, and the observatory designation.obscode.data List of Observatory Codes assigned by the Minor Planet Center (MPC). The codes are used in cataloguing astrometric observations of small bodies in the solar system. A code is unique for a certain location and consists of three digits or one letter and two digits. In this representation, we give the observatory code, the geocentric coordinates, and the observatory designation.2280codeObservatory Code assigned by the Minor Planet Centermeta.idcharnullablelongLongitude of the observatorydegpos.earth.lonfloatnullablecosphipParallax constant, cosinefloatnullablesinphipParallax constant, sinefloatnullablegclatGeocentric latitude of the observatorydegpos.earth.lat;pos.geocentricfloatnullablegdlatGeodetic latitude of the observatory WGS84degpos.earth.lat;pos.geocentricfloatnullableheightAltitude of the observatorympos.earth.altitudefloatnullablenameOperator-chosen designation of the Observatorymeta.id;meta.maincharnullablerr Tables containing the information in the IVOA Registry. To query these tables, use `our TAP service`_. For more information and example queries, see the `RegTAP specification`_. .. _our TAP service: /__system__/tap/run/info .. _RegTAP specification: http://www.ivoa.net/documents/RegTAP/ivo://ivoa.net/std/regtap#1.2rr.resource The resources (like services, data collections, organizations) present in this registry.xpath:/24138ivoidUnambiguous reference to the resource conforming to the IVOA standard for identifiers.xpath:identifiercharindexedprimaryres_typeResource type (something like vg:authority, vs:catalogservice, etc).xpath:@xsi:typecharnullablecreatedThe UTC date and time this resource metadata description was created.xpath:@createdcharnullableshort_nameA short name or abbreviation given to something, for presentation in space-constrained fields (up to 16 characters).xpath:shortNamecharindexednullableres_titleThe full name given to the resource.xpath:titleunicodeCharindexednullableupdatedThe UTC date this resource metadata description was last updated.xpath:@updatedcharnullablecontent_levelA hash-separated list of content levels specifying the intended audience.xpath:content/contentLevelcharnullableres_descriptionAn account of the nature of the resource.xpath:content/descriptionunicodeCharindexednullablereference_urlURL pointing to a human-readable document describing this resource.xpath:content/referenceURLcharnullablecreator_seqThe creator(s) of the resource in the order given by the resource record author, separated by semicolons.xpath:curation/creator/nameunicodeCharindexednullablecontent_typeA hash-separated list of natures or genres of the content of the resource.xpath:content/typecharnullablesource_formatThe format of source_value. This, in particular, can be ``bibcode''.xpath:content/source/@formatcharnullablesource_valueA bibliographic reference from which the present resource is derived or extracted.xpath:content/sourceunicodeCharnullableres_versionLabel associated with creation or availablilty of a version of a resource.xpath:curation/versioncharnullableregion_of_regardA single numeric value representing the angle, given in decimal degrees, by which a positional query against this resource should be ``blurred'' in order to get an appropriate match.degxpath:coverage/regionOfRegardfloatnullablewavebandA hash-separated list of regions of the electro-magnetic spectrum that the resource's spectral coverage overlaps with.xpath:coverage/wavebandcharnullablerightsA statement of usage conditions (license, attribution, embargo, etc).xpath:/rightscharnullablerights_uriA URI identifying a license the data is made available under.xpath:/rights/@rightsURIcharnullableharvested_fromIVOID of the registry this record came from.charnullablerr.registriesharvested_fromivoidrr.capability Pieces of behaviour of a resource.xpath:/capability/95817ivoidThe parent resource.xpath:/identifiercharindexedprimarycap_indexAn arbitrary identifier of this capability within the resource.shortindexedprimarycap_typeThe type of capability covered here. If looking for endpoints implementing a certain standard, you should not use this column but rather match against standard_id.xpath:@xsi:typecharnullablecap_descriptionA human-readable description of what this capability provides as part of the over-all service.xpath:descriptionunicodeCharnullablestandard_idA URI for a standard this capability conforms to.xpath:@standardIDcharnullablerr.resourceivoidivoidrr.tap_table TAP-queriable tables.ivo://ivoa.net/std/regtap#1.2residIVOA identifier of the resource this table was taken from (where there is a dedicated resource containing this table in its tableset, that resource is preferred over a TAP service).charindexednullablesvcidIVOA identifier of the TAP service making this table queriable.charindexednullabletable_nameThe fully qualified name of the table. As per VODataService, this includes all catalog or schema prefixes needed to distinguish it in a query, and it comes with SQL delimiters where necessary.xpath:namecharindexednullabletable_titleA descriptive, human-interpretable name for the table.xpath:titleunicodeCharindexednullabletable_descriptionA free-text description of the table's contents.xpath:descriptionunicodeCharindexednullabletable_utypeAn identifier for a concept in a data model that the data in this table as a whole represent.xpath:utypecharnullablerr.stc_spatial The spatial coverage of resources. This table associates footprints (ADQL geometries) with ivoids. The footprints are intended for resource discovery; a reasonable expectation for the resolution thus is something like a degree.xpath:/coverage/spatial16828ivoidThe parent resource.xpath:/identifiercharindexednullablecoverageA geometry representing the area a resource contains data for; this should be tight at least with a resolution of degrees.posxpath:.charnullableref_system_nameThe reference frame coverage is written in. This is currently reserved and fixed to NULL. Clients should always add a constraint to NULL for this to avoid matching non-celestial resources later.pos.framexpath:@framecharnullablerr.resourceivoidivoidrr.stc_spectral The spectral coverage of resources, given as one or more intervals. The total coverage is (a subset of) the union of all intervals given for a resource. The spectral values are given as messenger energy.xpath:/coverage/spectral89ivoidThe parent resource.xpath:/identifiercharindexednullablespectral_startLower limit (in Joules) of messenger energy interval covered by the resource (for the solar system barycenter).Jxpath:.floatspectral_endUpper limit (in Joules) of messenger energy interval covered by the resource (for the solar system barycenter).Jxpath:.floatrr.resourceivoidivoidrr.stc_temporal The temporal coverage of resources, given as one or more intervals. The total coverage is (a subset of) the union of all intervals given for a resource. All times are understood as MJD for TDB at the solar system barycenter.xpath:/coverage/temporal104ivoidThe parent resource.xpath:/identifiercharindexednullabletime_startLower limit of a time interval covered by the resource in MJD.dxpath:.floattime_endUpper limit of a time interval covered by the resource in MJD.dxpath:.floatrr.resourceivoidivoidrr.alt_identifier An alternate identifier associated with this record. This can be a resiource identifier like a DOI (in URI form, e.g., doi:10.1016/j.epsl.2011.11.037).xpath:/(curation/creator/|)altIdentifier63ivoidThe parent resource.xpath:/identifiercharindexednullablealt_identifierAn identifier for the resource or an entity related to the resource in URI form.charindexednullablerr.resourceivoidivoidrr.authorities A mapping between the registries and the authorities they claim to manage.ivo://ivoa.net/std/regtap#1.2142ivoidIVOID of the registry.charnullablemanaged_authorityAn authority this registry claims to serve.charindexedprimaryrr.registriesivoidivoidrr.g_num_stat An experimental table containing advanced statistics for numeric table columns. This is only available for very few tables at this point. Note that the values reported here may be estimates based on a subeset of the table rows.ivo://ivoa.net/std/regtap#1.21052ivoidThe parent resource.xpath:/identifiercharnullabletable_indexIndex of the table this column belongs to.shortnameName of the column (see rr.table_column for more metadata).charindexednullablefill_factorAn estimate for the ratio of non-NULL values in this column to the number of rows in the table.floatnullablemin_valueThe largest value found in the column.floatnullablepercentile03An estimate for the value in the 3rd percentile of the column's distribution (for a Gaussian, roughly the lower limit of a 2σ interval).floatindexednullablemedianAn estimate for the median value (or 50th percentile) of the column's distributionfloatindexednullablepercentile97An estimate for the value in the 97th percentile of the column's distribution (for a Gaussian, roughly the upper limit of a 2σ interval).floatindexednullablemax_valueThe largest value found in the column.floatnullablerr.res_tableivoidivoidtable_indextable_indexrr.interface Information on access modes of a capability.xpath:/capability/interface/95935ivoidThe parent resource.xpath:/identifiercharindexedprimarycap_indexThe index of the parent capability.shortindexedintf_indexAn arbitrary identifier for the interfaces of a resource.shortindexedprimaryintf_typeThe type of the interface (vr:webbrowser, vs:paramhttp, etc).xpath:@xsi:typecharnullableintf_roleAn identifier for the role the interface plays in the particular capability. If the value is equal to "std" or begins with "std:", then the interface refers to a standard interface defined by the standard referred to by the capability's standardID attribute.xpath:@rolecharnullablestd_versionThe version of a standard interface specification that this interface complies with. When the interface is provided in the context of a Capability element, then the standard being refered to is the one identified by the Capability's standardID element.xpath:@versioncharnullablequery_typeHash-joined list of expected HTTP method (get or post) supported by the service.xpath:queryTypecharnullableresult_typeThe MIME type of a document returned in the HTTP response.xpath:resultTypecharnullablewsdl_urlThe location of the WSDL that describes this Web Service. If NULL, the location can be assumed to be the accessURL with '?wsdl' appended.xpath:wsdlURLcharnullableurl_useA flag indicating whether this should be interpreted as a base URL ('base'), a full URL ('full'), or a URL to a directory that will produce a listing of files ('dir').xpath:accessURL/@usecharnullableaccess_urlThe URL at which the interface is found.xpath:accessURLcharnullablemirror_urlSecondary access URLs of this interface, separated by hash characters.xpath:mirrorURLcharnullableauthenticated_onlyA flag for whether an interface is available for anonymous use (=0) or only authenticated clients are served (=1).shortsecurity_method_idThis column was mentioned in drafts of RegTAP 1.1 but was abandoned before RegTAP 1.1 REC. Do not use any more. This is just here to avoid a flag day for clients that experimentally used this column. This is always NULL here.not mappedcharnullablerr.capabilityivoidivoidcap_indexcap_indexrr.intf_param Input parameters for services.xpath:/capability/interface/param/3178ivoidThe parent resource.xpath:/identifiercharindexednullableintf_indexThe index of the interface this parameter belongs to.shortnameThe name of the parameter.xpath:namecharnullableucdA unified content descriptor that describes the scientific content of the parameter.xpath:ucdcharnullableunitThe unit associated with all values in the parameter.xpath:unitcharnullableutypeAn identifier for a role in a data model that the data in this parameter represents.xpath:utypecharnullablestdIf 1, the meaning and use of this parameter is reserved and defined by a standard model. If 0, it represents a database-specific parameter that effectively extends beyond the standard.xpath:@stdshortnullabledatatypeThe type of the data contained in the parameter.xpath:dataTypecharnullableextended_schemaAn identifier for the schema that the value given by the extended attribute is drawn from.xpath:dataType/@extendedSchemacharnullableextended_typeA custom type for the values this parameter contains.xpath:dataType/@extendedTypecharnullablearraysizeThe shape of the array that constitutes the value, e.g., 4, *, 4*, 5x4, or 5x*, as specified by VOTable.xpath:dataType/@arraysizecharnullabledelimThe string that is used to delimit elements of an array value when arraysize is not '1'.xpath:dataType/@delimcharnullableparam_useAn indication of whether this parameter is required to be provided for the application or service to work properly (one of required, optional, ignored, or NULL).xpath:@usecharnullableparam_descriptionA free-text description of the parameter's contents.xpath:descriptionunicodeCharnullablerr.interfaceivoidivoidintf_indexintf_indexrr.registries Administrative table: publishing registries we harvest, together with the dates of last full and incremental harvests.ivo://ivoa.net/std/regtap#1.253ivoidIVOID of the registry.charindexedprimaryaccessurlURL of the registry's OAI-PMH endpoint.charnullabletitleName of the registry.unicodeCharnullablelast_full_harvestDate and time of the last full harvest of the registry.charnullablelast_inc_harvestDate and time of the last incremental harvest of the registry.charnullablerr.relationship Relationships between resources (like mirroring, derivation, serving a data collection).xpath:/content/relationship/23702ivoidThe parent resource.xpath:/identifiercharindexednullablerelationship_typeThe type of the relationship; these terms are drawn from a controlled vocabulary and are DataCite-compatible.xpath:relationshipTypecharnullablerelated_idThe IVOA identifier for the resource referred to.xpath:relatedResource/@ivo-idcharnullablerelated_nameThe name of resource that this resource is related to.xpath:relatedResourcecharnullablerelated_alt_identifierA non-IVOA identifier for the related resource. This will typically be a DOI in URI form ('doi:10...')xpath:relatedResource/@altIdentifiercharnullablerr.resourceivoidivoidrr.res_date A date associated with an event in the life cycle of the resource. This could be creation or update. The role column can be used to clarify.xpath:/curation/23363ivoidThe parent resource.xpath:/identifiercharindexednullabledate_valueA date associated with an event in the life cycle of the resource.xpath:datecharnullablevalue_roleA string indicating what the date refers to, e.g., created, availability, updated. This value is generally drawn from a controlled vocabulary.xpath:date/@rolecharnullablerr.resourceivoidivoidrr.res_detail XPath-value pairs for members of resource or capability and their derivations that are less used and/or from VOResource extensions. The pairs refer to a resource if cap_index is NULL, to the referenced capability otherwise.ivo://ivoa.net/std/regtap#1.2215590ivoidThe parent resource.xpath:/identifiercharindexednullablecap_indexThe index of the parent capability; if NULL the xpath-value pair describes a member of the entire resource.shortnullabledetail_xpathThe xpath of the data item.charnullabledetail_value(Atomic) value of the member.unicodeCharnullablerr.resourceivoidivoidrr.res_role Entities (persons or organizations) operating on resources: creators, contacts, publishers, contributors.ivo://ivoa.net/std/regtap#1.295827ivoidThe parent resource.xpath:/identifiercharindexednullablerole_nameThe real-world name or title of a person or organization.unicodeCharindexednullablerole_ivoidAn IVOA identifier of a person or organization.charnullablestreet_addressA mailing address for a person or organization.unicodeCharnullableemailAn email address the entity can be reached at.charnullabletelephoneA telephone number the entity can be reached at.charnullablelogoURL pointing to a graphical logo, which may be used to help identify the entity.charnullablebase_roleThe role played by this entity; this is one of contact, publisher, contributor, or creator.charindexednullablealt_identifierA non-IVOA identifier for the entity, for instance an ORCID or a ROR id. See the RegTAP document for the notations for the various identifier types.charindexednullablerr.resourceivoidivoidrr.res_schema Sets of tables related to resources.xpath:/tableset/schema/2137ivoidThe parent resource.xpath:/identifiercharindexedprimaryschema_indexAn arbitrary identifier for the res_schema rows belonging to a resource.shortindexedprimaryschema_descriptionA free text description of the tableset explaining in general how all of the tables are related.xpath:descriptionunicodeCharnullableschema_nameA name for the set of tables.xpath:name charnullableschema_titleA descriptive, human-interpretable name for the table set.xpath:titleunicodeCharnullableschema_utypeAn identifier for a concept in a data model that the data in this schema as a whole represent.xpath:utypecharnullablerr.resourceivoidivoidrr.res_subject Topics, object types, or other descriptive keywords about the resource.xpath:/content/55057ivoidThe parent resource.xpath:/identifiercharindexednullableres_subjectTopics, object types, or other descriptive keywords about the resource.xpath:subjectcharindexednullablerr.resourceivoidivoidrr.res_table (Relational) tables that are part of schemata or resources.xpath:/(tableset/schema/|)table/60176ivoidThe parent resource.xpath:/identifiercharindexedprimaryschema_indexIndex of the schema this table belongs to, if it belongs to a schema (otherwise NULL).shortnullabletable_descriptionA free-text description of the table's contents.xpath:descriptionunicodeCharnullabletable_nameThe fully qualified name of the table. As per VODataService, this includes all catalog or schema prefixes needed to distinguish it in a query, and it comes with SQL delimiters where necessary.xpath:namecharnullabletable_indexAn arbitrary identifier for the tables belonging to a resource.shortindexedprimarytable_titleA descriptive, human-interpretable name for the table.xpath:titleunicodeCharnullabletable_typeA name for the role this table plays. Recognized values include "output", indicating this table is output from a query; "base_table", indicating a table whose records represent the main subjects of its schema; and "view", indicating that the table represents a useful combination or subset of other tables. Other values are allowed.xpath:@typecharnullabletable_utypeAn identifier for a concept in a data model that the data in this table as a whole represent.xpath:utypecharnullablenrowsAn estimate for the number of rows in the table.xpath:nrowslongnullablerr.resourceivoidivoidrr.subject_uat res_subject mapped to the UAT. This is based on a manual mapping of keywords found in 2020, where subjects not mappable were dropped. This is a non-standard, local extension. Don't base your procedures on it, we will tear it down once there is sufficient takeup of the UAT in the VO.ivo://ivoa.net/std/regtap#1.251571ivoidThe parent resource.xpath:/identifiercharindexednullableuat_conceptTerm from http://www.ivoa.net/rdf/uat; most of these resulted from mapping non-UAT designations.charindexednullablerr.resourceivoidivoidrr.table_column Metadata on columns of a resource's tables.xpath:/(tableset/schema/|)/table/column/1300000ivoidThe parent resource.xpath:/identifiercharindexednullabletable_indexIndex of the table this column belongs to.shortnameThe name of the column.xpath:namecharindexednullableucdA unified content descriptor that describes the scientific content of the column.xpath:ucdcharindexednullableunitThe unit associated with all values in the column.xpath:unitcharnullableutypeAn identifier for a role in a data model that the data in this column represents.xpath:utypecharnullablestdIf 1, the meaning and use of this column is reserved and defined by a standard model. If 0, it represents a database-specific column that effectively extends beyond the standard.xpath:@stdshortnullabledatatypeThe type of the data contained in the column.xpath:dataTypecharnullableextended_schemaAn identifier for the schema that the value given by the extended attribute is drawn from.xpath:dataType/@extendedSchemacharnullableextended_typeA custom type for the values this column contains.xpath:dataType/@extendedTypecharnullablearraysizeThe shape of the array that constitutes the value, e.g., 4, *, 4*, 5x4, or 5x*, as specified by VOTable.xpath:dataType/@arraysizecharnullabledelimThe string that is used to delimit elements of an array value when arraysize is not '1'.xpath:dataType/@delimcharnullabletype_systemThe type system used, as a QName with a canonical prefix; this will ususally be one of vs:simpledatatype, vs:votabletype, and vs:taptype.xpath:dataType/@xsi:typecharnullableflagHash-separated keywords representing traits of the column. Recognized values include "indexed", "primary", and "nullable".xpath:flagcharnullablecolumn_descriptionA free-text description of the column's contents.xpath:descriptionunicodeCharindexednullablerr.res_tableivoidivoidtable_indextable_indexrr.validationValidation levels for resources and capabilities.xpath:/(capability/|)validationLevel23685ivoidThe parent resource.xpath:/identifiercharindexednullablevalidated_byThe IVOA ID of the registry or organisation that assigned the validation level.xpath:validationLevel/@validatedBycharnullableval_levelA numeric grade describing the quality of the resource description, when applicable, to be used to indicate the confidence an end-user can put in the resource as part of a VO application or research study.xpath:validationLevelshortnullablecap_indexIf non-NULL, the validation only refers to the capability referenced here.shortnullablerr.resourceivoidivoidrr.resourceivoidivoidspecies A TAP-queriable database of common names of molecules and their InChIs. This is an experimental copy of http://species.vamdc.org created in the context of the LineTAP effort, augmented with names found in the CASA line list. You will probably want to query this using SQL wildcards (% and _) and the ILIKE operator.species.main A TAP-queriable database of common names of molecules and their InChIs. This is an experimental copy of http://species.vamdc.org created in the context of the LineTAP effort, augmented with names found in the CASA line list. You will probably want to query this using SQL wildcards (% and _) and the ILIKE operator.ivo://ivoa.net/std/linetap#species-1.0inchikeyInChIKey of this speciescharindexednullableinchiInChI of this speciescharnullablenameA common name of this speciesunicodeCharindexednullableformulaChemical formula of this species in some free-ish notationcharindexednullablesource_idVAMDC identifier of the origin of this mappingcharnullableamandaA list of neutrino candidate events recorded by the AMANDA-II neutrino telescope during the period 2000-2006.amanda.nucand Detection parameters of neutrino candidates recorded by the AMANDA-II telescope. This table can be queried on the web at http://dc.g-vo.org/amanda/q/web6595idArtifical primary key.meta.id;meta.maincharindexedprimaryraj2000Neutrino arrival direction, RAdegpos.eq.ra;meta.main0.063312711.3906182.019350.228359.9831floatindexeddej2000Neutrino arrival direction, Declinationdegpos.eq.dec;meta.main-9.9621-4.2885436.23778.013188.96691floatindexednchNumber of optical modules hit in an eventmeta.number1322.034.090.02211.0shortang_errorAngular resolution of a neutrino eventdegpos.angResolution0.7119981.227542.192563.097355.825271floatmjdObservation time, Modified Julian Daydtime.epoch;obs51590.651665.452884.653995.754039.71floatatmonusubsetSubset of candidates used in AMANDA's seven-year atmospheric neutrino analysismeta.codebooleanorigin_estA circle around the most likely position with ang_error radius (for convenient matching).pos.outline;obs.fielddoublenullableannisred This survey gives photometric redshifts of objects within 275 deg² (−50◦ < α < 60◦ and −1.◦25 < δ < +1.◦25) centered on the Celestial Equator. Each piece of sky has ∼20 runs of repeated scanning by the SDSS camera contributing and thus reaches ∼2 mag fainter than the SDSS single pass data, i.e., to r ∼ 23.5 for galaxies.annisred.main This survey gives photometric redshifts of objects within 275 deg² (−50◦ < α < 60◦ and −1.◦25 < δ < +1.◦25) centered on the Celestial Equator. Each piece of sky has ∼20 runs of repeated scanning by the SDSS camera contributing and thus reaches ∼2 mag fainter than the SDSS single pass data, i.e., to r ∼ 23.5 for galaxies.14000000objidUnique SDSS identifier.meta.id;meta.main86474746903123067028.647474690332297e+188.647475119815855e+188.647475122523472e+1886474751227617642731.0longindexedrunRun numbermeta.id;obs106106.0206.0206.02061.0shortrerunRerun numbermeta.id;obs22.02.02.021.0shortcamcolCamera columnmeta.id;instr11.03.06.061.0shortfieldidField numbermeta.id;obs.field6287.0453.0771.08001.0longobjThe object id within a field. Usually changes between reruns of the same field.meta.id1145.01687.03270.050711.0shortraj2000Right ascension of the object.degpos.eq.ra;meta.main0.0001323573.1477650.1463356.6143601doubleindexednullabledej2000Declination of the object.degpos.eq.dec;meta.main-1.25848-1.1791-0.01587851.174321.258811doubleindexednullablezphotPhotometric redshift from SDSS' PHOTO pipeline00.2000670.7742111.0769621floatindexednullablezphoterrError in the photometric redshift from SDSS' PHOTO pipeline0.0057720.0276870.1962150.4449640.7000651floatnullableantares A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2012 by the ANTARES neutrino telescope. This dataset includes a total of 5921 events obtained during the effective livetime of 1338 days.antares.data A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2012 by the ANTARES neutrino telescope. This dataset includes a total of 5921 events obtained during the effective livetime of 1338 days.5921idIdentifier for this neutrino.meta.id;meta.maincharindexedprimaryraj2000Right Ascension, ICRSdegpos.eq.ra;meta.mainfloatnullabledej2000Declination, ICRSdegpos.eq.dec;meta.mainfloatnullablen_hitsNumber of signals from the photo multiplier tubes contributing to this observation.meta.number;obsshortang_error1 sigma confidence radius of the position.degstat.error;pos0.11floatindexednullableepoch_mjdArrival time in UTC TOPOCENTER.dtime.epoch54138.156292.6doublenullableorigin_estA circle around the most likely position with ang_error radius (for convenient matching).pos.outline;obs.fielddoubleindexednullableantares10 A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2010 by the ANTARES neutrino telescope. This dataset includes a total of 3058 events obtained during the effective livetime of 813 days. This is legacy data. The most recently released data can be found at ivo://org.gavo.dc/antares/q/cone.antares10.data A time integrated search for point sources of cosmic neutrinos was performed using the data collected from January 2007 to November 2010 by the ANTARES neutrino telescope. This dataset includes a total of 3058 events obtained during the effective livetime of 813 days. This is legacy data. The most recently released data can be found at ivo://org.gavo.dc/antares/q/cone.3092idIdentifier for this neutrino.meta.id;meta.maincharindexedprimaryraj2000Right Ascension, ICRSdegpos.eq.ra;meta.mainfloatnullabledej2000Declination, ICRSdegpos.eq.dec;meta.mainfloatnullablen_hitsNumber of signals from the photo multiplier tubes contributing to this observation.meta.number;obsshortang_error1 sigma confidence radius of the position.degstat.error;pos0.11floatindexednullableorigin_estA circle around the most likely position with ang_error radius (for convenient matching).meta.id;obs.fielddoublenullableapoObservations of the lensed quasar Q2237+0305 performed between 1995 and 1998.apo.framesObservations of the lensed quasar Q2237+0305 performed between 1995 and 1998.527accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullabletypecharnullableobjectcharnullableraw_objectcharnullablefilter1Filters on filter wheel 1charnullablefilter2Filters on filter wheel 2charnullableexposurefloatnullablealpharawRA of center of view 1950.0charnullabledeltarawDec of center of view 1950.0charnullablepub_didPublisher DID for this dataset.charnullablearihip The catalogue ARIHIP has been constructed by selecting the 'best data' for a given star from combinations of HIPPARCOS data with Boss' GC and/or the Tycho-2 catalogue as well as the FK6. It provides 'best data' for 90 842 stars with a typical mean error of 0.89 mas/year (about a factor of 1.3 better than Hipparcos for this sample of stars).arihip.main The catalogue ARIHIP has been constructed by selecting the 'best data' for a given star from combinations of HIPPARCOS data with Boss' GC and/or the Tycho-2 catalogue as well as the FK6. It provides 'best data' for 90 842 stars with a typical mean error of 0.89 mas/year (about a factor of 1.3 better than Hipparcos for this sample of stars).90842hipnoNumber of the star in the HIPPARCOS Catalogue (ESA 1997).meta.id;meta.main13488.6958948.5114865.771204041.0intindexedprimarysrcselSource of the astrometric solutionmeta.codecharnullableraj2000Right ascension from a single-star solutiondegpos.eq.ra;meta.main0.00090000811.1353181.28348.946359.9791doubleindexeddej2000Declination from a single-star solutiondegpos.eq.dec;meta.main-89.7824-70.7875-2.111869.099489.56941doubleindexedpmraProper motion in right ascension times cos(delta) for a single-star solution.deg/yrpos.pm;pos.eq.ra-0.000904975-3.31434e-05-4.38889e-073.23571e-050.00187971floatnullablepmdeProper motion in declination for a single-star solution.deg/yrpos.pm;pos.eq.dec-0.0016153-4.22579e-05-1.56389e-061.49154e-050.002868891floatnullablet_raCentral epoch of RA (SI)yrstat.error;time.epoch;pos.eq.ra1989.871990.951991.241991.561992.331floatnullableerr_raError in RA from the single star solution, with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.25e-074.83333e-074.84444e-061floatnullableerr_pmraMean error in PM(RA)*cos(delta) from the single star solutiondeg/yrstat.error;pos.pm;pos.eq.ra5.55556e-081.25e-072.19444e-074.13889e-079.37222e-061floatnullablet_deCentral epoch of Dec (SI)yrstat.error;time.epoch;pos.eq.dec1990.351990.851991.271991.661992.411floatnullableerr_deError in Dec from the single star solutiondegstat.error;pos.eq.dec8.33333e-081.19444e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdeMean error in PM(Dec) form the single star solutiondeg/yrstat.error;pos.pm;pos.eq.dec5e-081.22222e-071.97222e-073.63889e-077.35e-061floatnullableparallaxParallax used in deriving the data of the star in the catalogue selected for the ARIHIP. This is either the HIPPARCOS parallax or a photometric/spectroscopic parallax (see Kp).degpos.parallax-8.21667e-06-1.66667e-081.21944e-066.84444e-060.0001525031floatnullablee_parallaxMean error of the parallaxdegstat.error;pos.parallax1.11111e-081.61111e-072.94444e-075.97222e-075.77778e-061floatnullablekpSource of the parallax: H Hipparcos, P photometric parallaxmeta.ref;pos.parallaxcharnullablevradRadial velocity as used in calculating the foreshortening effect.km/sspect.dopplerVeloc;pos.heliocentric-409-61-2594710.17504floatnullablemvVisual magnitude taken from the HIPPARCOS cataloguemagphot.mag;em.opt.V-0.625.978.4710.7414.081floatindexednullablekmVariability flag. See note.meta.code;src.varcharnullablekbinBinarity flag. See note.meta.code.multipcharnullablekdmuBased on Delta mu, 1 is a single-star candidate, 2 is a Delta mu binary, and empty values mean uncertain casesmeta.code.multipcharnullablekaeMeasure of astrometric quality between 1 and 3, higher is better. Empty values mean the star is not 'astrometrically excellent'.meta.code.qualcharnullableraltpRight ascension in LTP modedegpos.eq.ra0.000900311.1353181.28348.946359.9791doublenullabledeltpDeclination in LTP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmraltpProper motion in RA, cos(delta) applied, in LTP modedeg/yrpos.pm;pos.eq.ra-0.000904736-3.30739e-05-4.41667e-073.23442e-050.001879961floatnullablepmdeltpProper motion in Dec in LTP modedeg/yrpos.pm;pos.eq.dec-0.00161528-4.225e-05-1.55972e-061.48494e-050.002869331floatnullablet_raltpCentral epoch of RA (LTP)yrstat.error;time.epoch;pos.eq.ra1957.051989.491991.241991.41992.271floatnullableerr_raltpError in RA (LTP) with cos(delta) already applieddegstat.error;pos.eq.ra9.16667e-084.22222e-072.22778e-064.30278e-065.15833e-061floatnullableerr_pmraltpMean error in PM(RA)*cos(delta) in LTP modedeg/yrstat.error;pos.pm;pos.eq.ra6.66667e-081.91667e-072.83333e-074.80556e-079.37222e-061floatnullablet_deltpCentral epoch of Dec (LTP)yrstat.error;time.epoch;pos.eq.dec1954.471989.631991.251991.431992.411floatnullableerr_deltpError in Dec (LTP)degstat.error;pos.eq.dec1e-073.52778e-072.225e-064.3e-065.12222e-061floatnullableerr_pmdeltpMean error in PM(Dec) in LTP modedeg/yrstat.error;pos.pm;pos.eq.dec5.83333e-081.86111e-072.77778e-074.52778e-077.36667e-061floatnullablerastpRight ascension in STP modedegpos.eq.ra0.00089966711.1353181.28348.946359.9791doublenullabledestpDeclination in STP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmrastpProper motion in RA, cos(delta) applied, in STP modedeg/yrpos.pm;pos.eq.ra-0.000905139-3.31299e-05-4.41667e-073.23487e-050.001879631floatnullablepmdestpProper motion in Dec in STP modedeg/yrpos.pm;pos.eq.dec-0.00161518-4.22632e-05-1.56389e-061.49139e-050.002868661floatnullablet_rastpCentral epoch of RA (STP)yrstat.error;time.epoch;pos.eq.ra1989.871990.931991.241991.581992.331floatnullableerr_rastpError in RA (STP) with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.27778e-074.83333e-074.84444e-061floatnullableerr_pmrastpMean error in PM(RA)*cos(delta) in STP modedeg/yrstat.error;pos.pm;pos.eq.ra8.33333e-081.33333e-072.47222e-074.75e-079.37222e-061floatnullablet_destpCentral epoch of Dec (STP)yrstat.error;time.epoch;pos.eq.dec1990.351990.831991.271991.681992.411floatnullableerr_destpError in Dec (STP)degstat.error;pos.eq.dec8.33333e-081.22222e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdestpMean error in PM(Dec) in STP modedeg/yrstat.error;pos.pm;pos.eq.dec8.61111e-081.30556e-072.11111e-074e-077.35e-061floatnullablerahipRight ascension in HIP modedegpos.eq.ra0.00089920811.1353181.28348.946359.9791doublenullabledehipDeclination in HIP modedegpos.eq.dec-89.7824-70.7875-2.111869.099489.56941doublenullablepmrahipProper motion in RA, cos(delta) applied, in HIP modedeg/yrpos.pm;pos.eq.ra-0.000905211-3.31047e-05-4.38889e-073.23509e-050.001879621floatnullablepmdehipProper motion in Dec in HIP modedeg/yrpos.pm;pos.eq.dec-0.00161518-4.22333e-05-1.56667e-061.49336e-050.002868591floatnullablet_rahipCentral epoch of RA (HIP)yrstat.error;time.epoch;pos.eq.ra1989.871990.921991.231991.61992.381floatnullableerr_rahipError in RA (HIP) with cos(delta) already applieddegstat.error;pos.eq.ra7.77778e-081.22222e-072.27778e-074.86111e-074.84444e-061floatnullableerr_pmrahipMean error in PM(RA)*cos(delta) in HIP modedeg/yrstat.error;pos.pm;pos.eq.ra8.61111e-081.36111e-072.72222e-076.41028e-079.37222e-061floatnullablet_dehipCentral epoch of Dec (HIP)yrstat.error;time.epoch;pos.eq.dec1990.321990.811991.271991.71992.51floatnullableerr_dehipError in Dec (HIP)degstat.error;pos.eq.dec8.33333e-081.22222e-071.86111e-073.69444e-073.02222e-061floatnullableerr_pmdehipMean error in PM(Dec) in HIP modedeg/yrstat.error;pos.pm;pos.eq.dec8.88889e-081.36111e-072.27778e-074.91667e-077.35e-061floatnullableparallaxsiParallax obtained in solution SIdegpos.parallax-8.21667e-06-1.66667e-081.21944e-066.85e-060.0001523251floatnullableerr_parallaxsiError in parallax obtained in solution SIdegstat.error;pos.parallax1.16667e-071.63889e-072.91667e-075.86111e-075.77778e-061floatnullableparallaxstpParallax obtained in solution STPdegpos.parallax-8.21667e-06-1.66667e-081.21944e-066.84444e-060.000152451floatnullableerr_parallaxstpError in parallax obtained in solution STPdegstat.error;pos.parallax1.16667e-071.63889e-072.94444e-075.88889e-075.77778e-061floatnullableparallaxhipParallax obtained in solution HIPdegpos.parallax-8.21667e-06-1.94444e-081.21944e-066.84444e-060.0001525031floatnullableerr_parallaxhipError in parallax obtained in solution HIPdegstat.error;pos.parallax1.16667e-071.63889e-072.97222e-075.97222e-075.77778e-061floatnullableffhF-Measure for proper motions FK5 proper motions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.030.311.484.357528.320.0454195floatnullableff0hF-Measure for proper motions original catalogue positions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.040.341.534.633.050.0454195floatnullableff0gchF-Measure for proper motions GC positions vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.010.271.373.96137.260.220922floatnullablef0fF-Measure for proper motions FK5 and Hipparcos positions vs. FK5 proper motionsstat.fit.goodness;pos.pm;arith.diff0.030.281.383.6117.290.0454195floatnullableft2hF-Measure for proper motions Tycho2 and Hipparcos proper motionsstat.fit.goodness;pos.pm;arith.diff00.231.173.1735.220.989718floatnullableflagsBinarity evidence and variability flags (see note)meta.codecharnullableaugerThis dataset comprises the public data observed by the Pierre Auger cosmic ray observatory, which is 1% of its total data. It contains 28493 events between 0.1 and 49.7 EeV collected between 2004 and 2013.auger.main Detection parameters of cosmic ray source candidates recorded by the Pierre Auger Telescope. This table can be queried on the web at http://dc.g-vo.org/auger/q/cone/form .28493eventidAuger event numbermeta.id;meta.maincharraj2000Incoming cosmic ray direction, RAdegpos.eq.ra;meta.main0.00040262510.9469180.763349.965359.9921floatdej2000Incoming cosmic ray direction, Declinationdegpos.eq.dec;meta.main-89.9781-74.9106-30.237410.888824.7081floatnstatNumber of stations participating in an eventmeta.number;obs33.03.05.0181.0shortcreReconstructed energy of the cosmic ray particleEeVphys.energy0.1103750.2400450.6095052.8442649.73311floatmjdObservation time, Modified Julian Daytime.epoch;obs53005.653404.655064.156289.156366.41floatgallonGalactic longitudedegpos.galactic.lon-179.993-158.679-50.8931120.675179.9931doublegallatGalactic latitudedegpos.galactic.lat-89.2921-74.8897-16.001553.629584.18611doubleboydendeThe Armagh-Dunsink-Harvard Becker-Schmidt Telescope was deployed at Boyden Station, Maselspoort South Africa between 1965 and 1970. During that time, astronomers from Bamberg, Heidelberg, Hamburg and Münster took astronomical images there, with a focus on old star clusters, the Magellanic clouds, and the southern milky way. This service provides scans of the plates obtained.boydende.dataThe Armagh-Dunsink-Harvard Becker-Schmidt Telescope was deployed at Boyden Station, Maselspoort South Africa between 1965 and 1970. During that time, astronomers from Bamberg, Heidelberg, Hamburg and Münster took astronomical images there, with a focus on old star clusters, the Magellanic clouds, and the southern milky way. This service provides scans of the plates obtained.244accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableexposureEffective exposure timestime.duration;obs.exposurefloatnullableobjectSpecial object on platemeta.idcharnullablestart_timeStart of exposuredtime.start;obsdoublenullableend_timeEnd of exposuredtime.end;obsdoublenullablewfpdb_idPlate identifier as in the WFPDBmeta.idcharnullablequalityPlate Qualitymeta.notecharnullablefilterFilter used (NULL if clear)meta.id;instr.filtercharnullableemulsionPlate emulsioninstr.plate.emulsioncharnullableobsnotesObservation Notesmeta.notecharnullabledatalink_urlURL to a datalink document for this plate (ancillary files, cutouts)meta.ref.urlcharnullableenvelopePlate envelope with plate metadatameta.ref.urlcharnullablepub_didGlobally unique dataset identifiercharindexednullablecarsImages and data from from the CFHTLS archive research survey, a multi-band dataset spanning 37 square degrees of sky in high galactic latitudes.cars.images Metadata for co-added CFHTLS archive images used for producing the CARS source list (cars.srccat).185accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size17640086401764008640.01764008640.01764008640.017640086401.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra33.542933.542938.3285335.224335.2241doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec-7.93333-7-4.252.641952.64191doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure0doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median3.74e-073.74e-076.28e-071.17e-061.17e-061floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max4.2e-074.2e-076.95e-071.2e-061.2e-061floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min3.3e-073.3e-075.5e-078.1e-078.1e-071floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablefieldkeyCARS field designationmeta.idcharnullablefieldbandkeyCARS field designation plus bandmeta.idcharnullablencombineNumber of individual frames in this stackmeta.number22.05.012.0141.0inttexptimeTotal Exposure Timestime.duration;obs.exposure1000.11000.153000.537200.568611.031floatnullablemagzpAB Magnitude Zeropointmagphot.mag;arith.zp24.6724.7125.7326.460326.51floatnullablemagzperrEstimated Magnitude Zeropoint Errormagstat.error;phot.mag;arith.zp0.050.050.050.150.151floatnullableseeingMeasured image seeingarcsecinstr.obsty.seeing0.480.530.7911.111floatnullableseeingerrMeasured image Seeing errorarcsecstat.error;instr.obsty.seeing000.010.07480.131floatnullablecars.srccatExtracted sources from the CARS survey, comprising positions and multiband photometry.5200000carsidCARS object IDmeta.id;meta.maincharindexedprimaryseqnrRunning object number (in field)meta.id14174.069959.0159735.01978081.0intraj2000Right ascension of barycenter (J2000)degpos.eq.ra;meta.main33.039133.402338.5181335.428335.7191doubleindexednullabledej2000Declination of barycenter (J2000)degpos.eq.dec;meta.main-8.45327-7.43634-3.8526152.776253.17111doubleindexednullablexposObject position on exposure along xpixpos.cartesian.x;instr.det852.3071611.1410536.119493.8202461floatnullableyposObject position on exposure along ypixpos.cartesian.y;instr.det315.7331312.7410692.919858.7209131floatnullablemagautoKron-like elliptical aperture magnitudemagphot.mag10.580819.644123.809425.34833.16480.999771floatindexednullablemagerrautoError in Kron-like elliptical aperture magnitudemagstat.error;phot.mag2.9648e-050.002989890.0804720.177188316.1780.999771floatnullablemagisouIsophotal magnitude in the u* bandmagphot.mag;em.opt14.44322.547326.531429.823735.69510.934003floatnullablemagisoerruRMS error of isophotal magnitude in the u* bandmagstat.error;phot.mag;em.opt9.83874e-050.01141640.1283351.8600799.93760.934003floatnullablemagapruFixed aperture magnitude in the u* bandmagphot.mag;em.opt16.168822.803525.52828.284235.56190.933742floatnullablemagaprerruRMS error of fixed aperture magnitude in the u* bandmagstat.error;phot.mag;em.opt0.0002489970.01031830.1138121.5180799.38550.933742floatnullablemaglimuLimiting magnitude at object's position in u* bandmag22.656327.45728.04728.4962106.580.998128floatnullablemagisogIsophotal magnitude in the g' bandmagphot.mag;em.opt13.311121.461725.849128.670535.70180.979261floatnullablemagisoerrgRMS error of isophotal magnitude in the g' bandmagstat.error;phot.mag;em.opt4.79987e-050.003123280.04604340.41429499.9050.979261floatnullablemagaprgFixed aperture magnitude in the g' bandmagphot.mag;em.opt16.409421.612924.884426.947836.23920.985983floatnullablemagaprerrgRMS error of fixed aperture magnitude in the g' bandmagstat.error;phot.mag;em.opt0.0001425810.002761680.04013440.3495499.35220.985983floatnullablemaglimgLimiting magnitude at object's position in g' bandmag21.420927.809628.320428.783125.1310.998303floatnullablemagisorIsophotal magnitude in the r' bandmagphot.mag;em.opt13.900720.76725.351928.004734.560.926875floatnullablemagisoerrrRMS error of isophotal magnitude in the r' bandmagstat.error;phot.mag;em.opt9.73191e-050.00382380.05945240.54719499.94960.926875floatnullablemagaprrFixed aperture magnitude in the r' bandmagphot.mag;em.opt15.378520.800424.419426.246535.75460.959629floatnullablemagaprerrrRMS error of fixed aperture magnitude in the r' bandmagstat.error;phot.mag;em.opt0.0001664950.00330010.05217540.47675298.7590.959629floatnullablemaglimrLimiting magnitude at object's position in r' bandmag20.759726.690527.340827.8543135.4070.986994floatnullablemagisoiIsophotal magnitude in the i' bandmagphot.mag;em.opt12.396820.066324.730627.047932.58960.985109floatnullablemagisoerriRMS error of isophotal magnitude in the i' bandmagstat.error;phot.mag;em.opt3.60199e-050.00156630.02582150.089544149.95440.985109floatnullablemagapriFixed aperture magnitude in the i' bandmagphot.mag;em.opt16.052420.186323.915325.210335.08390.997653floatnullablemagaprerriRMS error of fixed aperture magnitude in the i' bandmagstat.error;phot.mag;em.opt0.0001504640.001416710.02562370.093068895.08080.997653floatnullablemaglimiLimiting magnitude at object's position in i' bandmag21.121127.022827.541527.953937.50.999868floatnullablemagisozIsophotal magnitude in the z' bandmagphot.mag;em.opt12.504319.63824.445827.327133.79020.975752floatnullablemagisoerrzRMS error of isophotal magnitude in the z' bandmagstat.error;phot.mag;em.opt5.97762e-050.002604750.05324870.47647299.12760.975752floatnullablemagaprzFixed aperture magnitude in the z' bandmagphot.mag;em.opt14.458819.691723.510625.791433.50170.962883floatnullablemagaprerrzRMS error of fixed aperture magnitude in the z' bandmagstat.error;phot.mag;em.opt9.22014e-050.002076770.04795890.50915499.52440.962883floatnullablemaglimzLimiting magnitude at object's position in z' bandmag20.554225.927926.534927.0166123.8010.998727floatnullablefwhmFull width half max assuming a gaussian coredegphys.angSize-0.03157460.0001595550.0002919460.0006498650.09718711floatindexednullablefluxradiusFraction-of-light radiuspix-1.32913e+061.696262.828396.2875978221.41floatnullablemajoraxisProfile RMS along major axisdegphys.angSize.smajAxis2.58341e-053.90958e-058.28685e-050.0002539280.04533211floatnullableminoraxisProfile RMS along minor axisdegphys.angSize.sminAxis6.70848e-062.31541e-056.21943e-050.0001744590.0132611floatnullablethetaPosition angle (east of north) (J2000)degpos.posAng-90-86.1490.31008186.3225901floatnullablesgclassS/G classifier output (0..1)src.class.starGalaxy4.62885e-050.0003019550.1763220.9788520.999911floatnullableextflagsExtraction Flags00.00.01.011.0intmaskTrue if object is within an object maskmeta.codebooleanz_bPhotometric redshift0.020.140.663.93.91floatnullablet_bMask value112.6675.33361floatnullableoddsConfidence parameter for photometric redshift0.043510.29430.815910.9998111floatnullablengoodfiltersNumber of filters with good photometry for BPZmeta.code.qual01.05.05.051.0intnbadfiltersNumber of filters with bad photometry for BPZmeta.code.qual00.00.02.051.0intnfaintfiltersNumber of filters with faint photometry for BPZmeta.code.qual00.00.03.051.0intgoodfiltersFilters with faint photometry for BPZcharnullablebadfiltersFilters with bad photometry for BPZcharnullablefaintfiltersFilters with faint photometry for BPZcharnullablefieldkeyCARS field designationmeta.idcharnullablecs82morphoz This is a catalogue of photometric redshifts of galaxies in the Stripe 82 obtained when morphology (galaxy size, ellipticity, Sérsic index, and surface brightness) are included in training on galaxy samples from the SDSS and the CFHT Stripe-82 Survey (CS82). Our redshifts yield a 68th percentile error of 0.058(1 + z), and a outlier fraction of 5.2 per cent.cs82morphoz.main This is a catalogue of photometric redshifts of galaxies in the Stripe 82 obtained when morphology (galaxy size, ellipticity, Sérsic index, and surface brightness) are included in training on galaxy samples from the SDSS and the CFHT Stripe-82 Survey (CS82). Our redshifts yield a 68th percentile error of 0.058(1 + z), and a outlier fraction of 5.2 per cent.5800000objid_cs82Identifier built as im_num*1000000+se_idmeta.id;meta.main5675056558.6788027318.0168034150.981722278421.0intindexedprimaryraICRS Right Ascensiondegpos.eq.ra;meta.main0.0002067622.5797240.4515357.0043601doubleindexednullabledecICRS Declinationdegpos.eq.dec;meta.main-1.28482-0.961096-0.05497160.8761881.228251doubleindexednullableflagsSource extraction quality flag (ranges from 0 to 3, with 0 being the best)meta.code00.00.03.031.0shortweightlensFit shape measurement confidence. weight>0 indicates good shape measurementstat.weight007.7034515.538415.5631floatnullablefitclasslensFit star-galaxy classifier: 1=stars; 0=galaxies; -1=no usable data; -2=blended objects; -3=miscellaneous reasons; -4=chi-square exceeded critical valuemeta.code;src.class-4-2.00.00.011.0shortmag_autoCS82 Kron i-band magnitudemagphot.mag;em.opt.i15.401119.703722.757823.94324.21floatindexednullablemagerr_autoCS82 Kron i-band magnitude error. Signal-to-noise ratio is 1.086/MAGERR_AUTOmagstat.error;phot.mag;em.opt.i0.0002210160.005301010.05285830.10470.10861floatnullablemag_expCS82 exponential fit i-band magnitudemagphot.mag;em.opt.i14.228219.728722.681323.828724.42231floatnullablemag_psfCS82 PSF i-band magnitudemagphot.mag;em.opt.i16.855220.662323.32924.387824.81floatnullablereff_expExponential fit effective radiusarcsecphys.angsize;src0.1300080.2146830.5160231.520128.984911floatnullableaspect_expExponential fit axis-ratiosrc.morph.param0.03600280.1355070.5547260.9402950.9999961floatnullablemu_mean_expExponential fit mean surface brightnessmag/arcsec**2phot.mag.sb;em.opt.i17.203120.099222.28424.226825.21floatnullablep_expExponential shape probability: ~1 -> disc galaxy; ~0 -> elliptical galaxystat.fit.goodness0.1822790.4779520.5007720.5414390.8194761floatnullablen_serSersic indexstat.fit.param0.30.3520512.254248.8367101floatnullablespread_model_serSersic spread model, the star-galaxy separator we used for this study. All objects in this catalogue have SPREAD_MODEL_SER>0.008, which are considered extended objects (galaxies).stat.fit.param0.008000010.008819290.01833860.033171214695.81floatnullablelensLensing tag. Objects with lens=1 are objects from the lensing subsample (fitclass=0, weight>0)meta.code00.01.01.011.0shortobjid_sdssSDSS object ID for objects with matched ugriz broadband magnitudes (if available)meta.id.cross-9223372036854775808-9.223372036854776e+188.647474692489348e+188.647475121987258e+1886474751225259653211.0longnullablemag_dered_uSDSS dereddened u-band magnitudemagphot.mag;em.opt.U17.263321.85624.162629.301431.59960.822648floatnullablemag_dered_gSDSS dereddened g-band magnitudemagphot.mag;em.opt.V16.509320.818823.665325.627729.39970.822648floatnullablemag_dered_rSDSS dereddened r-band magnitudemagphot.mag;em.opt.R16.000119.858222.984224.226124.50.822648floatnullablemag_dered_iSDSS dereddened i-band magnitudemagphot.mag;em.opt.I15.455919.401622.476223.864725.19960.822648floatnullablemag_dered_zSDSS dereddened z-band magnitudemagphot.mag;em.opt.I14.851619.084722.10124.444128.79820.822648floatnullablezspecSpectroscopic redshift from source given in source_specsrc.redshift-9e-050.05089560.3582251.090737.011240.0111949floatnullablezphotPhotometric redshift estimated using inputs ugriz+morphologysrc.redshift0.02162620.2382850.8080471.196871.812910.822648floatnullablezmorphPhotometric redshift estimated using inputs i+morphologysrc.redshift0.01842690.3665350.908161.150573.40282e+381floatnullablezbestBest redshift for this object, in order of priority: zspec, zphot, zmorphsrc.redshift0.004540040.2527790.847411.209823.40282e+381floatindexednullableodds_photOdds value for zphotstat.fit.goodness0.04013940.3628110.6641660.92072410.822648floatnullableodds_morphOdds value for zmorphstat.fit.goodness0.02046160.2585220.4578180.66786610.999999floatnullableodds_bestOdds value for zbest (=1 if zspec is used)stat.fit.goodness0.02046160.3215290.6233540.92378811floatnullablesource_specSource of spectroscopy: SDSS, BOSS, DEEP2, WIGGLEZ or VVDSmeta.bibcharnullableclass_specClass of object based on spectral fit: GALAXY or QSOmeta.code.classcharnullabledanishTBDdanish.dataTBD2469accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableobservatObservatory the exposure was prepared atcharnullableinstrumemeta.id;instrcharnullabledetnamecharnullableorignameName given at La Sillameta.id;meta.filecharnullableobjectObject observedmeta.id;meta.maincharexptimeExposure timestime.duration;obs.exposurefloatnullabletm_startUT start timetime.epoch;obs.exposurecharnullabletm_endUT end timetime.epoch;obs.exposurecharnullablefilter_aFilter used on wheel Ameta.id;instr.filtercharnullablefilter_bFilter used on wheel Bmeta.id;instr.filtercharnullablefilterFilter usedmeta.id;instr.filter;meta.maincharnullablestSidereal time at startsfloatnullableraRight ascension at startdegpos.eq.ra;meta.mainfloatnullabledecDeclination at startdegpos.eq.dec;meta.mainfloatnullablehaHour Angle at startfloatnullablezdistZenith distance at startdegpos.az.zdfloatnullabledmubinA collection of binary stars with a difference in instantaneous proper motion as measured by HIPPARCOS and the long-term proper motion.dmubin.mainA collection of binary stars with a difference in instantaneous proper motion as measured by HIPPARCOS and the long-term proper motion.8039hipnoCatalog number in Hipparcos catalogmeta.id;meta.main143607.919999999999659816.0115066.31200821.0intraj2000Right ascension from Hipparcosdegpos.eq.ra;meta.main0.048271911.5579183.994349.574359.8761doubleindexednullabledej2000Declination from Hipparcosdegpos.eq.dec;meta.main-89.7717-70.9231-1.2634270.280789.40651doubleindexednullablecompComponent for resolved binariesmeta.codecharnullablemvVisual magnitudemagphot.mag;em.opt.V-1.444.147.5910.1313.311floatnullablecolorColor index B-V, Hipparcos V magnitudemagphot.color;em.opt.B;em.opt.V-0.4-0.090.541.53.30.989302floatnullableparallaxParallax from Hipparcosmaspos.parallax.trig-22.840.838.7345.7118742.121floatnullableffhF-Measure for proper motions FK5 vs. Hipparcosstat.fit.goodness;pos.pm;arith.diff0.050.66063.417.006961.520.143301floatnullablef0fF-measure for proper motions from FK5 vs. mu0Fstat.fit.goodness;pos.pm;arith.diff0.060.422.216.071158.720.143301floatnullablef0hF-measure for proper motions from Hipparcos vs. mu0Fstat.fit.goodness;pos.pm;arith.diff0.070.76123.6320.03581.870.143301floatnullablef0gchF-measure for proper motions from Hipparcos vs. mu0Gstat.fit.goodness;pos.pm;arith.diff0.020.633.816.664299.370.583033floatnullableft2hF-measure for proper motions from Hipparcos vs. Tycho-2stat.fit.goodness;pos.pm;arith.diff0.020.7384.1714.928212.250.977858floatnullablefmaxMaximum of F-measures reportedstat.fit.goodness;pos.pm;arith.diff3.453.484.6516.88212.251floatnullablefkFK Part the star was found inmeta.refcharnullablegcStar Identifier in the GCmeta.id.cross23978.319999999999916628.032409.52333370.5830327intnullablet2Object is in Tycho-2meta.codebooleanhdStar Identifier in the HD-Cataloguemeta.id.cross34825.16109499.0222890.243528600.9261102intnullablehrStar Identifier in the HR-Cataloguemeta.id.cross1239.874553.08820.6591100.25251898intnullablecns4Star Identifier in CNS4meta.id.crosscharnullablefknoStar Identifier in the FKmeta.id.cross384.062220.05789.70000000000161050.14330141intnullablestar_nameName of the starmeta.idcharnullableccdmStar Identifier in the CCDM-Cataloguemeta.id.crosscharnullableflare_survey From 1986 through 1991, the Astronomical Institute of Münster University performed a search for flare stars in several southern associations and open stellar clusters using the GPO telescope (d=40 cm, WFPDB identifier ESO040); the fields suveyed include Coalsack, M42, B228 Lup, the Chameleon T1 association, omicron Vel cluster, R CrA association, the Pipe nebula (B59 Oph), and the Sco-Oph association. This was done primarily through multiple exposures. The files published here are plate scans done in 2017. The obscore collection name for these files is Muenster Flare Survey.flare_survey.data From 1986 through 1991, the Astronomical Institute of Münster University performed a search for flare stars in several southern associations and open stellar clusters using the GPO telescope (d=40 cm, WFPDB identifier ESO040); the fields suveyed include Coalsack, M42, B228 Lup, the Chameleon T1 association, omicron Vel cluster, R CrA association, the Pipe nebula (B59 Oph), and the Sco-Oph association. This was done primarily through multiple exposures. The files published here are plate scans done in 2017. The obscore collection name for these files is Muenster Flare Survey.580accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size6837120096433920.096433920.0100175040.01001779201.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra83.796583.8208192.654285.475285.4751doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec-77.684-76.7448-36.9522-5.39111-5.071doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure4460846080.647537.148418.848452.31doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median4.1e-074.1e-074.1e-074.1e-076.5e-070.998276floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max5e-075e-075e-075e-077.1e-070.998276floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min3.4e-073.4e-073.4e-073.4e-075.4e-070.998276floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablekindDirect observation, stellar tracks, or multiple exposure?meta.code;obscharnullableobjectName of the target object (mostly, cluster or association)meta.id;srccharindexednullableobs_durationTime between first shutter open and last shutter close (for multiply exposed plates, this is not the total exposure time)stime.interval;obs.exposure624003600420054001floatnullabletotal_exptimeLength of exposure (non-contiguous for multiply exposed platesstime.duration;obs.exposure624003600420054001floatnullableemulsionPhotographic emulsion used.instr.plate.emulsioncharnullablepub_didPublisher data set id; this is an identifier for the dataset in question and can be used to retrieve the data through, e.g., datalink.meta.id;meta.maincharnullabledatalink_urlURL to a datalink document for this plate (ancillary files, cutouts)meta.ref.urlcharnullablewfpdb_idPlate identifier as in the WFPDBmeta.idcharnullablegdr2dist This catalogue provides distances estimates (and uncertainties therein) for 1.33 billion stars over the whole sky brighter than about G=20.7. These have been estimated using the parallaxes (and their uncertainties) from Gaia DR2. A Bayesian procedure was used involving a prior with a single parameter L(l,b), which varies smoothly with Galactic longitude and latitude according to a Galaxy model. The posterior is summarized with a point estimate (usually the mode) and a confidence interval (usually the 68% highest density interval). The estimation procedure is described in detail in the `accompanying paper`_, which also analyses the catalogue content. .. _accompanying paper: http://www.mpia.de/homes/calj/gdr2_distances.htmlgdr2dist.main This catalogue provides distances estimates (and uncertainties therein) for 1.33 billion stars over the whole sky brighter than about G=20.7. These have been estimated using the parallaxes (and their uncertainties) from Gaia DR2. A Bayesian procedure was used involving a prior with a single parameter L(l,b), which varies smoothly with Galactic longitude and latitude according to a Galaxy model. The posterior is summarized with a point estimate (usually the mode) and a confidence interval (usually the 68% highest density interval). The estimation procedure is described in detail in the `accompanying paper`_, which also analyses the catalogue content. .. _accompanying paper: http://www.mpia.de/homes/calj/gdr2_distances.html1400000000source_idUnique source identifier. Note that this *cannot* be matched against the DR1 source_id.meta.id;meta.main208907211095044.314552101313878e+174.317781268923228e+186.712850540084986e+1869175102672243891201.0longindexedprimaryr_estEstimated distancepcpos.distance0.593017533.8972839.876067.725939.10.999997floatindexednullabler_loLower bound on the 1 σ confidence intervalpcpos.distance;stat.min0373.0561572.493977.791floatnullabler_hiUpper bound on the 1 σ confidence intervalpcpos.distance;stat.max0.59354750.5965190.929857.761floatnullabler_lenLength scale used in the prior for the distance estimation.pcstat.fit.param;pos.distance335.228465.4391472.562320.332597.671floatnullableresult_flagType of result.meta.code.qual01.01.01.021.0shortmodality_flagResult regime flag: number of modes in the posterior (1 or 2).meta.code11.01.01.021.0shortgdr2mock This catalogue is a simulation of the Gaia DR2 stellar content using Galaxia (a tool to sample stars from a Besancon-like Milky Way model), 3d dust extinction maps and the latest PARSEC Isochrones. It is mimicking the Gaia DR2 data model and an apparent magnitude limit of g=20,7. Extinctions and photometry in different bands have also been included in a supplementary table as well as uncertainty estimates using a scaled nominal error model.gdr2mock.mainA synthetic Milky Way catalog mimicking GDR2 in stellar content and data model.source_idHealpix number using Nside = 4096 with the nested scheme on equatorial coordinates times 2^35. The last digits of the source_id are reserved for a running number that serves as a unique identifier per HEALPix cell. This is formed in accordance with Gaia's source_id definition, but of course mock objects have no relation to any Gaia objects that may have an identical source_id.meta.id;meta.main149808459284484.704526787411968e+174.2539869858043003e+186.718878990540472e+1869175283060865761301.0longindexedraBarycentric Right Ascension in ICRS at ref_epochdegpos.eq.ra;meta.maindoubleindexednullabledecBarycentric Declination in ICRS at ref_epochdegpos.eq.dec;meta.maindoubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.rafloatnullabledec_errorStandard error of decmasstat.error;pos.eq.decfloatnullablepmraProper motion in right ascension of the source in ICRS at ref_epoch. This is the projection of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.rafloatindexednullablepmdecProper motion in declination at ref_epoch.mas/yrpos.pm;pos.eq.decfloatindexednullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.rafloatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.decfloatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch ref_epoch. If looking for a distance, consider joining with gdr2dist.main and using the distances from there.maspos.parallaxfloatnullableparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale.magphot.mag;em.opt;stat.meanfloatindexednullablephot_g_mean_fluxG-band mean flux as electrons per second.s**-1phot.flux;em.opt;stat.meandoublenullablephot_g_mean_flux_errorError on phot_g_mean_fluxs**-1stat.error;phot.flux;em.opt;stat.meanfloatnullablephot_rp_mean_fluxMean flux in the integrated RP band.s**-1phot.flux;em.opt.Rdoublenullablephot_rp_mean_flux_errorError in the mean flux in the integrated RP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Rfloatnullablephot_rp_mean_magMean magnitude in the integrated RP band. This is computed from the RP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Rfloatindexednullablephot_bp_mean_fluxMean flux in the integrated BP band.s**-1phot.flux;em.opt.Bdoublenullablephot_bp_mean_flux_errorError in the mean flux in the integrated BP band. Errors are computed from the dispersion about the weighted mean of the input calibrated photometry.s**-1stat.error;phot.flux;em.opt.Bfloatnullablephot_bp_mean_magMean magnitude in the integrated BP band. This is computed from the BP-band mean flux applying the magnitude zero-point in the Vega scale. No error is provided for this quantity as the error distribution is only symmetric in flux space. For errors small compared to the flux (less than 10%, say), the magnitude error is well approximated by 1.09*flux/flux_err.magphot.mag;em.opt.Bfloatindexednullablephot_bp_rp_excess_factorBP/RP excess factor estimated from the comparison of the sum of integrated BP and RP fluxes with respect to the flux in the G band. This measures the excess of flux in the BP and RP integrated photometry with respect to the G band. This excess is believed to be caused by background and contamination issues affecting the BP and RP data. Therefore a large value of this factor for a given source indicates systematic errors in the BP and RP photometry.stat.fit.goodnessfloatnullableradial_velocitySpectroscopic radial velocity in the solar barycentric reference frame. The radial velocity provided is the median value of the radial velocity measurements at all epochs. Warning: in the vicinity of bright stars, DR2 RVs can be grossly wrong. See arXiv:1901.10460 for details.km/sspect.dopplerVelocfloatnullableradial_velocity_errorThe radial velocity error is the error on the median to which a constant noise floor of 0.11 km/s has been added in quadrature to take into account the calibration contribution.km/sstat.error;spect.dopplerVelocfloatnullableastrometric_gof_alGoodness-of-fit statistic of the astrometric solution for the source in the along-scan direction (you probably want to use RUWE instead of this).stat.fit.goodnessfloatnullableastrometric_params_solvedThis is a binary code indicating which astrometric parameters were estimated for the source. A set bit means the parameter was estimated. The least-significant bit represents α, the next bits δ, parallax, PM(RA) and PM(De). For Gaia DR2 the only relevant values are 31 (all five parameters solved) and 3 (only positions).meta.codeshortnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.codelongindexedlGalactic longitude (converted from ra, dec)degpos.galactic.londoubleindexednullablebGalactic latitude (converted from ra, dec)degpos.galactic.latdoubleindexednullablephot_g_n_obsNumber of observations contributing to G photometrymeta.numbershortnullablephot_variable_flagPhotometric variability flagmeta.code;src.varcharnullablephot_rp_n_obsNumber of observations (CCD transits) that contributed to the integrated RP mean flux and mean flux error.meta.number;obs;phot.mag;em.opt.Rshortphot_bp_n_obsNumber of observations (CCD transits) that contributed to the integrated BP mean flux and mean flux error.meta.number;obs;phot.mag;em.opt.Bshortbp_rpBP-RP colormagphot.color;em.opt.B;em.opt.Rfloatnullablebp_gBP-G colormagphot.color;em.opt.B;em.opt.Vfloatnullableg_rpG-RP colormagphot.color;em.opt.V;em.opt.Rfloatnullablephot_rvs_mean_magApproximate estimate for the RVS magnitude. This uses formulae (2) and (3) from 2018A&A...616A...1G. Outside of the range 0.1<BP-G<1.7 we use Eq. 3 (which means the value is probably fairly bogus).magphot.color;em.opt.Ifloatnullablerv_nb_transitsNumber of transits (epochs) used to compute radial velocity.meta.number;obs;spect.dopplerVelocshortref_epochReference epoch to which the astrometic source parameters are referred, expressed as a Julian Year in TCB.yrmeta.ref;time.epochdoublenullableastrometric_delta_qHipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)stat.valuefloatnullableastrometric_excess_noiseExcess noise of the sourcemasstat.valuefloatnullableastrometric_excess_noise_sigSignificance of excess noisestat.valuefloatnullableastrometric_n_obs_acTotal number of observations ACmeta.numbershortastrometric_n_obs_alTotal number of observations ALmeta.numbershortastrometric_n_bad_obs_acNumber of bad observations ACmeta.numbershortastrometric_n_bad_obs_alNumber of bad observations ALmeta.numbershortastrometric_n_good_obs_acNumber of good observations ACmeta.numbershortastrometric_n_good_obs_alNumber of good observations ALmeta.numbershortastrometric_chi2_alAstrometric goodness-of-fit (χ²) in the AL direction; χ² values were computed for the ‘good’ AL observations of the source, without taking into account the astrometric excess noise (if any) of the source. They do, however, take into account the attitude excess noise (if any) of each observation.stat.fit.chi2floatnullableastrometric_primary_flagOnly primary sources (for which this flag is True) contribute to the estimation of attitude, calibration, and global parameters. The estimation of source parameters is not affected by primariness.meta.codeshortastrometric_pseudo_colourColour of the source assumed in the final astrometric processing, given as he effective wavenumber of the photon flux distribution in the astrometric (G) band. The value given in this field was astrometrically determined in a preliminary solution, using the chromatic displacement of image centroids calibrated by means of the effective wavenumbers (ν_eff) of primary sources calculated from BP and RP magnitudes. The field is empty when no such determination was possible, in which case a default value of 1.6 1/µm was assumed.um**-1floatnullablemean_varpi_factor_alMean parallax factor in the AL direction, computed from all the good observations of the source processed in the astrometry. The value given in this field is typically in the range [−0.23, +0.32] (1st and 99th percentiles). A value outside this range indicates a distribution of observations that is unfavourable for the determination of the parallax, and the calculated parallax could then be more vulnerable to errors, e.g. from the calibration model, not reflected in the formal uncertainties.stat.fit.paramfloatnullablevisiblilty_periods_usedNumber of visibility periods used in Astrometric solution. A visibility period is a group of observations separated from other groups by a gap of at least 4 days.meta.number;obsshortastrometric_sigma5d_maxThe longest principal axis in the 5-dimensional error ellipsoid. This is useful for filtering out cases where one of the five parameters, or some linear combination of several parameters, is particularly ill-determined. It is measured in mas and computed as the square root of the largest singular value of the scaled 5 × 5 covariance matrix of the astrometric parameters.masstat.error;obs;stat.maxfloatnullablematched_observationsThe number of observations (detection transits) that have been matched to a given source during the last internal crossmatch revision.meta.numbershortastrometric_priors_usedType of prior used in in the astrometric solutionshortnullableastrometric_relegation_factorRelegation factor of the source calculated as per Eq. (118) in 2012A&A...538A..78L used for the primary selection process.arith.factorfloatnullableastrometric_weight_acMean astrometric weight of the sourcemas**-2stat.weight;stat.meanfloatnullableastrometric_weight_alMean astrometric weight of the sourcemas**-2stat.weight;stat.meanfloatnullableduplicated_sourceDuring data processing, this source happened to have been duplicated and one source only has been kept.shortra_dec_corrCorrelation between right ascension and declinationstat.correlationfloatnullablera_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatnullablera_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatnullabledec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatnullabledec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatnullablepmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatnullablera_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatnullabledec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatnullableparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatnullableparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatnullablescan_direction_mean_k1Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k1Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k2Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k2Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k3Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k3Degree of concentration of scan directions across the sourcefloatnullablescan_direction_mean_k4Mean position angle of scan directions across the sourcedegfloatnullablescan_direction_strength_k4Degree of concentration of scan directions across the sourcefloatnullablepriam_flagsFlags describing the status of the astrophysical parameters Teff, A G and E[BP-RP] (i.e., those determined by Apsis-Priam). See the release documentation.meta.codelongnullableflame_flagsFlags describing the status of the astrophysical parameters radius and luminosity (i.e., those determined by Apsis-FLAME). See the release documentation.meta.codelongnullableteff_valEffective temperature of the starKphys.temperaturefloatnullableteff_percentile_lowerLower uncertainty bound of the effective temperature estimate from Apsis-Priam. This is the 16th percentile of its PDF.Kphys.temperature;stat.minfloatnullableteff_percentile_upperUpper uncertainty bound of the effective temperature estimate from Apsis-Priam. This is the 84th percentile of its PDF.Kphys.temperature;stat.maxfloatnullablea_g_valLine-of-sight extinction in the G band, A_Gmagphys.absorptionfloatnullablea_g_percentile_lowerLower uncertainty bound of the line-of-sight extinction in the G-band estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablea_g_percentile_upperUpper uncertainty bound of the line-of-sight extinction in the G-band estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullablee_bp_min_rp_valLine-of-sight reddening E(BP-RP)magphys.absorptionfloatnullablee_bp_min_rp_percentile_lowerLower uncertainty bound of the line-of-sight reddening E(BP-RP) estimate from Apsis-Priam. This is the 16th percentile of its PDF.magphys.absorption;stat.minfloatnullablee_bp_min_rp_percentile_upperUpper uncertainty bound of the line-of-sight reddening E(BP-RP) estimate from Apsis-Priam. This is the 84th percentile of its PDF.magphys.absorption;stat.maxfloatnullableradius_valStellar radius in solar radiisolRadphys.size.radiusfloatnullableradius_percentile_lowerLower uncertainty bound of the radius estimate from Apsis-FLAME. This is the 16th percentile of its PDF.solRadphys.size.radius;stat.minfloatnullableradius_percentile_upperUpper uncertainty bound of the radius estimate from Apsis-FLAME. This is the 84th percentile of its PDF.solRadphys.size.radius;stat.maxfloatnullablelum_valStellar luminosity in solar luminosities.solLumphys.luminosityfloatnullablelum_percentile_lowerLower uncertainty bound of the luminosity estimate from Apsis-FLAME. This is the 16th percentile of its PDF.solLumphys.luminosity;stat.minfloatnullablelum_percentile_upperUpper uncertainty bound of the luminosity estimate from Apsis-FLAME. This is the 84th percentile of its PDF.solLumphys.luminosity;stat.maxfloatnullablefehFe/H as log10 of solar ratio ('dex')phys.abund.Fefloatnullablea0Monochromatic extinction at lambda = 547.7nmmagphys.absorptionfloatnullablemassInitial mass of the starsolMassphys.massfloatnullableageAge of the starGyrtime.agefloatnullableloggLogarithm of surface gravity.log(cm/(s**2))phys.gravityfloatnullablenobsNominal number of observations, scaled to the shorter time base of GDR2 (a function with ecliptic latitude).meta.number;obsintindex_parsecForeign key into the photometry/extinction table.meta.id.crossintgdr2mock.photometryindex_parsecindex_parsecgdr2mock.photometryThis table contains simulated absolute magnitudes to about 0.1 mag precision for all the stars, as well as extinctions in several bands; To use it, join it USING (parsec_index) with the gdr2mock.main table.mag_gaia_gSimulated absolute magnitude in the Gaia G band (note that no extinction is applied).magphot.mag;em.opt.Vfloatnullablemag_ubv_uSimulated absolute magnitude in the Johnson U band (note that no extinction is applied).magphot.mag;em.opt.Ufloatnullablemag_ubv_bSimulated absolute magnitude in the Johnson B band (note that no extinction is applied).magphot.mag;em.opt.Bfloatnullablemag_ubv_vSimulated absolute magnitude in the Johnson V band (note that no extinction is applied).magphot.mag;em.opt.Vfloatnullablemag_ubv_rSimulated absolute magnitude in the Johnson R band (note that no extinction is applied).magphot.mag;em.opt.Rfloatnullablemag_ubv_iSimulated absolute magnitude in the Johnson I band (note that no extinction is applied).magphot.mag;em.opt.Ifloatnullablemag_ubv_jSimulated absolute magnitude in the Johnson J band (note that no extinction is applied).magphot.mag;em.ir.Jfloatnullablemag_ubv_hSimulated absolute magnitude in the Johnson H band (note that no extinction is applied).magphot.mag;em.ir.Hfloatnullablemag_ubv_kSimulated absolute magnitude in the Johnson K band (note that no extinction is applied).magphot.mag;em.ir.Kfloatnullablemag_sdss_uSimulated absolute magnitude in the SDSS u band (note that no extinction is applied).magphot.mag;em.opt.Ufloatnullablemag_sdss_gSimulated absolute magnitude in the SDSS g band (note that no extinction is applied).magphot.mag;em.opt.Vfloatnullablemag_sdss_rSimulated absolute magnitude in the SDSS r band (note that no extinction is applied).magphot.mag;em.opt.Rfloatnullablemag_sdss_iSimulated absolute magnitude in the SDSS i band (note that no extinction is applied).magphot.mag;em.opt.Ifloatnullablemag_sdss_zSimulated absolute magnitude in the SDSS z band (note that no extinction is applied).magphot.mag;em.opt.Ifloatnullablemag_2mass_jSimulated absolute magnitude in the 2MASS J band (note that no extinction is applied).magphot.mag;em.ir.Jfloatnullablemag_2mass_hSimulated absolute magnitude in the 2MASS H band (note that no extinction is applied).magphot.mag;em.ir.Hfloatnullablemag_2mass_ksSimulated absolute magnitude in the 2MASS K' band (note that no extinction is applied).magphot.mag;em.ir.Kfloatnullablemag_wise_w1Simulated absolute magnitude in the WISE W1 band (note that no extinction is applied).magphot.mag;em.ir.3-4umfloatnullablemag_wise_w2Simulated absolute magnitude in the WISE W2 band (note that no extinction is applied).magphot.mag;em.ir.4-8umfloatnullablemag_wise_w3Simulated absolute magnitude in the WISE W3 band (note that no extinction is applied).magphot.mag;em.ir.8-15umfloatnullablemag_wise_w4Simulated absolute magnitude in the WISE W4 band (note that no extinction is applied).magphot.mag;em.ir.15-30umfloatnullableindex_parsecThe parsec bin has the format AABBCCCDDD, where AA denotes the metallicity bin, BB the luminosity bin, CCC the T_eff bin, and DDD the extinction bin.meta.id;meta.maininta_bpExtinction in the Gaia BP bandmagphys.absorption;em.opt.Bfloatnullablea_rpExtinction in the Gaia RP bandmagphys.absorption;em.opt.Rfloatnullablea_juExtinction in the Johnson U bandmagphys.absorption;em.opt.Ufloatnullablea_jbExtinction in the Johnson B bandmagphys.absorption;em.opt.Bfloatnullablea_jvExtinction in the Johnson V bandmagphys.absorption;em.opt.Vfloatnullablea_jrExtinction in the Johnson R bandmagphys.absorption;em.opt.Rfloatnullablea_jiExtinction in the Johnson I bandmagphys.absorption;em.opt.Ifloatnullablea_jjExtinction in the Johnson J bandmagphys.absorption;em.ir.Jfloatnullablea_jhExtinction in the Johnson H bandmagphys.absorption;em.ir.Hfloatnullablea_jkExtinction in the Johnson K bandmagphys.absorption;em.ir.Kfloatnullablea_suExtinction in the SDSS u bandmagphys.absorption;em.opt.Ufloatnullablea_sgExtinction in the SDSS g bandmagphys.absorption;em.opt.Vfloatnullablea_srExtinction in the SDSS r bandmagphys.absorption;em.opt.Rfloatnullablea_siExtinction in the SDSS i bandmagphys.absorption;em.opt.Ifloatnullablea_szExtinction in the SDSS z bandmagphys.absorption;em.opt.Ifloatnullablegps1 This catalog combines Gaia DR1, Pan-STARRS 1, SDSS and 2MASS astrometry to compute proper motions for 350 million sources across three-fourths of the sky down to a magnitude of mr≈20. Positions of galaxies from Pan-STARRS 1 are used to build a reference frame for PS1, SDSS, and 2MASS data. Gaia DR1 is adapted to that reference frame by exploiting that locally, proper motions are linear. GPS1 has a characteristic systematic error of less than 0.3 mas/yr, and a typical precision of 1.5−2.0 mas/yr. The proper motions have been validated using galaxies, open clusters, distant giant stars and QSOs. In comparison with other published faint proper motion catalogs, GPS1's systematic error (<0.3 mas/yr) is about 10 times better than that of PPMXL and UCAC4 (>2.0 mas/yr). Similarly, its precision (~1.5 mas/yr) is an improvement by ∼ 4 times relative to PPMXL and UCAC4 (∼6.0 mas/yr). For QSOs, the precision of GPS1 is found to be worse (∼2.0−3.0 mas/yr), possibly due to their particular differential chromatic refraction (DCR).gps1.mainGPS1 main table with some deviations from the published paper. In particular note that Gaia and Pan-STARRS1 photometry results from blind crossmatching; see d_g and d_ps1 fields for the offsets in the respective crossmatches.350000000obj_idUnique object identifier (this is not the Pan-STARRS1 identifier).meta.id;meta.main-9218886029413203196-8.58618305832599e+18-5.348270848105831e+188.182160913630508e+1892188684372277388521.0longindexedraRight Ascension from fit (ICRS, Epoch J2010).degpos.eq.ra;meta.main2.03091e-0519.8061268.6343.3853601doubleindexednullabledecDeclination from fit (ICRS, Epoch J2010).degpos.eq.dec;meta.main-30-28.328113.662467.218489.53741doubleindexednullablee_raError in Right Ascension from Gaia DR1.degstat.error;pos.eq.ra;meta.main5.28988e-093.09612e-082.47299e-075.26147e-062.77741e-050.954241floatnullablee_decError in Declination from Gaia DR1.degstat.error;pos.eq.dec;meta.main6.70455e-092.87448e-082.30374e-074.21526e-062.77294e-050.954241floatnullablera_ps1Right Ascension from Pan-STARRS1degpos.eq.ra019.5475268.586343.3753601doublenullabledec_ps1Declination from Pan-STARRS1degpos.eq.dec-30-28.328113.622767.058186.25011doublenullablepmraProper motion in RA with cos(δ) applied; robust fit.deg/yrpos.pm;pos.eq.ra-0.000449655-5.14574e-06-1.88763e-074.74565e-060.001377421floatnullablee_pmraError of proper motion in RA, cos(δ) applied; robust fit.deg/yrstat.error;pos.pm;pos.eq.ra1.0351e-072.61013e-075.61542e-072.23567e-061.351661floatnullablepmdeProper motion in Declination; robust fit.deg/yrpos.pm;pos.eq.dec-0.000457723-5.81873e-06-4.02035e-074.08758e-060.003206861floatnullablee_pmdeError of proper motion in Declination; robust fit.deg/yrstat.error;pos.pm;pos.eq.dec1.1018e-072.478e-074.98165e-071.64354e-060.001036591floatnullablepmra_xProper motion in RA with cos(δ) applied; x-validation fit.deg/yrpos.pm;pos.eq.ra-0.000449655-4.72603e-06-1.88546e-074.27875e-060.001377421floatnullablee_pmra_xError of proper motion in RA, cos(δ) applied; x-validation fit.deg/yrstat.error;pos.pm;pos.eq.ra4.51099e-082.83695e-076.73695e-073.17563e-061.351661floatnullablepmde_xProper motion in Declination; x-validation fit.deg/yrpos.pm;pos.eq.dec-0.000439966-5.34988e-06-4.0822e-073.77059e-060.003206861floatnullablee_pmde_xError of proper motion in Declination; x-validation fit.deg/yrstat.error;pos.pm;pos.eq.dec1.11227e-072.68129e-075.96791e-072.37835e-060.001036591floatnullablepmra_ngProper motion in RA with cos(δ) applied; fit without Gaia.deg/yrpos.pm;pos.eq.ra-0.000480685-4.69048e-06-1.90879e-074.21832e-060.001377421floatnullablee_pmra_ngError of proper motion in RA, cos(δ) applied; fit without Gaia.deg/yrstat.error;pos.pm;pos.eq.ra4.56484e-084.0577e-079.60884e-074.10442e-068.426141floatnullablepmde_ngProper motion in Declination; fit without Gaia.deg/yrpos.pm;pos.eq.dec-0.000463342-5.23359e-06-4.23781e-073.74603e-060.003206861floatnullablee_pmde_ngError of proper motion in Declination; fit without Gaia.deg/yrstat.error;pos.pm;pos.eq.dec5.39438e-083.85657e-078.54277e-072.99007e-060.001036591floatnullablepmra_psProper motion in RA with cos(δ) applied; fit with only Pan-STARRS.deg/yrpos.pm;pos.eq.ra-0.000480681-4.76317e-06-1.84308e-074.32662e-060.001377421floatnullablee_pmra_psError of proper motion in RA, cos(δ) applied; fit with only Pan-STARRS.deg/yrstat.error;pos.pm;pos.eq.ra1.12563e-074.40996e-071.16899e-064.82792e-0623.81751floatnullablepmde_psProper motion in Declination; fit with only Pan-STARRS.deg/yrpos.pm;pos.eq.dec-0.000439966-5.34697e-06-4.25653e-073.9063e-060.003206861floatnullablee_pmde_psError of proper motion in Declination; fit with only Pan-STARRS.deg/yrstat.error;pos.pm;pos.eq.dec7.59397e-084.16606e-079.95097e-073.24361e-060.001036591floatnullablechi2pmraReduced χ² for the robust fit of proper motion in RAstat.fit.chi2;pos.pm;pos.eq.ra4.45838e-230.01364030.3759072.4278711952.11floatnullablechi2pmdeReduced χ² for the robust fit of proper motion in Declinationstat.fit.chi2;pos.pm;pos.eq.dec9.11828e-240.02724020.5136982.876967577.51floatnullablechi2pmra_psReduced χ² for the Pan-STARRS 1-only fit of proper motion in RAstat.fit.chi2;pos.pm;pos.eq.ra5.60253e-150.02872870.7556525.3287414249.51floatnullablechi2pmde_psReduced χ² for the Pan-STARRS 1-only fit of proper motion in Declinationstat.fit.chi2;pos.pm;pos.eq.dec1.00113e-120.06255191.062046.3593121436.41floatnullablemaggg-band PSF magnitude from Pan-STARRS1 DR1magphot.mag;em.opt.V-0.2992415.390719.273421.164630.0130.99249floatnullablee_maggError in g-band PSF magnitude from Pan-STARRS1 DR1magstat.error;phot.mag;em.opt.V00.001950760.0103710.057512458.91820.99249floatnullablemagrr-band PSF magnitude from Pan-STARRS1 DR1magphot.mag;em.opt.R014.757918.413219.946226.86480.998751floatnullablee_magrError in r-band PSF magnitude from Pan-STARRS1 DR1magstat.error;phot.mag;em.opt.R00.001529380.006610980.02878814.176790.998751floatnullablemagii-band PSF magnitude from Pan-STARRS1 DR1magphot.mag;em.opt.I014.41217.910919.533128.61310.998831floatnullablee_magiError in i-band PSF magnitude from Pan-STARRS1 DR1magstat.error;phot.mag;em.opt.I00.001382720.005327430.025059276.33590.998831floatnullablemagzz-band PSF magnitude from Pan-STARRS1 DR1magphot.mag;em.opt.I014.199417.639619.389727.85650.998626floatnullablee_magzError in z-band PSF magnitude from Pan-STARRS1 DR1magstat.error;phot.mag;em.opt.I00.001624690.00695480.032784794.70010.998626floatnullablemagyy-band PSF magnitude from Pan-STARRS1 DR1magphot.mag;em.opt.I-4.4301814.037417.461219.271726.33470.997409floatnullablee_magyError in y-band PSF magnitude from Pan-STARRS1 DR1magstat.error;phot.mag;em.opt.I00.00230360.01136170.060317248.24650.997409floatnullablemagjJ-band magnitude from 2MASSmagphot.mag;em.ir.J012.47415.51416.78621.7490.570122floatnullablee_magjError in J-band magnitude from 2MASSmagstat.error;phot.mag;em.ir.J00.0180.0610.1589.9990.570122floatnullablemaghH-band magnitude from 2MASSmagphot.mag;em.ir.H011.79414.97816.28619.9170.570123floatnullablee_maghError in H-band magnitude from 2MASSmagstat.error;phot.mag;em.ir.H00.0010.0710.2129.9990.570123floatnullablemagkK_s-band magnitude from 2MASSmagphot.mag;em.ir.K011.55114.78916.2320.3710.570124floatnullablee_magkError in K_s-band magnitude from 2MASSmagstat.error;phot.mag;em.ir.K00.0010.0650.2389.9980.570124floatnullablemaggaiaG-band magnitude from Gaiamagphot.mag;em.opt.V10.197114.605918.170119.807226.20750.954241floatnullablee_maggaiaError in G-band magnitude from Gaiamagstat.error;phot.mag;em.opt.V0.0001447570.0006872610.004555970.01725210.4011710.954241floatnullablen_obsps1Number of PS1 SeasonAVG detections.meta.number;obs34.05.06.0131.0shortn_obsnumber of all the detections.meta.number;obs35.07.09.0161.0shortsurveysSum of source codes for the source catalogues that went into this row. Pan-STARRS is always present. Source codes: 5 -- 2MASS; 10 -- SDSS, 20 -- Gaia.meta.code00.025.035.0351.0shortd_ps1Distance between position in GPS1 and the associated (closest) position in Pan-STARRS1 used for (not accounting for the epoch difference).arcsecpos.eq;arith.diff00.01734330.08259390.2137071.600741floatnullabled_gDistance between position in GPS1 and the associated (closest) position in Gaia DR1 (not accounting for the epoch difference).arcsecpos.eq;arith.diff000.08272860.2531212.999991floatnullableicecubeA list of neutrino candidate events recorded by the IceCube neutrino telescope operating in a 40 string configuration between April 2008 and May 2009.icecube.nucand Detection parameters of neutrino candidates recorded by the IceCube Neutrino Observatory. This table can be queried on web at http://dc.g-vo.org/icecube/q/web .12876evidGAVO-local event id, IAU-formatmeta.id;meta.maincharindexedprimarynualphaNeutrino arrival direction, RAdegpos.eq.ra;meta.main0.016511.0888180.57349.335359.971floatnudeltaNeutrino arrival direction, Declinationdegpos.eq.dec;meta.main02.8719726.03972.569589.5691floatmuelossEstimated muon energy loss in iceGeV/mphys.absorption0.00710.0576250.23131.511543.4351floatmueEstimated muon energy at closest distance to the center of the IceCube detectorGeVphys.energy301.35864.5352130.6512185.83195561floatnchNumber of optical modules hit in an eventmeta.number1113.020.054.02621.0shortmjdObservation time, Modified Julian Daytime.epoch;obs54562.454573.454757.754956.854971.11floatkapteyn In the context of Kapteyn's plan to obtain a photometric standard, in Potsdam more than 400 photographic plates of several Selected Areas, Special Areas, and Kapteyn-Pritchard areas were obtained between 1910 and 1933, both as direct images and with an object prism. This service provides FITS images of the science area of the plates as well as images of the entire plates, including previous markings.kapteyn.plates In the context of Kapteyn's plan to obtain a photometric standard, in Potsdam more than 400 photographic plates of several Selected Areas, Special Areas, and Kapteyn-Pritchard areas were obtained between 1910 and 1933, both as direct images and with an object prism. This service provides FITS images of the science area of the plates as well as images of the entire plates, including previous markings.374accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoublenullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullableexposureEffective exposure time.stime.duration;obs.exposurefloatnullableairmassAirmass at mean epoch.obs.airMassfloatnullableobjectSpecial object on plate.meta.idcharnullableobserverObserver.obs.observercharnullablestart_timeUT at start of exposure.dtime.start;obscharnullableend_timeUT at end of exposure.dtime.end;obscharnullablewfpdb_idPlate identifier as in the WFPDB.meta.idcharnullablepub_didDataset identifier assigned by the publisher.meta.ref.urlcharnullableplatephotoImage of the plate including border and other markings.meta.ref.urlcharnullablekatkat ARI katkat is a catalog of star catalogues in the spirit of G. Teleki's catalog of star catalogs (`1989BOBeo.140..131T`_ and references in there). It contains 2573 catalogs suitable for astrometric usage, starting with Flamsteed (1835) and ending in the 1970ies. For almost all of them, there is a column description file (as PDF, and unfortunately sometimes in German) and the digitized content. .. _1989BOBeo.140..131T: http://ads.g-vo.org/abs/1989BOBeo.140..131Tkatkat.katkatThe "catalog of catalogs" lists catalogs containing stellar positions for the last centuries. It also lets you access digitized table data.2573fileidARI-internal file identifiermeta.id;meta.maincharindexedprimarykkidARIGFH identifier of the tablemeta.idcharnullabletelekiTeleki number of the catalogmeta.id66231.11459.02589.951090.9214924intnullablehdwlHDWL number of the catalogmeta.idcharnullablenrowsNumber of rows (i.e., lines) in the catalogmeta.number015.0408.020341.27999999998425399130.52429074intnullablenidNumber of objects that could be matched with the ARIGFH mastermeta.number013.0397.517332.649999999985853820.52467936intnullablesourceBibliographical information for the catalog.meta.refcharindexednullableremarksRemarks, e.g., on the identification process or where to find media (typically not interesting outside ARI).meta.notecharnullableminepochEarliest epoch of observation (approximate)yrtime.epoch;stat.min1917651910198420000.879907floatnullablemaxepochLatest epoch of observation (approximate)yrtime.epoch;stat.max191778.621918199020000.876409floatnullablekatdataRelative path to the data file (see table description to obtain the data if this is not a complete URLcharnullablekatfieldsURL of a PDF containing the field description (see table description to obtain the data if this is not a complete URLcharnullableliesfPainful FORTRAN used to parse the raw textcharnullablelamost5 This services provides 1D spectra from DR5 of LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) through SSAP; data is served both in VO-standard SDM and, via datalink, the original SDSS-inspired FITS described in http://dr5.lamost.org/doc/data-production-description .lamost5.data This services provides 1D spectra from DR5 of LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) through SSAP; data is served both in VO-standard SDM and, via datalink, the original SDSS-inspired FITS described in http://dr5.lamost.org/doc/data-production-description .9100000accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size100000100000.0100000.0100000.01000001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshift-0.00494382-0.00033757-1.935e-050.000504085.598880.926546floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNR0floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.0009166670.0009166670.0009166670.0009166670.0009166671floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value55858.555913.656964.957866.557920.81doubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent353.2210001800540090001floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value2.61962e-072.67242e-072.69957e-072.60729e-062.60729e-061floatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extent5.23924e-075.34484e-075.39915e-075.21458e-065.21458e-061floatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start3.69999e-073.69999e-073.69999e-073.69999e-063.69999e-061floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop8.93923e-079.05524e-079.09913e-078.91456e-068.91456e-061floatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Length37483820.03909.03909.039091.0intnullableraj2000Observed RA of the objectdegpos.eq.ra;meta.main012.0573118.133340.7453601doublenullabledej2000Main value of declinationdegpos.eq.dec;meta.main-9.8628-2.7504127.640255.30762.6041doublenullablessa_targsubclassObject subclasscharnullablelightmeter We give continuous night and day light measurements at all natural outdoor light levels by a network of low-cost lightmeters. Developed to start simple, global continuous high cadence monitoring of night sky brightness and artificial night sky brightening (light pollution) in 2009. The lightmeter network is a project of the Thüringer Landessternwarte, Tautenburg, Germany and the Kuffner-Sternwarte society at the Kuffner-Observatory, Vienna, Austria. It started as part of the Dark Skies Awareness cornerstone of the International Year of Astronomy.lightmeter.geocountsLightmeter data by date and geographic positionepochJD of measurement, UTCdtime.epoch2.4548e+062.45517e+062.45646e+062.45902e+062.45944e+061doublestationidIdentifier of the measuring station, starting with an ISO CCmeta.id;meta.maincharlatLatitude of the observing stationdegpos.earth.lat-111.707148.322453.098453.62020.954545doublenullablelongLongitude of the observing stationdegpos.earth.lon-78.789-5.08813.3519133.545139.6440.931818doublenullablefluxCalibrated fluxW.m**-2phot.flux-3.27131.07366e-052.87037797.3111floatlightmeter.measurementsTime-averaged lightmeter measurements3400000stationidIdentifier of the measuring station, starting with an ISO CCmeta.id;meta.maincharindexedepochJD of measurement, UTCdtime.epoch2.4548e+062.45517e+062.45646e+062.45902e+062.45944e+061doubleindexedfluxCalibrated fluxW.m**-2phot.flux-3.27131.07366e-052.87037797.3111floats_fluxStandard deviation of light measurements contributing to this averageW.m**-2stat.stdev;phot.fluxfloatnullablenvalsNumber of measurements contributing to this valuemeta.number;obs15.0568.0600.053191.0intsourceSource file keymeta.id;meta.filecharnullablelightmeter.stationsStations in the lightmeter network44stationidIdentifier of the measuring station, starting with an ISO CCmeta.id;meta.maincharindexedprimarylatLatitude of the observing stationdegpos.earth.lat-111.707148.322453.098453.62020.954545doublenullablelongLongitude of the observing stationdegpos.earth.lon-78.789-5.08813.3519133.545139.6440.931818doublenullableheightHeight above sea levelmpos.earth.altitude68.0720215753.7600000.954545floatnullablefullnameFull name of the stationmeta.idchardevtypeDevice type (as in: IYA Lightmeter, SQM, ...)meta.code;instrcharnullabletimecorrectionSeconds to add to this stations reported times to obtain UTC-32400-32400.00.00.001.0intnullablecalibaCalibration parameter, ainstr.calib1011801071421248542013402110000.545455floatnullablecalibbCalibration parameter, binstr.calib0.0002940980.000342470.005055750.03822060.0456560.545455floatnullablecalibcCalibration parameter, cW.m**-2instr.calib1.4673e-091.55417e-094.79595e-097.63699e-081.20908e-070.545455floatnullablecalibdCalibration parameter, dK**-1instr.calib0.00236970.00236970.00451250.005881180.006353440.545455floatnullableliverpoolThis collection includes optical monitorings of gravitationally lensed quasars. The frames can be used to make light curves of quasar images and field objects. From quasar light curves, one may measure time delays and flux ratios, analyse variability and chromaticity, etc. These direct analyses/measurements are basic tools for different astrophysical studies, e.g., expansion rate of the Universe, mechanism of intrinsic variability in quasars, accretion disk structure, supermassive black holes, dark halos of galaxies (dust, collapsed dark matter, smoothly distributed dark matter,...)liverpool.rawframesThis collection includes optical monitorings of gravitationally lensed quasars. The frames can be used to make light curves of quasar images and field objects. From quasar light curves, one may measure time delays and flux ratios, analyse variability and chromaticity, etc. These direct analyses/measurements are basic tools for different astrophysical studies, e.g., expansion rate of the Universe, mechanism of intrinsic variability in quasars, accretion disk structure, supermassive black holes, dark halos of galaxies (dust, collapsed dark matter, smoothly distributed dark matter,...)561accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size21196802119680.02119680.02122560.021225601.0longnullablecenteralphaApproximate center of image, RAdegpos.eq.ra138.232138.235147.843213.944340.1211doubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.dec3.3726511.495626.597855.895655.91051doubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposure54009.254017.254156.954614.154674.91doublenullablenaxesNumber of axes in datapos.wcs.naxes22.02.02.021.0intnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinox200020002000200020001floatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.median4.71e-074.71e-076.18e-077.49e-077.49e-071floatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.max5.8e-075.8e-077.2e-078.6e-078.6e-071floatnullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.min3.65e-073.65e-075.4e-076.45e-076.45e-071floatnullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablecreation_dateDate of FITS file creationdtime.creationcharnullabletypeType of the observation (Science, Flat...)meta.code.classcharobjectObject observed, Simbad resolvable identifiermeta.idcharnullableraw_objectObject observed as given in the headermeta.idcharnullableobservatoryObservatory of origin for this framemeta.id;instr.obstycharnullabletelescopeTelescope used to obtain the frameinstr.telcharnullableinstrumentIdentifier of the originating instrumentcharnullabledetectorDetector usedmeta.id;instrcharnullableexposureExposure timestime.duration;obs.exposure1001001203003001floatnullableairmassAir mass at center of observationobs.airMass1.020671.04511.452.122.628361floatnullablemoonfracFraction of illuminated area of the moon at obs. timeobs.param;arith.ratio0.00036590.001574740.4467480.9978770.99981floatnullablemoondistLunar distance from targetdegpos.angDistance30.303434.147690.9128164.078169.8221floatnullablel1satIs the brightest object in the field saturated?instr.saturation;stat.maxbooleanbackgroundBackground in countsct.s**-1instr.background98.176111.519418.6557400.59205261floatnullableseeingEstimate for seeing at observation timearcsecinstr.obsty.seeing0.6147190.9027121.49773.75204278.0921floatnullablestarttimeUT at start of observationtime.startcharnullablelspm The LSPM catalog is a comprehensive list of 61,977 stars north of the J2000 celestial equator that have proper motions larger than 0.15"/yr (local-background-stars frame). Positions are given with an accuracy of <~100 mas at the 2000.0 epoch, and absolute proper motions are given with an accuracy of ~8 mas/yr. The catalog is estimated to be over 99% complete at high Galactic latitudes (|b|>15{deg}) and over 90% complete at low Galactic latitudes (|b|>15{deg}), down to a magnitude.lspm.main The LSPM catalog is a comprehensive list of 61,977 stars north of the J2000 celestial equator that have proper motions larger than 0.15"/yr (local-background-stars frame). Positions are given with an accuracy of <~100 mas at the 2000.0 epoch, and absolute proper motions are given with an accuracy of ~8 mas/yr. The catalog is estimated to be over 99% complete at high Galactic latitudes (|b|>15{deg}) and over 90% complete at low Galactic latitudes (|b|>15{deg}), down to a magnitude.61977idLSPM star namemeta.id;meta.maincharnullableraj2000Right Ascension (J2000, Ep=J2000)degpos.eq.ra;meta.main0.0156819.569181.188350.114359.9931doubleindexednullabledej2000Declination (J2000, Ep=J2000)degpos.eq.dec;meta.main0.0003621.7601230.092576.301289.68731doubleindexednullablepmTotal Proper Motiondeg/yrpos.pm2.38889e-054.27778e-055.5e-050.0001469440.002863331floatnullablepmraProper Motion in Right Ascensiondeg/yrpos.pm;pos.eq.ra-0.00122722-8.72222e-05-1.38889e-068.63889e-050.001154171floatnullablepmdeProper Motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.00161472-0.000105833-3.36111e-055.30556e-050.002854721floatnullableaflagAstrometry sourcemeta.refcharnullablebmagOptical B magnitudemagphot.mag;em.opt.B05.640811.7115.9417.160.189086floatnullablevmagOptical V magnitudemagphot.mag;em.opt.V06.105410.9214.515.510.189086floatnullablebjmagPhotographic Blue (IIIaJ) magnitudemagphot.mag;em.opt.B08.917.420.925.20.974684floatnullablerfmagPhotographic Red (IIIaF) magnitudemagphot.mag;em.opt.R-0.48.115.419.120.70.988496floatnullableinmagPhotographic Infrared (IVN) magnitudemagphot.mag;em.opt.R-0.77.713.817.923.10.939429floatnullablejmag2MASS J magnitudemagphot.mag;em.ir.J-2.257.0112.5116.1617.410.963002floatnullablehmag2MASS H magnitudemagphot.mag;em.ir.H-2.816.6111.9515.6527.770.963002floatnullablekmag2MASS K_s magnitudemagphot.mag;em.ir.K-3.046.5111.7215.427.770.96297floatnullablevmag_eEstimated V magmagphot.mag;em.opt.V08.5716.4920.1399.91floatnullablemaidanakObservations of (mainly) lensed quasars from Maidanak Observatory, Uzbekhistanmaidanak.reduced Reduced frames of lensed quasar observations from Maidanak Observatory. See the referenceURL for details on the reduction procedure and calibration data.accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.SizelongnullablecenteralphaApproximate center of image, RAdegpos.eq.radoubleindexednullablecenterdeltaApproximate center of image, Decdegpos.eq.decdoubleindexednullableimagetitleSynthetic name of the imagemeta.titlecharnullableinstidIdentifier of the originating instrumentmeta.id;instrcharnullabledateobsEpoch at midpoint of observationdtime;obs.exposuredoubleindexednullablenaxesNumber of axes in datapos.wcs.naxesintnullablepixelsizeNumber of pixels along each of the axespixelpos.wcs.naxisintnullablepixelscaleThe pixel scale on each image axisdeg/pixelpos.wcs.scalefloatnullablerefframeCoordinate system reference framepos.framecharnullablewcs_equinoxEquinox of the given coordinatesyrtime.equinoxfloatnullablewcs_projectionFITS WCS projection typepos.wcs.ctypecharnullablewcs_refpixelWCS reference pixelpixelpos.wcs.crpixfloatnullablewcs_refvaluesWorld coordinates at WCS reference pixeldegpos.wcs.crvaldoublenullablewcs_cdmatrixFITS WCS CDij matrixdeg/pixelpos.wcs.cdmatrixfloatnullablebandpassidFree-form name of the bandpass usedinstr.bandpasscharnullablebandpassunitUnit of bandpass specifications (always m).charnullablebandpassrefvalCharacteristic quantity for the bandpass of the imageminstr.bandpass;stat.medianfloatnullablebandpasshiUpper limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.maxfloatindexednullablebandpassloLower limit of the bandpass (in BandPass_Unit units)minstr.bandpass;stat.minfloatindexednullablepixflagsFlags specifying the processing done (C-original; F-resampled; Z-fluxes valid; X-not resampled; V-for display onlymeta.codecharnullablecoverageField covered by the imagedegdoubleindexednullablefilenameFile name as supplied by the observatory -- unreliablemeta.idchartypeType of observation (science, flat, bias, calib...)meta.code.classcharobjectObject being observed, Simbad-resolvable formmeta.id;meta.maincharnullableraw_objectTarget object as supplied by the observatorymeta.idcharnullableobservatoryObservatory the image was obtained atmeta.id;instr.obstycharnullabletelescopeTelescope used to obtain the imageinstr.telcharnullableinstrumentIdentifier of the detecting instrumentinstr.setupcharnullabledetectorInternal detector IDmeta.id;instr.detcharnullableexposureExposure timestime.duration;obs.exposurefloatnullablestarttimeStart of exposure in UTtime.startcharnullableendtimeEnd of exposure in UTtime.endcharnullablechipidDetector Chipmeta.id;instr.detcharnullablep_dewarDewar Pressure (unreliable)phys.pressure;instr.paramfloatnullableari_rawRaw object name assigned at ARImeta.idcharnullablepub_didPublisher dataset Identifiermeta.ref.ivoidcharnullablemlqso An archive of optical and near-infrared spectra of strongly lensed quasars and the lensing galaxies. The spectra are resolved to about a few Ångstroms and are flux-calibrated. The spectra resulted from deblending the lensed images in bidimensional spectra available from the SSAP service for `ivo://org.gavo.dc/mlqso/q/s <http://dc.g-vo.org/mlqso/q/s/info>`_.mlqso.cubes Bidirectional spectra as FITS image.12accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Sizelongnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent0107206960934800.00296283floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime-6146.555450.156458.35814959214.20.620126doublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime-6146.5562865762658738.163023.50.620108doublenullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c1020.1413209.025341.7143600.982073doublenullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-89.9161-63.4054-18.958256.480589.9880.982073doublenullabledatalinkDatalinks (related data, cutouts, etc) for this datasetmeta.ref.urlcharnullablemlqso.slitspectra Bidimensional spectra of galaxies lensing QSOs.832accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size319680319680.0406080.0443520.04435201.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpasscharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharindexedssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshift1.1231.1231.6784.4264.4261floatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNR1001001001001001floatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value53304533045356953969539691doublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent1399.931399.931399.931399.931399.931floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Value1.64494e-071.64493e-072.09954e-072.2865e-072.2865e-071floatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extent3.28987e-073.28987e-074.19909e-074.573e-074.573e-071floatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start4.26e-074.26e-074.35e-074.96e-074.96e-071floatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop8.04875e-078.04875e-078.55003e-078.869e-078.869e-071floatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Length12241224.01562.01701.017011.0intnullableremarkRemarks on the data set by the data creator.meta.notecharnullableonebigb This catalog presents the 1-100 GeV spectral energy distribution (SED) for a population of 148 high-synchrotron-peaked blazars (HSPs) recently detected with Fermi-LAT as part of the First Brazil-ICRANet Gamma-ray Blazar catalogue (1BIGB). A series of two works describe details on the broadband analysis: :bibcode:`2017A&A...598A.134A`, and the calculation of the gamma-ray SEDs :bibcode:`2018MNRAS.480.2165A`. The 1BIGB sample was originally selected from an excess signal in the 0.3-500 GeV band The flux estimates presented here are derived considering PASS8 data, integrating over more than 9 years of Fermi-LAT observations. The full broadband fit between 0.3-500 GeV presented in paper 1 for all sources was reevaluated in paper 2, updating the power-law parameters with currentlyonebigb.measurementsA table of raw measurement points. See the seds table for combined SEDs.1329idDatapoint IDmeta.id;meta.mainintiauidIAU-compliant identifier of the Blazarmeta.idcharnullableraRight Ascensiondegpos.eq.ra;meta.maindoublenullabledecDeclinationdegpos.eq.dec;meta.maindoublenullablefrequencyFlux measurement frequencyHzem.freqfloatnufnunuFnu Fluxerg.cm**-2.s**-1phot.fluxfloatnufnu_errornuFnu Flux errorerg.cm**-2.s**-1stat.error;phot.fluxfloatupper_limitFlux upper limitmeta.codecharnullableonebigb.ssaSSA-compliant table of SEDs constructed within 1BIGB.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassGamma-raycharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.ClassBlazarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.freqcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitHzcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.fluxcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Uniterg.cm**-2.s**-1charssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collection1BIGBcharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.Instrumentcharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcepointedcharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypecharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationABSOLUTEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperturedoubleindexednullablefrequencyFlux measurement frequencyHzem.freqfloatnufnunuFnu Fluxerg.cm**-2.s**-1phot.fluxfloatnufnu_errorError in nuFnu; a zero here indicates an upper limiterg.cm**-2.s**-1stat.error;phot.fluxfloatplc2 From the Gaia DR2 catalogue we predict astrometric microlensing events by foreground stars with high proper motion (µ_tot >150mas/yr) passing a background source in the next decades. Using Gaia DR2 photometry we determine an approximate mass of the lens, which we use to calculate the expected microlensing effects. This yields 3914 microlensing events by 2875 different lenses between 2010 and 2065 with expected shifts larger than 0.1 mas between the lensed and unlensed positions of the source. 513 of those are expected to happen between 2014.5 - 2026.5 and might be measured by Gaia. For 127 events we also expect a magnification between 1 mmag and 3 mag.plc2.dataThe final candidate table for astrometric microlensing events predicted from Gaia DR2. This has estimates of minimal distances, epochs, etc. Columns prefixed with lens_ are for the lens, columns prefixed with ob_ are for the lensed object.3914event_idUnique identifier of this event. This is the decimal representation of the Gaia DR2 source_id of the lens, and a disambiguator for the lensed object.meta.id;meta.maincharindexedprimarylens_idGaia DR2 source_id of the lens.meta.id225799530407285764.170184671489307e+174.524048089080652e+186.657800844699378e+1869166447797744936961.0longlens_raGaia DR2 RA of the lensdegpos.eq.ra;meta.main0.54830726.5858248.251335.035359.9731doubleindexednullablelens_decGaia DR2 Declication of the lensdegpos.eq.dec;meta.main-88.0806-70.1382-27.896961.732884.33381doubleindexednullablelens_err_raError of lens__ra from Gaia DR2degstat.error;pos.eq.ra;meta.main3.26422e-095.27607e-091.47986e-081.68696e-077.85181e-071floatnullablelens_err_decError of lens__dec from Gaia DR2degstat.error;pos.eq.dec;meta.main3.16569e-095.62946e-091.34019e-081.71019e-075.04639e-071floatnullablelens_pmraProper motion in RA of the lens from Gaia DR2deg/yrpos.pm;pos.eq.ra-0.00105036-0.000451125-2.34289e-050.0005414360.001803191floatnullablelens_pmdecProper motion in Declination of the lens from Gaia DR2deg/yrpos.pm;pos.eq.ra-0.00161607-0.000370206-4.58556e-050.0003663380.002878471floatnullablelens_err_pmraError of lens_pmra from Gaia DR2deg/yrpos.pm;pos.eq.ra6.50797e-091.10549e-082.84367e-083.70681e-071.07382e-061floatnullablelens_err_pmdecError of lens_pmdec from Gaia DR2deg/yrpos.pm;pos.eq.dec5.33081e-091.11704e-082.61823e-083.34841e-079.10603e-071floatnullablelens_parallaxParallax of the lens from Gaia DR2degpos.parallax4.82628e-071.23813e-066.75017e-060.000152070.0002134721floatnullablelens_err_parallaxStandard error of the parallax the lens from Gaia DR2degstat.error;pos.parallax3.93094e-097.284e-091.77209e-082.08635e-077.63231e-071floatnullablelens_phot_g_mean_magMean magnitude of the lens in the integrated G band from Gaia DR2.magphot.mag;em.opt.V2.655925.3827312.755719.424420.71081floatnullablelens_phot_rp_mean_magMean magnitude of the lens in the integrated RP band from Gaia DR2.magphot.mag;em.opt.R2.431954.5875911.587418.19419.91550.978794floatnullablelens_phot_bp_mean_magMean magnitude of the lens in the integrated BP band from Gaia DR2.magphot.mag;em.opt.B3.667645.8326813.865819.94222.18110.978539floatnullableob_idGaia DR2 source_id of the lensed object.meta.id225799487457216004.170196195730165e+174.5240480890788644e+186.657800847317848e+1869166447840705996801.0longob_raGaia DR2 RA of the lensed objectdegpos.eq.ra0.55214726.5862248.244335.033359.9721doublenullableob_decGaia DR2 Declication of the lensed objectdegpos.eq.dec-88.0796-70.1323-27.897161.724584.33361doublenullableob_err_raError of ob__ra from Gaia DR2degstat.error;pos.eq.ra2.395e-099.33263e-091.271e-071.36619e-062.75684e-061floatnullableob_err_decError of ob__dec from Gaia DR2degstat.error;pos.eq.dec3.26394e-099.87225e-091.20198e-071.2051e-062.60586e-061floatnullableob_pmraProper motion in RA of the lensed object from Gaia DR2deg/yrpos.pm;pos.eq.ra-8.21525e-06-3.34887e-06-7.64003e-071.75717e-062.09543e-050.729177floatnullableob_pmdecProper motion in Declination of the lensed object from Gaia DR2deg/yrpos.pm;pos.eq.ra-2.84144e-05-3.5915e-06-7.80647e-071.74456e-061.12712e-050.729177floatnullableob_err_pmraError of ob_pmra from Gaia DR2deg/yrpos.pm;pos.eq.ra5.03869e-091.63113e-081.72199e-078.12211e-071.37284e-060.729177floatnullableob_err_pmdecError of ob_pmdec from Gaia DR2deg/yrpos.pm;pos.eq.dec6.76228e-091.57175e-081.64055e-077.67711e-071.30854e-060.729177floatnullableob_parallaxParallax of the lensed object from Gaia DR2degpos.parallax-1.42986e-06-3.69772e-078.65674e-086.50024e-073.08697e-060.729177floatnullableob_err_parallaxStandard error of the parallax the lensed object from Gaia DR2degstat.error;pos.parallax3.77422e-091.06159e-081.08427e-074.46462e-071.03184e-060.729177floatnullableob_phot_g_mean_magMean magnitude of the lensed object in the integrated G band from Gaia DR2.magphot.mag;em.opt.V3.3952513.121619.337520.969721.33561floatnullableob_phot_rp_mean_magMean magnitude of the lensed object in the integrated RP band from Gaia DR2.magphot.mag;em.opt.R2.8196913.191218.036819.719720.47510.731477floatnullableob_phot_bp_mean_magMean magnitude of the lensed object in the integrated BP band from Gaia DR2.magphot.mag;em.opt.B4.1946614.725519.520221.294123.080.730199floatnullablestar_typeType of the lensing star: WD = White Dwarf, MS = Main Sequence, RG = Red Giant, BD = Brown Dwarfsrc.classcharnullablemassEstimated mass of the lens from Gaia DR2solMassphys.mass0.070.08194090.418691.148722.075721floatnullableerr_massError in the mass of the lens from Gaia DR2solMassstat.error;phys.mass0.007152850.01164650.0418690.150.51floatnullabletheta_eEinstein radius of the eventmasphys.angsize1.338233.158739.2560332.254639.31641doublenullableerr_theta_eError in the Einstein radius of the eventmasstat.error;phys.angsize0.1419620.1817240.5319141.964674.041471floatnullabletime_scaleApproximate duration of the eventyrtime.duration0.109410.4656563.2832115.525943.72370.98186doublenullabletcaEstimated time of the closest approach.yrtime.epoch2009.792012.352043.562064.682068.281doublenullableerr_tcaError in tca.yrstat.error;time.epoch0.0001551080.001681380.07975071.671933.111961floatnullabledistEstimated distance at closest approach.maspos.angdistance0.066591311.7639359.584668.886803.521floatnullableerr_distError d_min.masstat.error;pos.angdistance0.2354462.1779829.2177437.186646.6361floatnullableuEstimated distance at closest approach in Einstein radii.0.004003592.1754141.6963170.28246.4131doublenullableerr_uError in u.0.2503471.005896.1008356.3488178.5591floatnullableshiftMaximal astrometric shift of the center of light.maspos;arith.diff0.100050.103730.2059072.221858.966591doublenullableerr_shiftError in shiftmasstat.error;pos;arith.diff0.007083840.007949440.03708484.329852545.551floatnullableshift_lumMaximal astrometric shift including lens-luminosity effects.maspos;arith.diff5.08683e-088.24668e-070.001164050.2363542.172421doublenullableerr_shift_lumError in shift_lum.masstat.error;pos;arith.diff3.81168e-097.05359e-080.000244870.24555631.1871floatnullableshift_plusMaximal astrometric shift of brighter image.maspos;arith.diff0.1001180.1037420.2059732.9655318.31541doublenullableerr_shift_plusError in shift_plus.masstat.error;pos;arith.diff0.007084270.007951760.03721585.88048210.3461floatnullablemagnificationMaximal magnification.magphot.mag;arith.ratio4.82164e-163.17698e-146.04644e-090.001078133.148881doublenullableerr_magnificationError in magnification.magstat.error;phot.mag;arith.ratio1.5662e-168.18147e-153.65579e-090.00797008377.5951floatnullablel2_tcaEstimated time of the closest approachas seen from Earth-Sun L2 point.yrtime.epoch2009.792012.352043.572064.682068.281doublenullablel2_err_tcaError in l2_tca.yrstat.error;time.epoch0.0001558890.001683770.07993441.671953.111951floatnullablel2_distEstimated distance at closest approachas seen from Earth-Sun L2 point.maspos.angdistance0.0018486411.7662359.4724666.816803.031floatnullablel2_err_distError l2_d_min.masstat.error;pos.angdistance0.2355062.1812729.2239437.6651.011floatnullablel2_uEstimated distance at closest approach in Einstein radiias seen from Earth-Sun L2 point.0.0002600742.190141.6752170.195246.3511doublenullablel2_err_uError in l2_u.0.2513551.01296.1016156.3487178.5591floatnullablel2_shiftMaximal astrometric shift of the center of lightas seen from Earth-Sun L2 point.maspos;arith.diff0.100050.1037570.2059542.223238.851581doublenullablel2_err_shiftError in l2_shiftmasstat.error;pos;arith.diff0.007084290.007953810.03712644.2150317706.41floatnullablel2_shift_lumMaximal astrometric shift including lens-luminosity effectsas seen from Earth-Sun L2 point.maspos;arith.diff5.08895e-088.24872e-070.001164420.235952.172421doublenullablel2_err_shift_lumError in l2_shift_lum.masstat.error;pos;arith.diff3.81396e-097.05517e-080.0002452210.25003331.27211floatnullablel2_shift_plusMaximal astrometric shift of brighter imageas seen from Earth-Sun L2 point.maspos;arith.diff0.1001180.1037980.206022.963918.10811doublenullablel2_err_shift_plusError in l2_shift_plus.masstat.error;pos;arith.diff0.007084720.007956140.03727015.92609209.8681floatnullablel2_magnificationMaximal magnificationas seen from Earth-Sun L2 point.magphot.mag;arith.ratio4.82164e-163.17698e-146.03769e-090.00107154.15831doublenullablel2_err_magnificationError in l2_magnification.magstat.error;phot.mag;arith.ratio1.56681e-168.19186e-153.66356e-090.007723317485.561floatnullableppmxPPM-Extended (PPMX) is a catalogue of 18 088 919 stars on the ICRS system containing astrometric and photometric information. Its limiting magnitude is about 15.2 in the GSC photometric system.ppmx.dataPPM-Extended (PPMX) is a catalogue of 18 088 919 stars on the ICRS system containing astrometric and photometric information. Its limiting magnitude is about 15.2 in the GSC photometric system.19000000alphafloatMain value of right ascensiondegpos.eq.ra;meta.main0.00013555615.7176189.961345.893601doubleindexednullabledeltafloatMain value of declinationdegpos.eq.dec;meta.main-89.9473-71.8887-0.65687970.436889.961doubleindexednullablec_xx coordinate of intersection of radius vector and unit spherepos.cartesian.x-0.999998-0.874438-0.009660210.88264211floatnullablec_yy coordinate of intersection of radius vector and unit spherepos.cartesian.y-1-0.950209-0.04542640.95582211floatnullablec_zz coordinate of intersection of radius vector and unit spherepos.cartesian.z-1-0.950454-0.01146450.94227211floatnullablelocalidName (IAU convention HHMMSS.s+DDMMSS), p or f appended to desambiguatemeta.id;meta.maincharindexedprimarypmraProper Motion in RA*cos(delta)arcsec/yrpos.pm;pos.eq.ra-3.63374-0.03909-0.001890.035434.138131floatnullablepmdeProper Motion in Decarcsec/yrpos.pm;pos.eq.dec-4.7715-0.04416-0.003210.0300610.3281floatnullableraerrMean error in RA*cos(DEmas) at epRAmasstat.error;pos.eq.ra11519771801floatnullabledecerrMean error in DE at epDEmasstat.error;pos.eq.dec11519771801floatnullablepmraerrMean error in pmRA*cos(DEmas)arcsec/yrstat.error;pos.pm;pos.eq.ra0.00020.00140.01030.02210.08921floatnullablepmdeerrMean error in pmDEarcsec/yrstat.error;pos.pm;pos.eq.ra0.00010.00140.01020.02210.08921floatnullableepraMean Epoch (RA)yrtime.epoch;pos.eq.racharnullableepdeMean Epoch (Dec)yrtime.epoch;pos.eq.deccharnullablecmagCatalogue magnitude from sourcemagphot.mag-1.510.3813.7715.4617.021floatindexednullablermagcalculated Ru magnitude from sourcemagphot.mag;em.opt.R-1.83710.05513.48915.45217.6990.998326floatnullablebmagB magnitude in Johnson systemmagphot.mag;em.opt.B-1.439.10211.97613.33217.0630.134226floatnullablee_bmagStandard error on B magnitudemagstat.error;phot.mag;em.opt.B00.0150.1360.4110.9970.134226floatnullablevmagV magnitude in Johnson systemmagphot.mag;em.opt.V-1.1218.4514811.27412.63715.9780.135808floatindexednullablee_vmagStandard error on V magnitudemagstat.error;phot.mag;em.opt.V0.0010.0130.1010.2460.9430.135808floatnullablejmagJ magnitude in Johnson systemmagphot.mag;em.IR.J-2.9898.42512.1314.10916.8280.998326floatnullablee_jmagStandard error on J magnitudemagstat.error;phot.mag;em.IR.J0.0140.020.0240.0390.9990.993077floatnullablehmagH magnitude in Johnson systemmagphot.mag;em.IR.H-4.0077.81111.76813.76917.7330.998327floatnullablee_hmagStandard error on H magnitudemagstat.error;phot.mag;em.IR.H00.0180.0260.0530.9990.998324floatnullablekmagK magnitude in Johnson systemmagphot.mag;em.IR.K-4.3787.62111.68413.68517.1680.998327floatnullablee_kmagStandard error on K magnitudemagstat.error;phot.mag;em.IR.K00.0170.0240.0530.9990.998323floatnullablen_obsnumber of observations in LSQ fitmeta.number;obs22.04.07.0160.9925215intnullablep_flagTrue if LSQ fit is badmeta.code.qualbooleansub_flagSubset flagmeta.codecharnullablesrccatSource cataloguemeta.refcharnullablesrcidStar identifier in the source cataloguemeta.id.crosscharnullablepm_totalTotal proper motionarcsec/yrpos.pm00.002534030.01453370.079658610.3591floatindexednullableangle_pmPosition angle of total proper motiondegpos.posAng;pos.pm-179.997-172.428-33.0721172.2441801floatnullablesdssdr7 This is the result of the query:: select objID, field.run, field.rerun, field.camcol, field.fieldId, obj, ra, dec, raErr, decErr, raDecCorr, offsetRa_u, offsetRa_g, offsetRa_r, offsetRa_i, offsetRa_z, offsetDec_u, offsetDec_g, offsetDec_r, offsetDec_i, offsetDec_z, u, g, r, i, z, err_u, err_g, err_r, err_i, err_z, mjd_u, mjd_g, mjd_r, mjd_i, mjd_z from PhotoObjAll join field on (field.fieldId=PhotoObjAll.fieldId) on SDSS DR7, kindly provided by the Potsdam mirror. All angular quantities are given in degrees here.sdssdr7.sources This is the result of the query:: select objID, field.run, field.rerun, field.camcol, field.fieldId, obj, ra, dec, raErr, decErr, raDecCorr, offsetRa_u, offsetRa_g, offsetRa_r, offsetRa_i, offsetRa_z, offsetDec_u, offsetDec_g, offsetDec_r, offsetDec_i, offsetDec_z, u, g, r, i, z, err_u, err_g, err_r, err_i, err_z, mjd_u, mjd_g, mjd_r, mjd_i, mjd_z from PhotoObjAll join field on (field.fieldId=PhotoObjAll.fieldId) on SDSS DR7, kindly provided by the Potsdam mirror. All angular quantities are given in degrees here.590000000objidUnique SDSS identifier composed from [skyVersion,rerun,run,camcol,field,obj].meta.id;meta.main5877229516933038245.877255522646106e+175.877425909451995e+177.588848214521307e+177588873699775621751.0longrunRun numbermeta.id;obs7451239.04520.06709.072651.0shortrerunRerun numbermeta.id;obs4040.040.0648.06481.0shortcamcolCamera columnmeta.id;instr11.03.06.061.0shortfieldidField numbermeta.id;obs.field5877229516933038085.877255522646098e+175.877425909451981e+177.588848214521283e+177588873699775610881.0longobjThe object id within a field. Usually changes between reruns of the same field.meta.id142.0687.03676.0140851.0shortraJ2000 right ascension (r')degpos.eq.ra;meta.main1.423e-0524.6837195.68343.6593601doubleindexednullabledecJ2000 declination (r')degpos.eq.dec;meta.main-24.185-10.649422.179864.336584.97911doubleindexednullableraerrError in RAdegstat.error;pos.eq.ra;meta.main1.71543e-069.98489e-062.51993e-058.38383e-051.212341floatnullabledecerrError in Decdegstat.error;pos.eq.dec;meta.main1.79947e-069.84014e-062.40708e-058.1806e-051.093491floatnullableradeccorrRA/dec correlationstat.correlation;pos.eq.ra;pos.eq.dec-1-0.34570300.3626311floatnullableoffsetra_uFilter position RA minus final RA, cos(dec) applieddegpos.eq.ra;arith.diff-0.181639-7.28694e-052.34722e-067.47889e-050.1786371floatnullableoffsetdec_uFilter position Dec minus final Decdegpos.eq.dec;arith.diff-0.19449-7.38333e-05-9.44444e-077.46139e-050.217441floatnullableuMagnitude in u band, better of deVaucouleurs and exponential fitsmagphot.mag;em.opt.U5.9145117.479723.380226.219134.90040.961051floatnullableerr_uError in corresponding magnitudemagstat.error;phot.mag;em.opt.U1.04835e-060.01108820.7130852.12721841.830.961051floatnullableepoch_uDate of observation in u bandyrtime.epoch1999.212000.172004.212007.120081floatnullableoffsetra_gFilter position RA minus final RA, cos(dec) applieddegpos.eq.ra;arith.diff-0.181615-9.60083e-052.43611e-069.73722e-050.1401541floatnullableoffsetdec_gFilter position Dec minus final Decdegpos.eq.dec;arith.diff-0.211201-9.57528e-056.13889e-079.60861e-050.2040381floatnullablegMagnitude in g band, better of deVaucouleurs and exponential fitsmagphot.mag;em.opt.V4.4999715.962722.553125.497437.05350.958441floatnullableerr_gError in corresponding magnitudemagstat.error;phot.mag;em.opt.V1.55949e-070.003862440.1634730.818601726.0390.958441floatnullableepoch_gDate of observation in g bandyrtime.epoch1999.212000.172004.212007.120081floatnullableoffsetra_rFilter position RA minus final RA, cos(dec) applieddegpos.eq.ra;arith.diff000001floatnullableoffsetdec_rFilter position Dec minus final Decdegpos.eq.dec;arith.diff000001floatnullablerMagnitude in r band, better of deVaucouleurs and exponential fitsmagphot.mag;em.opt.R4.2207815.313221.495124.85134.81080.963678floatnullableerr_rError in corresponding magnitudemagstat.error;phot.mag;em.opt.R1.66783e-070.003686470.09486080.701801773.0090.963678floatnullableepoch_rDate of observation in r bandyrtime.epoch1999.212000.172004.212007.120081floatnullableoffsetra_iFilter position RA minus final RA, cos(dec) applieddegpos.eq.ra;arith.diff-0.158773-9.55278e-05-1.02778e-078.8225e-050.1468671floatnullableoffsetdec_iFilter position Dec minus final Decdegpos.eq.dec;arith.diff-0.187484-9.89139e-05-6.66667e-088.74111e-050.1922641floatnullableiMagnitude in i band, better of deVaucouleurs and exponential fitsmagphot.mag;em.opt.I3.2760215.042820.835824.364835.85230.962304floatnullableerr_iError in corresponding magnitudemagstat.error;phot.mag;em.opt.I8.08271e-080.003824780.08224490.685265909.2440.962304floatnullableepoch_iDate of observation in i bandyrtime.epoch1999.212000.172004.212007.120081floatnullableoffsetra_zFilter position RA minus final RA, cos(dec) applieddegpos.eq.ra;arith.diff-0.168936-8.1425e-053.83333e-078.29917e-050.1715251floatnullableoffsetdec_zFilter position Dec minus final Decdegpos.eq.dec;arith.diff-0.194483-7.96583e-05-1.55556e-078.19889e-050.1841421floatnullablezMagnitude in z band, better of deVaucouleurs and exponential fitsmagphot.mag;em.opt.I4.7150514.768620.36923.225833.90950.960365floatnullableerr_zError in corresponding magnitudemagstat.error;phot.mag;em.opt.I3.89903e-070.005155930.1906041.050791206.490.960365floatnullableepoch_zDate of observation in z bandyrtime.epoch1999.212000.172004.212007.120081floatnullablespm4 The SPM4 Catalog contains absolute proper motions, celestial coordinates, and B,V photometry for 103,319,647 stars and galaxies between the south celestial pole and -20 degrees declination. The catalog is roughly complete to V=17.5. It is based on photographic and CCD observations taken with the Yale Southern Observatory's double-astrograph at Cesco Observatory in El Leoncito, Argentina.spm4.main The SPM4 Catalog contains absolute proper motions, celestial coordinates, and B,V photometry for 103,319,647 stars and galaxies between the south celestial pole and -20 degrees declination. The catalog is roughly complete to V=17.5. It is based on photographic and CCD observations taken with the Yale Southern Observatory's double-astrograph at Cesco Observatory in El Leoncito, Argentina.110000000spmidUnique SPM4 id (field number + input catalog line number)meta.id;meta.maincharindexednullableraj2000Right Ascension (ICRS, epoch=2000.0)degpos.eq.ra;meta.main0.000267373.4763219.67309.4143601doubleindexednullabledej2000Declination (ICRS, epoch=2000.0)degpos.eq.dec;meta.main-89.8786-74.8567-47.6455-21.7063-201doubleindexednullablee_raj2000Expected uncertainty in Right Ascension at mean epochdegstat.error;pos.eq.ra;meta.main02.77778e-061.90833e-055.41667e-050.0001810281floatnullablee_dej2000Expected uncertainty in Declination at mean epochdegstat.error;pos.eq.dec;meta.main2.77778e-082.77778e-061.90278e-055.43056e-050.0001891floatnullablepmraAbsolute proper motion in RA (mu_alpha*cos(Dec))deg/yrpos.pm;pos.eq.ra-0.00276335-8.41944e-06-6.83333e-077.55833e-060.002777851floatnullablepmdeAbsolute proper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.00277242-8.27222e-06-7.5e-087.21944e-060.002778511floatnullablee_pmraExpected uncertainty in proper motion in RA (mu_alpha*cos(Dec)), at mean epochdeg/yrstat.error;pos.pm;pos.eq.ra1.02778e-073.69444e-071.13333e-064.06389e-062.70722e-051floatnullablee_pmdeExpected uncertainty in proper motion in Declination, at mean epoch.deg/yrstat.error;pos.pm;pos.eq.dec6.94444e-083.77778e-071.14444e-064.14722e-069.10195e-051floatnullablemagbB magnitudemagphot.mag;em.opt.B013.3817.6219.92300.999842floatnullablemagvV magnitudemagphot.mag;em.opt.V013.2116.918.6300.999984floatindexednullablei_magbsource flag for B magnitudemeta.code;phot.mag;em.opt.Bchari_magvsource flag for V magnitudemeta.code;phot.mag;em.opt.VcharmeanepWeighted mean epochyrtime.epoch1965.721972.781991.052006.2720071floatnullableep1Weighted mean epoch of first observationyrtime.epoch1965.51966.391969.011973.281981.691floatnullableep2Weighted mean epoch of second observationyrtime.epoch1987.581989.342007200720071floatnullablenplates1Number of 1st epoch plates usedmeta.number;instr.plate11.04.010.01611.0shortnplates2Number of 2nd epoch plates usedmeta.number;instr.plate00.00.04.091.0shortnccd2Number of 2nd epoch ccd frames usedmeta.number00.01.05.091.0shorti_galGalaxy/extended-source flagsrc.class.starGalaxy00.00.00.031.0shorti_catCode for the input catalogmeta.code13.04.04.071.0shortmagjJ selected default magnitude from 2MASSmagphot.mag;em.IR.J0.16111.02914.7816.51418.8980.998479floatnullablemaghH selected default magnitude from 2MASSmagphot.mag;em.IR.H0.19210.32414.316.08920.4140.998378floatnullablemagkK_s selected default magnitude from 2MASSmagphot.mag;em.IR.K0.17110.08614.1716.12919.7170.998497floatnullablesupercosmos The SuperCOSMOS data primarily originate from scans of the UK Schmidt and Palomar POSS II blue, red and near-IR sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide an early (1st) epoch red measurement. Mirrored here is the source table containing four-plate multi-colour, multi-epoch data which are merged into a single source catalogue for general science exploitation. Within the GAVO DC, some column names have been adapted to local customs (primarily positions, proper motions).supercosmos.sources The SuperCOSMOS data primarily originate from scans of the UK Schmidt and Palomar POSS II blue, red and near-IR sky surveys. The ESO Schmidt R (dec < -17.5) and Palomar POSS-I E (dec > -17.5) surveys have also been scanned and provide an early (1st) epoch red measurement. Mirrored here is the source table containing four-plate multi-colour, multi-epoch data which are merged into a single source catalogue for general science exploitation. Within the GAVO DC, some column names have been adapted to local customs (primarily positions, proper motions).1900000000objidSuperCOSMOS identifier of merged sourcemeta.id;meta.main281479271677954281775625383852.44848092832381847.02254900780282753.525371144913322301.0longobjidbobjID for B band detection merged into this objectmeta.id.assoc281479271677954281715500438049.94284172216678249.01692152690261488.216927024462417340.60287184longnullableobjidr1objID for R1 band detection merged into this objectmeta.id.assoc11259042018099231126170491444901.51407847331003175.02536882563501036.025371144913322300.6302184longnullableobjidr2objID for R2 band detection merged into this objectmeta.id.assoc562954248388609563207651856265.8565977905513815.51973636256922457.519741774229013780.61956656longnullableobjidiobjID for I band detection merged into this objectmeta.id.assoc844429225099265844699809496843.0847435703817796.02255106938711949.022556523995976190.5208855longnullableepochEpoch of position (variance weighted mean epoch of available measures)yrtime.epoch1949.881953.031984.91996.872002.861floatnullableraj2000Mean RA, computed from detections merged in this cataloguedegpos.eq.ra;meta.main5.72958e-0716.7712221.967342.7083601doubleindexednullabledej2000Mean Dec, computed from detections merged in this cataloguedegpos.eq.dec;meta.main-89.9977-70.4193-6.4339867.814189.99841doubleindexednullablesigraUncertainty in RA (formal random error not including systematic errors)degstat.error;pos.eq.ra5.72958e-069.74028e-063.15127e-050.0001329260.0002778851floatnullablesigdecUncertainty in Dec (formal random error not including systematic errors)degstat.error;pos.eq.ra6.30254e-069.74028e-063.15127e-050.000131780.0002778851floatnullablepmraProper motion in RA directiondeg/yrpos.pm;pos.eq.ra-1.48739-4.30523e-054.66255e-094.55932e-051.506630.589978floatnullablepmdeProper motion in Dec directiondeg/yrpos.pm;pos.eq.dec-1.48067-4.45538e-05-2.34246e-074.31339e-051.482340.589978floatnullablee_pmraError on proper motion in RA directiondeg/yrstat.error;pos.pm;pos.eq.ra4.97808e-078.45183e-072.61134e-064.16894e-050.1454150.589978floatnullablee_pmdeError on proper motion in Dec directiondeg/yrstat.error;pos.pm;pos.eq.dec5.49934e-078.67452e-072.57763e-064.12364e-050.137570.589978floatnullablechi2Chi-squared value of proper motion solutionstat.fit.chi22.51978e-080.09488611.0931370.88991.06917e+060.455165floatnullablenplatesNo. of plates used for this proper motion measurementmeta.number;obs11.02.04.041.0shortclassmagbB band magnitude selected by B image classmagphot.mag;em.opt.B-31.98815.88820.66722.54828.7550.602872floatindexednullableclassmagr1R1 band magnitude selected by R1 image classmagphot.mag;em.opt.R-30.83214.61419.29720.89726.4940.630218floatnullableclassmagr2R2 band magnitude selected by R2 image classmagphot.mag;em.opt.R-28.6614.64919.44121.25131.9430.619567floatnullableclassmagiI band magnitude selected by I image classmagphot.mag;em.opt.I-32.65613.74518.30920.08732.3680.520886floatindexednullablegcormagbB band magnitude assuming object is galaxymagphot.mag;em.opt.B8.19917.42320.69522.34823.4060.602872floatnullablegcormagr1R1 band magnitude assuming object is galaxymagphot.mag;em.opt.R6.73616.14319.25620.8122.250.630218floatnullablegcormagr2R2 band magnitude assuming object is galaxymagphot.mag;em.opt.R8.22616.22419.56421.2722.6260.619567floatnullablegcormagiI band magnitude assuming object is galaxymagphot.mag;em.opt.I6.06915.02418.41419.99821.190.520886floatnullablescormagbB band magnitude assuming object is starmagphot.mag;em.opt.B-31.34315.79120.70622.66528.7550.602872floatnullablescormagr1R1 band magnitude assuming object is starmagphot.mag;em.opt.R-30.83214.5419.31920.92626.4940.630218floatnullablescormagr2R2 band magnitude assuming object is starmagphot.mag;em.opt.R-31.98714.5819.39421.25431.9430.619567floatnullablescormagiI band magnitude assuming object is starmagphot.mag;em.opt.I-32.2513.70118.26220.17431.870.520886floatnullablemeanclassEstimate of image class based on unit-weighted mean of individual classessrc.class.starGalaxy11.02.02.041.0shortclassbImage classification from B band detectionsrc.class;em.opt.B11.02.02.040.60287184shortnullableclassr1Image classification from R1 band detectionsrc.class;em.opt.R11.02.02.040.6302184shortnullableclassr2Image classification from R2 band detectionsrc.class;em.opt.R11.02.02.040.61956656shortnullableclassiImage classification from I band detectionsrc.class;em.opt.I11.02.02.040.5208855shortnullableellipbEllipticity of B band detectionsrc.ellipticity00.02987060.2335590.6542610.602872floatnullableellipr1Ellipticity of R1 band detectionsrc.ellipticity;em.opt.R00.03295250.2561170.65844610.630218floatnullableellipr2Ellipticity of R2 band detectionsrc.ellipticity;em.opt.R00.03406770.2413790.64374610.619567floatnullableellipiEllipticity of I band detectionsrc.ellipticity;em.opt.I00.03593340.2544520.66207410.520886floatnullablequalbBitwise quality flag from B band detectionmeta.code.qual;em.opt.B00.00.01024.0276640.60287184intnullablequalr1Bitwise quality flag from R1 band detectionmeta.code.qual;em.opt.R00.00.01024.0276640.6302184intnullablequalr2Bitwise quality flag from R2 band detectionmeta.code.qual;em.opt.R00.00.01024.0276640.61956656intnullablequaliBitwise quality flag from I band detectionmeta.code.qual;em.opt.I00.00.01024.0276640.5208855intnullableblendbBlend flag from B band detectionmeta.code.qual;em.opt.B00.00.06.06390.60287184intnullableblendr1Blend flag from R1 band detectionmeta.code.qual;em.opt.R00.00.04.06370.6302184intnullableblendr2Blend flag from R2 band detectionmeta.code.qual;em.opt.R00.00.05.06400.61956656intnullableblendiBlend flag from I band detectionmeta.code.qual;em.opt.I00.00.04.06370.5208855intnullableprfstatbProfile statistic from B band detectionsrc.class.starGalaxy-1000-1.7880.6338.8110000.602872floatnullableprfstatr1Profile statistic from R1 band detectionsrc.class.starGalaxy;em.opt.R-200.631-1.7790.76.96110000.630218floatnullableprfstatr2Profile statistic from R2 band detectionsrc.class.starGalaxy;em.opt.R-1000-1.8270.6177.49210000.619567floatnullableprfstatiProfile statistic from I band detectionsrc.class.starGalaxy;em.opt.R-1000-2.1350.6856.93910000.520886floatnullableebmvThe estimated foreground reddening at this position from Schlegel et al. (1998)magphys.absorption0.0007037530.01389050.1724692.75042156.1361floatnullabletgas This table is a subset of GaiaSource comprising those stars in the Hipparcos and Tycho-2 Catalogues for which a full 5-parameter astrometric solution has been possible in Gaia Data Release 1. This is possible because the early Hipparcos epoch positions break some degeneracies due to the limited Gaia time coverage. This table contains a substantial fraction of the around 2.5 million stars in the Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to several reasons, such as saturation, cross-match errors or bad astrometric solution. All rows have Gaia solution id 1635378410781933568.tgas.main This table is a subset of GaiaSource comprising those stars in the Hipparcos and Tycho-2 Catalogues for which a full 5-parameter astrometric solution has been possible in Gaia Data Release 1. This is possible because the early Hipparcos epoch positions break some degeneracies due to the limited Gaia time coverage. This table contains a substantial fraction of the around 2.5 million stars in the Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to several reasons, such as saturation, cross-match errors or bad astrometric solution. All rows have Gaia solution id 1635378410781933568.2100000source_idUnique source identifiermeta.id;meta.main76278620747522.7821002160144275e+173.7237859862162985e+186.668831054679873e+1869175215372186086401.0longindexedprimaryraBarycentric Right Ascension in ICRS at ref_epochdegpos.eq.ra;meta.main0.00042866515.8353182.89345.9913601doubleindexednullabledecBarycentric Declination in ICRS at ref_epochdegpos.eq.dec;meta.main-89.8897-70.7701-4.7710469.730689.83231doubleindexednullablera_errorStandard error of ra (with cos δ applied).masstat.error;pos.eq.ra0.03532310.1218080.254141.0020419.06271floatnullabledec_errorStandard error of decmasstat.error;pos.eq.dec0.03801270.11230.2333840.93758318.52811floatnullablelGalactic longitude (converted from ra, dec)degpos.galactic.lon0.00036545915.1964197.07347.418359.9991doublenullablebGalactic latitude (converted from ra, dec)degpos.galactic.lat-89.7408-59.6663-0.98220158.064689.89971doublenullablepmraProper motion in right ascension of the source in ICRS at ref_epoch. This is the projection of the proper motion vector in the direction of increasing right ascension.mas/yrpos.pm;pos.eq.ra-3259.36-37.9827-1.8084235.32012890.431doublenullablepmdecProper motion in declination at ref_epoch.mas/yrpos.pm;pos.eq.dec-3159.34-44.9869-2.9297622.77361858.531doublenullablepmra_errorStandard error of pmramas/yrstat.error;pos.pm;pos.eq.ra0.01182640.07837151.133093.8722318.00841floatnullablepmdec_errorStandard error of pmdecmas/yrstat.error;pos.pm;pos.eq.dec0.01269480.06773680.8669483.2961518.85441floatnullableparallaxAbsolute barycentric stellar parallax of the source at the reference epoch ref_epochmaspos.parallax-24.820.201511.779848.26584295.8041floatnullableparallax_errorStandard error of parallaxmasstat.error;pos.parallax0.2039740.2273690.3219730.8624960.9999981floatnullablephot_g_mean_magMean magnitude in the G band. This is computed from the G-band mean flux applying the magnitude zero-point in the Vega scale.magphot.mag;em.opt;stat.mean4.395128.1807711.035312.376519.30791floatnullablephot_g_mean_fluxG-band mean flux as electrons per second.s**-1phot.flux;em.opt;stat.mean306.7361816836248778.66161e+062.83047e+081doublenullablephot_g_mean_flux_errorError on phot_g_mean_fluxs**-1stat.error;phot.flux;em.opt;stat.mean1.0490265.62561029.94103694.35696e+061floatnullablephot_g_n_obsNumber of observations contributing to G photometrymeta.number1150.0115.0269.018661.0shortnullablephot_variable_flagPhotometric variability flagmeta.code;src.varcharnullableref_epochReference epoch to which the astrometic source parameters are referred, expressed as a Julian Year in TCB.yrmeta.ref;time.epoch201520152015201520151doublenullableastrometric_delta_qHipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)stat.value3.77047e-050.09693042.3578439.98120437.80.0456015floatnullableastrometric_excess_noiseExcess noise of the sourcemasstat.value00.2410380.4780171.289565.296921floatnullableastrometric_excess_noise_sigSignificance of excess noisestat.value058.6683220.2231067.431.02922e+241floatnullableastrometric_n_obs_acTotal number of observations ACmeta.number044.099.0252.018711.0shortastrometric_n_obs_alTotal number of observations ALmeta.number1244.099.0254.018781.0shortastrometric_n_bad_obs_acNumber of bad observations ACmeta.number00.04.012.01001.0shortastrometric_n_bad_obs_alNumber of bad observations ALmeta.number00.00.04.0701.0shortastrometric_n_good_obs_acNumber of good observations ACmeta.number042.096.0243.017911.0shortastrometric_n_good_obs_alNumber of good observations ALmeta.number1244.099.0252.018661.0shortastrometric_primary_flagOnly primary sources (for which this flag is True) contribute to the estimation of attitude, calibration, and global parameters. The estimation of source parameters is not affected by primariness.meta.code11.01.01.011.0shortmatched_observationsThe number of observations (detection transits) that have been matched to a given source during the last internal crossmatch revision.meta.number46.015.033.02231.0shortastrometric_priors_usedType of prior used in in the astrometric solution33.05.05.051.0shortnullableastrometric_relegation_factorRelegation factor of the source calculated as per Eq. (118) in 2012A&A...538A..78L used for the primary selection process.arith.factor12.449334.7074912.406950.00961floatnullableastrometric_weight_acMean astrometric weight of the sourcemas**-2stat.weight;stat.mean1.53261e-061.24645e-052.75841e-053.9385e-050.008712820.998931floatnullableastrometric_weight_alMean astrometric weight of the sourcemas**-2stat.weight;stat.mean0.0351490.5869194.1013814.6345205.4751floatnullableduplicated_sourceDuring data processing, this source happened to been duplicated and one source only has been kept.00.00.01.011.0shortra_dec_corrCorrelation between right ascension and declinationstat.correlation-0.999982-0.910318-0.02372160.91570.9999721floatnullablera_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlation-0.999882-0.974559-0.7062460.2889750.9979091floatnullablera_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlation-0.999417-0.919702-0.00684510.9090370.9993831floatnullabledec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlation-0.999119-0.8951080.0006947730.8852080.9992261floatnullabledec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlation-0.999646-0.951697-0.5853950.4865970.9987811floatnullablepmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlation-0.99975-0.962630.007280440.9632550.9997221floatnullablera_parallax_corrCorrelation between right ascension and parallaxstat.correlation-0.998476-0.901085-0.04409620.9056230.9977221floatnullabledec_parallax_corrCorrelation between declination and parallaxstat.correlation-0.996157-0.7410470.1620420.8685810.9979521floatnullableparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlation-0.99835-0.9443230.04760410.9379210.9987621floatnullableparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlation-0.996898-0.913624-0.1604170.7864370.9962621floatnullablescan_direction_mean_k1Mean position angle of scan directions across the sourcedeg-180-165.847-77.5503163.398179.9991floatnullablescan_direction_strength_k1Degree of concentration of scan directions across the source0.0001913880.07712940.3532390.690190.9999851floatnullablescan_direction_mean_k2Mean position angle of scan directions across the sourcedeg-89.9998-82.7701-0.0097433782.680789.99991floatnullablescan_direction_strength_k2Degree of concentration of scan directions across the source9.12868e-050.07295880.3503220.7835670.9999421floatnullablescan_direction_mean_k3Mean position angle of scan directions across the sourcedeg-60-55.8162-7.7615155.644859.99991floatnullablescan_direction_strength_k3Degree of concentration of scan directions across the source0.0002512340.06138910.3211560.7130640.9998691floatnullablescan_direction_mean_k4Mean position angle of scan directions across the sourcedeg-45-43.74340.46108943.6762451floatnullablescan_direction_strength_k4Degree of concentration of scan directions across the source0.0003052650.09603290.515670.9561310.9999931floatnullablerandom_indexRandom index that can be used to deterministically select subsetsmeta.code061777.6599999999961028874.01995274.339999999920570491.0longhipHipparcos identifier13527.859999999999759238.5114982.069999999991204040.045601476intnullabletycho2_idTycho 2 identifiercharnullableucac3The Third US Naval Observatory CCD Astrograph catalogue (UCAC3) is an all-sky catalgoue containing just over 100 million objects covering about R = 8-16 mag. This table contains the original data content of UCAC3 but leaves out the data objetained by crossmatching to other catalogs.ucac3.icrscorrCorrections between UCAC3 and the ICRS as represented by PPMXL on a grid of degrees, obtained by substracting UCAC3 from PPMXL in cones of radius sqrt(2)/2 degrees around the given center position.65294nobNumber of objects the correction is based onmeta.number147.0620.07177.0600751.0intalphaCenter for field, RAdegpos.eq.ra;meta.main0.510.5180.5350.5360.51floatindexednullabledeltaCenter for field, Decdegpos.eq.dec;meta.main-89.5-84.50.585.590.51floatindexednullabled_alphaCorrection PPMXL-UCAC3 in alpha (Epoch 2000.0)degpos.eq.ra;arith.diff-0.0425202-0.0001459467.32904e-085.69315e-050.04112481floatnullabled_deltaCorrection PPMXL-UCAC3 in delta (Epoch 2000.0)degpos.eq.dec;arith.diff-0.000135361-1.07023e-051.19213e-061.56531e-050.0001475561floatnullabled_pmalphaCorrection PPMXL-UCAC3 in proper motion alpha*cos(delta)deg/yrpos.pm;pos.eq.ra;arith.diff-8.81235e-05-2.28867e-062.8376e-073.21312e-061.53264e-051floatnullabled_pmdeltaCorrection PPMXL-UCAC3 in deltadeg/yrpos.pm;pos.eq.dec;arith.diff-5.54408e-05-2.93633e-06-3.50119e-071.64512e-062.17293e-051floatnullableucac3.mainThe UCAC3 all-sky CCD astrograph catalogue, minus the fields from 2MASS and SuperCosmos and matching/object flags (which can be recovered with a local crossmatch).110000000raj2000Right ascension at epoch (ICRS)degpos.eq.ra;meta.main5.55556e-0725.3713241.933338.8623601doubleindexednullabledej2000Declination at epoch (ICRS)degpos.eq.dec;meta.main-89.9367-69.5781-17.27363.644889.76991doubleindexednullablemmagUCAC fit model magnitudemagphot.mag;em.opt3.06712.17715.75516.891181floatnullablemaperUCAC aperture magnitudemagphot.mag;em.opt4.48712.15115.77117.063181floatnullablesigmagUCAC error on magnitude (larger of obs. scatter and model error)magstat.error;phot.mag;em.opt-0.001-0.0010.1180.4590.91floatnullableobjtObject typesrc.classcharnullabledsfDouble star flagmeta.codecharnullablesigras.e. at central epoch in RA (*cos Dec)degstat.error;pos.eq.ra1.38889e-063.88889e-061.44444e-055.47222e-050.0001388891floatnullablesigdcs.e. at central epoch in Decdegstat.error;pos.eq.dec1.38889e-063.88889e-061.38889e-055.22222e-050.0001388891floatnullablena1Total number of CCD images of this starmeta.number11.02.08.0551.0shortnu1Number of CCD images used for this starmeta.number;stat.fit01.02.07.0521.0shortus1Number of catalogs/epochs used for proper motionsmeta.number11.02.04.0311.0shortcn1Number of catalogs/epochs in initial matchmeta.number01.02.04.01131.0shortcepraCentral epoch for mean RAtime.epochcharnullablecepdcCentral epoch for mean Declinationtime.epochcharnullablepmraProper motion in RA, cos(Dec) applieddeg/yrpos.pm;pos.eq.ra-0.000684722-1.11111e-05-6.11111e-079.58333e-060.001879721floatnullablepmdeProper motion in Declinationdeg/yrpos.pm;pos.eq.dec-0.00161472-1.11389e-05-1.11111e-079.13889e-060.0003686111floatnullablesigpmraError in proper motion in RA, cos(Dec) applieddeg/yrstat.error;pos.pm;pos.eq.ra-2.77778e-07-2.77778e-071.83333e-065.58333e-061.38889e-051floatnullablesigpmdeError in proper motion in Declinationdeg/yrstat.error;pos.pm;pos.eq.dec-2.77778e-07-2.77778e-071.75e-065.33333e-061.38889e-051floatnullableucac3.ppmxlcrossA crossmatch between UCAC3 and PPMXL, created solely based on positions with a window of 1.5 arcsec radius.99000000ucac3idipix of UCAC3 objectmeta.id85491483705531.231447568510247e+174.927828329999753e+186.403765881614033e+1869174641277657002951.0longindexedppmxlidPPMXL ipixmeta.id;meta.main68187852794531.4555397969262336e+174.897678929650011e+186.544739885363848e+1869175110039938228571.0longindexeducac4 UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to 16 magnitude range in a single bandpass between V and R. Positional errors are about 15 to 20 mas for stars in the 10 to 14 mag range. Proper motions have been derived for most of the about 113 million stars utilizing about 140 other star catalogs with significant epoch difference to the UCAC CCD observations. These data are supplemented by 2MASS photometric data for about 110 million stars and 5-band (B,V,g,r,i) photometry from the APASS (AAVSO Photometric All-Sky Survey) for over 50 million stars. UCAC4 also contains error estimates and various flags. All bright stars not observed with the astrograph have been added to UCAC4 from a set of Hipparcos and Tycho-2 stars. Thus UCAC4 should be complete from the brightest stars to about R=16, with the source of data indicated in flags.ucac4.main UCAC4 is a compiled, all-sky star catalog covering mainly the 8 to 16 magnitude range in a single bandpass between V and R. Positional errors are about 15 to 20 mas for stars in the 10 to 14 mag range. Proper motions have been derived for most of the about 113 million stars utilizing about 140 other star catalogs with significant epoch difference to the UCAC CCD observations. These data are supplemented by 2MASS photometric data for about 110 million stars and 5-band (B,V,g,r,i) photometry from the APASS (AAVSO Photometric All-Sky Survey) for over 50 million stars. UCAC4 also contains error estimates and various flags. All bright stars not observed with the astrograph have been added to UCAC4 from a set of Hipparcos and Tycho-2 stars. Thus UCAC4 should be complete from the brightest stars to about R=16, with the source of data indicated in flags.120000000ucacidUCAC 2 identification number (UCAC4-zzz-nnnnnn)meta.id;meta.maincharindexednullableraj2000Right Ascension at epoch J2000.0 (ICRS)degpos.eq.ra;meta.main1.05556e-0525.4659241.39338.4233601doubleindexednullabledej2000Declination at epoch J2000.0 (ICRS)degpos.eq.dec;meta.main-89.9821-69.5891-17.173363.522189.76991doubleindexednullablemagmUCAC fit model magnitudemagphot.mag;em.opt.V4.11212.23515.63516.45716.5930.999395floatnullablemagaUCAC aperture magnitudemagphot.mag;em.opt.V4.16812.18715.62516.51216.5720.987501floatindexednullablesigmagerror of UCAC magnitudemagstat.error;phot.mag;em.opt.V00.030.120.460.90.729271floatnullableobjtObject typesrc.class00.00.05.091.0shortcdfCombined double star flagmeta.code.multip00.00.01.0361.0shortsigraStandard error at central epoch in RA (*cos Dec)degstat.error;pos.eq.ra2.77778e-073.88889e-061.44444e-055.86111e-057.08333e-051floatnullablesigdecStandard error at central epoch in Decdegstat.error;pos.eq.dec2.77778e-073.88889e-061.44444e-055.66667e-057.08333e-051floatnullablena1Total number of CCD images of this starmeta.number01.02.08.0581.0shortnu1Number of CCD images used for this starmeta.number00.02.07.0571.0shortcu1Number of catalogs (epochs) used for proper motionsmeta.number11.02.04.0341.0shortcepraCentral epoch for mean RAyrtime.epoch1947.071969.081993.932002.42004.381floatnullablecepdecCentral epoch for mean Decyrtime.epoch1947.081969.361994.172002.442004.381floatnullablepmraProper motion in RA*cos(Dec)deg/yrpos.pm;pos.eq.ra-0.000539361-9.25e-06-4.44444e-078.36111e-060.001112030.956001floatnullablepmdeProper motion in Decdeg/yrpos.pm;pos.eq.dec-0.00161531-9.69444e-06-6.11111e-077.66667e-060.0004783610.956001floatnullablesigpmrStandard error of proper motion in RA*cos(Dec)deg/yrstat.error;pos.pm;pos.eq.ra8.33333e-083.88889e-071.25e-065.19444e-061.25e-050.956001floatnullablesigpmdStandard error of proper motion in Decdeg/yrstat.error;pos.pm;pos.eq.dec8.33333e-083.88889e-071.25e-065.16667e-061.25e-050.956001floatnullablepts_key2MASS unique star identifiermeta.id24825400932.83644301697.01302466140.3113400371290.966025intnullablemagj2MASS J magnitudemagphot.mag;em.IR.J-2.30210.25913.84515.45617.1210.966025floatnullablesigmagjError in 2MASS J magnitudemagstat.error;phot.mag;em.IR.J0.010.020.030.070.990.966025floatnullableicqflgjQuality flag for 2MASS J magnitudemagmeta.code;phot.mag;em.IR.J00.05.025.0581.0shortnullablemagh2MASS H magnitudemagphot.mag;em.IR.H-3.2249.58713.37715.09317.9940.966023floatnullablesigmaghError in 2MASS H magnitudemagstat.error;phot.mag;em.IR.H0.010.020.040.110.990.966023floatnullableicqflghQuality flag for 2MASS H magnitudemagmeta.code;phot.mag;em.IR.H00.05.025.0581.0shortnullablemagk_s2MASS K_s magnitudemagphot.mag;em.IR.K-3.5119.36513.25615.01417.9790.966025floatnullablesigmagk_sError in 2MASS K_s magnitudemagstat.error;phot.mag;em.IR.K0.010.020.040.190.990.966025floatnullableicqflgk_sQuality flag for 2MASS K_s magnitudemagmeta.code;phot.mag;em.IR.K00.05.025.0581.0shortnullablemagbB magnitude from APASSmagphot.mag;em.opt.B-0.41712.30316.01717.66818.9990.450797floatnullablesigmagbError in B magnitude from APASSmagstat.error;phot.mag;em.opt.B00.010.050.230.990.450797floatnullablemagvV magnitude from APASSmagphot.mag;em.opt.V-0.60811.54115.12716.69418.9980.457715floatnullablesigmagvError in V magnitude from APASSmagstat.error;phot.mag;em.opt.V00.010.020.140.990.457715floatnullablemaggg magnitude from APASSmagphot.mag;em.opt.V6.98111.97415.44117.00518.9820.402124floatnullablesigmaggError in g magnitude from APASSmagstat.error;phot.mag;em.opt.V00.010.030.130.90.402124floatnullablemagrr magnitude from APASSmagphot.mag;em.opt.R6.28911.33814.72316.29218.8120.4005floatnullablesigmagrError in r magnitude from APASSmagstat.error;phot.mag;em.opt.R00.010.030.120.90.4005floatnullablemagii magnitude from APASSmagphot.mag;em.opt.I5.51610.86914.29815.89118.9740.36431floatnullablesigmagiError in i magnitude from APASSmagstat.error;phot.mag;em.opt.I00.010.040.220.90.36431floatnullablespmflagsYale SPM g and c flagsmeta.code;src00.02.04.0371.0shortnullablesrcflagsSource flags (see note)meta.code00.010.010001001.09880200201.0intnullablediam2massObject size from 2MASSdegphys.angSize;src0.0002777780.0008333330.001666670.005555560.02277780.000667226floatnullablernmUnique star identification numbermeta.id36872039.2581135932.5175047628.751828931831.0intzn2Zone number of UCAC2meta.id.part139.0141.0269.02880.42441082shortnullablern2Running record number along UCAC2 zonemeta.id15128.093214.0218525.02701660.42441082intnullableucac5 New astrometric reductions of the US Naval Observatory CCD Astrograph Catalog (UCAC) all-sky observations were performed from first principles using the TGAS stars in the 8 to 11 magnitude range as reference star catalog. Significant improvements in the astrometric solutions were obtained and the UCAC5 catalog of mean positions at a mean epoch near 2001 was generated. By combining UCAC5 with Gaia DR1 data new proper motions on the Gaia coordinate system for over 107 million stars were obtained with typical accuracies of 1 to 2 mas/yr (R = 11 to 15 mag), and about 5 mas/yr at 16th mag. Proper motions of most TGAS stars are improved over their Gaia data and the precision level of TGAS proper motions is extended to many millions more, fainter stars. The database table uses actual NULLs for missing photometry, and all angular coordinates have been homogenised to degrees.ucac5.main New astrometric reductions of the US Naval Observatory CCD Astrograph Catalog (UCAC) all-sky observations were performed from first principles using the TGAS stars in the 8 to 11 magnitude range as reference star catalog. Significant improvements in the astrometric solutions were obtained and the UCAC5 catalog of mean positions at a mean epoch near 2001 was generated. By combining UCAC5 with Gaia DR1 data new proper motions on the Gaia coordinate system for over 107 million stars were obtained with typical accuracies of 1 to 2 mas/yr (R = 11 to 15 mag), and about 5 mas/yr at 16th mag. Proper motions of most TGAS stars are improved over their Gaia data and the precision level of TGAS proper motions is extended to many millions more, fainter stars. The database table uses actual NULLs for missing photometry, and all angular coordinates have been homogenised to degrees.110000000source_idGaia source IDmeta.id;meta.main448738183320323.076592671645764e+174.2013910933282806e+186.720608487973016e+1869175286496842024961.0longraGaia DR1 Right Ascension at epoch J2015.0degpos.eq.ra;meta.main1.66667e-0625.1937239.959338.4843601doubleindexednullabledecGaia DR1 Declination at epoch J2015.0degpos.eq.dec;meta.main-89.948-69.5278-16.804363.661589.85931doubleindexednullablera_errorStandard error of ra (with cos δ applied); from Gaia DR1.degstat.error;pos.eq.ra02.77778e-088.33333e-083.83333e-062.77222e-051floatnullabledec_errorStandard error of dec; from Gaia DR1.degstat.error;pos.eq.dec02.77778e-085.55556e-083.58333e-062.76944e-051floatnullablesrcflagsSource for the star: 1 = TGAS, 2 = other UCAC-Gaia star, 3 = other NOMADmeta.code12.02.03.031.0shortnu1Number of images used for UCAC mean positionmeta.number00.02.07.0481.0shortepuMean UCAC epoch (i.e. epoch for ra_ucac and de_ucac)yrtime.epoch1998.121998.221999.92003.712004.381floatnullablera_ucacMean UCAC RA at epoch epu on Gaia reference framedegpos.eq.ra1.02778e-0525.1938239.959338.4843601doublenullablede_ucacmean UCAC Dec at epoch epu on Gaia reference framedegpos.eq.dec-89.9478-69.5278-16.804363.661689.85921doublenullablepmraPM(RA), cos(δ) applied, computed from UCAC and Gaia DR1 positions.deg/yrpos.pm;pos.eq.ra-0.000340944-6.80556e-06-6.38889e-075.61111e-060.0003886671floatnullablepmdePM(Dec), computed from UCAC positions and Gaia DR1 positions.deg/yrpos.pm;pos.eq.dec-0.000405-7.55556e-06-7.5e-075e-060.0003999441floatnullablesigpmrStandard error of proper motion in RA*cos(Dec)deg/yrstat.error;pos.pm;pos.eq.ra1.94444e-072.77778e-071e-065.83333e-062.44444e-051floatnullablesigpmdStandard error of proper motion in Decdeg/yrstat.error;pos.pm;pos.eq.dec1.94444e-072.77778e-071e-065.58333e-062.44167e-051floatnullablegmagGaia DR1 G magnitudemagphot.mag;em.opt3.32712.00615.45816.80321.5111floatnullableumagMean UCAC model magnitude (20 in the source is mapped to NULL)magphot.mag;em.opt.V3.88512.30215.87417.16718.30.998539floatnullablermagNOMAD photographic R mag (0 and 30 in the source are mapped to NULL)magphot.mag;em.opt.R2.3111.6815.2116.74250.86721floatnullablejmag2MASS J magnitude (0 and 30 in the source are mapped to NULL)magphot.mag;em.IR.J0.48210.32813.84215.46218.5220.897972floatnullablehmag2MASS H magnitude (0 and 30 in the source are mapped to NULL)magphot.mag;em.IR.H-0.4769.70513.38315.10218.9890.897971floatnullablekmag2MASS K_s magnitude (0 and 30 in the source are mapped to NULL)magphot.mag;em.IR.K-0.6629.50513.26615.02319.8650.897969floatnullableurat1 URAT1 is an observational catalog at a mean epoch between 2012.3 and 2014.6; ot covers the magnitude range 3 to 18.5 in R-band, with a positional precision of 5 to 40 mas. It covers most of the northern hemisphere and some areas down to -24.8° in declination. In the GAVO data center, we left out all columns originating from cross matches with other catalogs; on-the fly crossmatches can be done in our TAP service.urat1.main URAT1 is an observational catalog at a mean epoch between 2012.3 and 2014.6; ot covers the magnitude range 3 to 18.5 in R-band, with a positional precision of 5 to 40 mas. It covers most of the northern hemisphere and some areas down to -24.8° in declination. In the GAVO data center, we left out all columns originating from cross matches with other catalogs; on-the fly crossmatches can be done in our TAP service.230000000idURAT1 recommended identifier (ZZZ-NNNNNN)meta.id;meta.maincharindexedprimaryraj2000Right ascension on ICRS, at Epochdegpos.eq.ra;meta.main2.5e-0515.9969279.607345.9993601doubleindexednullabledej2000Declination on ICRS, at Epochdegpos.eq.dec;meta.main-24.8053-10.217427.550170.284689.83641doubleindexednullablepos_err_scatterPosition error per coordinate, from scatterdegstat.error;pos1.38889e-061.66667e-065.27778e-063.11111e-050.0002258331floatnullablepos_err_modelPosition error per coordinate, from modeldegstat.error;pos1.38889e-061.66667e-065.27778e-062.80556e-050.0001191671floatnullableepochMean URAT observation epochyrtime.epoch2012.312012.892013.462014.122014.681floatnullablemagMean URAT model fit magnitude (between R and I)magphot.mag;em.opt.R2.82212.90317.36619.048301floatindexednullablee_magError in URAT model fit magnitude, derived from the scatter of individual observations, plus a floor of 0.01.magstat.error;phot.mag;em.opt.R0.010.0110.0260.2380.8990.902096floatnullablen_setsTotal number of images (observations)meta.number;obs11.05.013.0251.0shortn_sets_posNumber of sets used for mean positionmeta.number;obs-241.05.013.0251.0shortn_sets_magNumber of sets used for URAT magnitudemeta.number;obs01.05.013.0251.0shortrefstarLargest reference star flagmeta.code.qualcharn_imTotal number of images (observations)meta.number;obs11.015.088.03861.0shortn_im_usedNumber of images used for mean positionmeta.number;obs11.015.087.03411.0shortn_gratingTotal number of 1st order grating observationsmeta.number;obs00.00.00.01271.0shortn_grating_usedNumber of 1st order grating positions usedmeta.number;obs00.00.00.01271.0shortwdsdss10 The catalogue WDSLOAN10 has been constructed by spectroscopically selecting white dwarfs and subdwarfs in the Sloan Digital Sky Survey Data Release 10. It offers Teff, log(g) and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white dwarf stars (DBs), and estimatives of calcium/helium abundances for the white dwarf stars with metallic lines (DZs) and carbon/helium for carbon dominated spectra DQs.wdsdss10.main The catalogue WDSLOAN10 has been constructed by spectroscopically selecting white dwarfs and subdwarfs in the Sloan Digital Sky Survey Data Release 10. It offers Teff, log(g) and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white dwarf stars (DBs), and estimatives of calcium/helium abundances for the white dwarf stars with metallic lines (DZs) and carbon/helium for carbon dominated spectra DQs.9114raj2000Right ascensiondegpos.eq.ra;meta.main0.29858316.9492191.311334.839359.9061doubleindexeddecj2000Declinationdegpos.eq.dec;meta.main-13.1491-2.1054618.181949.688382.33191doubleindexedsnrg-band signal-to-noise ratiostat.snr;phot.flux;em.opt.B11.08.053.0911.0intuSDSS u band PSF magnitudemagphot.mag;em.opt.U13.5616.3920.722.9426.921floatu_errSDSS u band uncertaintymagstat.error;phot.mag;em.opt.U00.010.060.4111.091floatgSDSS g band PSF magnitudemagphot.mag;em.opt.B14.4516.520.122225.111floatg_errSDSS g band uncertaintymagstat.error;phot.mag;em.opt.B00.010.030.0811.341floatrSDSS r band PSF magnitudemagphot.mag;em.opt.R13.9116.843920.0322.0524.81floatr_errSDSS r band uncertaintymagstat.error;phot.mag;em.opt.R00.010.030.118.961floatiSDSS i band PSF magnitudemagphot.mag;em.opt.I13.8717.0620.0722.0824.371floati_errSDSS i band uncertaintymagstat.error;phot.mag;em.opt.I00.010.040.1810.921floatzSDSS z band PSF magnitudemagphot.mag;em.opt.I0.0317.2720.1622.123.411floatz_errSDSS z band uncertaintymagstat.error;phot.mag;em.opt.I0.010.020.120.633001floatpmSDSS proper motionmas/yrpos.pm0009.4845.671floatt_effEffective TemperatureKphys.temperature.effective;meta.main41136593.1710142.049287.4700000000161400001.0intt_errError effective temperatureKstat.error;phys.temperature.effective;meta.main036.389999999999986199.51999.6100000000006250001.0intlog_gSurface gravitylog(cm/s**2)phys.gravity;meta.main45.043989.15344101floatlog_gerrSurface gravity errorlog(cm/s**2)stat.error;phys.gravity;meta.main000.150.671835.6211floathumanidHuman clssificationmeta.code.classchart_eff_3dTemperature (convective model) for pure DAs and DBsKphys.temperature;meta.modelled45626796.389576.036002.889999999891000000.70484966intnullablet_err_3dError temperature (convective model)Kstat.error;phys.temperature;meta.modelled348.0194.01437.0299999999934100000.70484966intnullablelog_g_3dphys.gravity;meta.modelled3.846.17.988.9410.050.70485floatnullablelog_gerr_3dstat.error;phys.gravity;meta.modelled00.010.20.685.620.70485floatnullablemassCalculated masssolMassphys.mass0.0410.167950.6011.124151.4450.742374floatnullablemass_errMass uncertaintysolMassstat.error;phys.mass00.0050.080.2681.430.742374floatnullablelog_caCalcium/Helium emission lines ratiophys.abund;arith.ratio6.57.094688.98110.497710.50.0444371floatnullablelog_ca_errCalcium/Helium emission lines ratio errorstat.error;phys.abund;arith.ratio00.022120.1080.49641.050.0444371floatnullablelog_cCarbon/Helium emission lines ratiophys.abund;arith.ratio-0.51.45.3386.888717.5060.00658328floatnullablelog_c_errCarbon/Helium emission lines ratio errorstat.error;phys.abund;arith.ratio0.0180.021770.0580.192030.2460.00658328floatnullablepdfSDSS object/observation identifiermeta.id;meta.maincharindexedprimaryzcosmos The zCOSMOS redshift survey used 600h on the VIMOS spectrograph spread over five observing seasons (2005-2009) to obtain spectra of about 20,000 galaxies selected to have Iab < 22.5 across the full 1.7 deg2 of the COSMOS field. This part, "zCOSMOS-bright", was designed to yield a high and fairly uniform sampling rate (about 70%), with a high success rate in measuring redshifts (approaching 100% at 0.5 < z < 0.8), and with sufficient velocity accuracy (about 100 km/s) to efficiently map the environments of galaxies down to the scale of galaxy groups out to redshifts z ~ 1.zcosmos.data The zCOSMOS redshift survey used 600h on the VIMOS spectrograph spread over five observing seasons (2005-2009) to obtain spectra of about 20,000 galaxies selected to have Iab < 22.5 across the full 1.7 deg2 of the COSMOS field. This part, "zCOSMOS-bright", was designed to yield a high and fairly uniform sampling rate (about 70%), with a high success rate in measuring redshifts (approaching 100% at 0.5 < z < 0.8), and with sufficient velocity accuracy (about 100 km/s) to efficiently map the environments of galaxies down to the scale of galaxy groups out to redshifts z ~ 1.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size3168034560.034560.037440.0403201.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassIR, Optical, UVcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.ClassXcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extent0.0008333330.0008333330.0008333330.0008333330.0008333331floatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Value53463.1534695381953876538841doubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extent2879.923599.923600.043600.077920.111floatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Start5.50511e-075.50511e-075.50511e-075.50511e-075.50511e-071floatindexednullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stop9.69458e-079.69458e-079.69458e-079.69458e-079.69458e-071floatindexednullablessa_lengthNumber of points in the spectrumssa:Dataset.Length16421642.01642.01642.016421.0intnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wl;obs.atmoscharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.Collectionzcosmoscharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcetheorycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationRELATIVEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullabledatalinkA link to a datalink document for this spectrum.meta.ref.urlcharnullablebrowndwarfsA catalogue of brown dwarfs produced by Gelino et al. The database reflects the state of http://www.dwarfArchives.org on 2015-09-29.browndwarfs.catA catalogue of brown dwarfs produced by Gelino et al. The database reflects the state of http://www.dwarfArchives.org on 2015-09-29.1281designationDesignation, typically from 2MASSmeta.id;meta.maincharnullableraj2000RA J2000.0degpos.eq.ra;meta.main0.05641658.92642179.325350.24359.991floatindexednullabledej2000Dec J2000.0degpos.eq.dec;meta.main-82.4398-63.41818.7925364.299687.89151floatindexednullablejmagMagnitude in the J bandmagphot.mag;em.IR.J11.5113.152516.00119.03123.570.960968floatnullableerrjmagError in magnitude in the J bandmagstat.error;phot.mag;em.IR.J0.010.020.0630.206211.20.932084floatnullablehmagMagnitude in the H bandmagphot.mag;em.IR.H10.8312.351215.13619.122.850.936768floatnullableerrhmagError in magnitude in the H bandmagstat.error;phot.mag;em.IR.H0.010.0210.0640.2330.660.906323floatnullablekmagMagnitude in the K bandmagphot.mag;em.IR.K10.3311.721714.47918.610821.10.891491floatnullableerrkmagError in magnitude in the K bandmagstat.error;phot.mag;em.IR.K0.010.0210.0620.2340.3990.814208floatnullableparallaxParallax as reported by parallax_paper.degpos.parallax2.73611e-064.46811e-061.54806e-056.923e-057.66e-050.0725995floatnullableparallax_errorError in parallax as reported by parallax_paper.degstat.error;pos.parallax8.33333e-081.6e-075.55556e-074.63944e-069.16667e-060.0725995floatnullableparallax_paperReference to the paper the parallax was taken frommeta.bib;pos.parallaxcharnullablepm_totTotal proper motiondeg/yrpos.pm2.77778e-068.68611e-067.17736e-050.00053860.001306650.340359floatnullablepm_tot_errError in total proper motion.deg/yrstat.error;pos.pm5.55556e-081.96944e-074.57222e-064.875e-050.0003388890.324746floatnullablepm_paPosition angle of proper motiondegpos.posAng;pos.pm2.527.027175.7301.7358.90.337237floatnullablepm_pa_errorError in the position angle of the proper motion.degstat.error;pos.posAng;pos.pm0.010.06063.3447.911700.313817floatnullablepm_paperPaper the proper motion was taken from.meta.bib;pos.pmcharnullablespectral_optSpectral type inferred from observation in visible lightsrc.spType;em.optcharindexednullablest_opt_paperReference to the paper the optical spectral type was taken frommeta.bib;src.spTypecharnullablespectral_irSpectral type inferred from observation in infraredsrc.spType;em.IRcharnullablest_ir_paperReference to the paper the infrared spectral type was taken frommeta.bib;src.spTypecharnullablediscovered_asName the object was discovered as.meta.idcharnullablediscovered_byReference to the paper in which the object was discovered.meta.bibcharnullablecarmenes The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The service publishes the radial velocities derived from the CARMENES guaranteed time observations (GTO), spanning from 2016 to 2020. This results in 362 individual time series mapping time to radial velocities.carmenes.dataThe spectra from which the CARMENES radial velocity curves were made. Note that we only publish spectra that were actually used in time series. Also, note that positions and object names from the headers of the spectra are unreliable.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.Bandpass520 .. 1063 nmcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoubleindexednullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.densitycharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionCARMENES DR1charnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationNORMALIZEDcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablen_ordersNumber of orders in the spectrum.meta.numberintnullableorder_minMinimal Echelle order in the spectrum.instr.order;stat.minintnullableorder_maxMaximal Echelle order in the spectrum.instr.order;stat.maxintnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullabledatalinkA link to a datalink document for this spectrum.meta.ref.urlcharnullablerv_driftEstimated RV drift against the evening referencem/sobs.paramfloatnullablename_hdrTarget name as given in the FITS header (ssa_targname is an attempt to clean these up, but that may occasionally be wrong).meta.idcharnullablecarmenes.objectsProperties of CARMENES DR1 target objects. This is derived from ivo://cds.vizier/J/A+A/670/A139.361carmenes_idCARMENES target designationmeta.id;meta.maincharindexedprimarynameSIMBAD-resolvable star namemeta.idcharnullablenobsNumber of nightly zero point corrected radial velocity measurements for this objectmeta.number;obsshortnullablenspectNumber of spectra for this object in DR1meta.numbershortmassMass of the star from CarmencitasolMassphys.massdoublenullableerr_massUncertainty in masssolMassstat.error;phys.massfloatnullableradiusRadius of the star from CarmencitasolRadphys.size.radiusdoublenullableerr_radiusUncertainty in radiussolRadstat.error;phys.size.radiusfloatnullableteffEffective temperature of the star from carmencitaKphys.temperature.effectivefloatnullableerr_teffUncertainty in teffKstat.error;phys.temperature.effectivefloatnullablep_rotRotation period of the star (see p_rot_source for the provenance of this value)dtime.perioddoublenullablep_rot_sourceSource of the value in p_rot (see 2023A&A...670A.139R for the meaning of the abbreviations)meta.bibcharnullablesurveyFlag identifying stars that are part of the blind radial velocity survey (GTO) or the program to determine the mass of transiting planets (TESS). An asterisk marks stars already tabulated in Reiners et al., 2018A&A...612A..49Rmeta.codecharnullableremarksComment identifying spectroscopic multiple systems: Double-line spectroscopic binaries (SB2), triple-line spectroscopic binaries (ST3), and visual binaries (Visual). Multiplicity references: Bar18 – 2018A&A...619A..32B; Bar21 – 2021A&A...653A..49B; Gaia – 2016A&A...595A...1G; Mor09 – 2009ApJ...691.1400Mmeta.notecharnullableraRight Ascension (J2000) from SIMBADdegpos.eq.ra;meta.maindoublenullabledecDeclination (J2000) from SIMBADdegpos.eq.dec;meta.maindoublenullablecarmenes.rvsAll RV estimates from CARMENES DR1, for all objects. To obtain single time series, it is probably simpler to use the SSA service or pull them from obscore.18642objectCarmenes identifier of the target objectmeta.id;meta.maincharnullablebjdJD of the observation at the solar system barycenter (probably in TDB).dtime.epochdoublenullablervRadial velocity derived by the Serval pipelinekm/sspect.dopplerVelocdoublenullableerr_rvUncertainty in rvkm/sstat.error;spect.dopplerVelocfloatnullablea_rvRadial velocity derived by the Serval pipeline, corrected for the CARMENES' nightly zero point (NZP), which ought to repair most of the instruments' drift.km/sspect.dopplerVelocdoublenullableerr_a_rvUncertainty in a_rvkm/sstat.error;spect.dopplerVelocfloatnullabledlwDifferential line width derived by the Serval pipeline; this is a marker for stellar activity.m**2/s**2spect.line.width;arith.difffloatnullableerr_dlwUncertainty in dlwm**2/s**2stat.error;spect.line.width;arith.difffloatnullableccf_rvBERV-, secular acceleration- and drift-corrected radial velocity derived by the Racoon pipeline (see 2020A&A...636A..36L).km/sspect.dopplerVelocdoublenullableerr_ccf_rvUncertainty in ccf_rvkm/sstat.error;spect.dopplerVelocfloatnullableccf_fwhmFull Width Half Maximum derived by the Racoon pipeline.km/sspect.dopplerVeloc;stat.fwhmdoublenullableerr_ccf_fwhmUncertainty in ccf_fwhmkm/sstat.error;spect.dopplerVeloc;stat.fwhmfloatnullableccf_contrastContrast derived by the Racoon Pipeline (see 2020A&A...636A..36L).%phot.flux;arith.ratiofloatnullableerr_ccf_contrastUncertainty in ccf_contrast%stat.error;phot.flux;arith.ratiofloatnullableccf_bisBisector inverse slope derived by the Racoon pipeline (see 2020A&A...636A..36L).km/sfloatnullableerr_ccf_bisUncertainty in ccf_biskm/sfloatnullablehalphaHα (λ=6562.81 Angstrom) index; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_halphaUncertainty in halphastat.error;spect.indexfloatnullablehacenFlat-normalised Hα mean fluxcountphot.flux;em.line.Halphafloatnullableerr_hacenUncertainty in hacencountstat.error;phot.flux;em.line.HalphafloatnullablehaleftFlat-normalised flux in the left Hα reference region, i.e., (-300, -100) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).countphot.flux;em.line.Halphafloatnullableerr_haleftUncertainty in haleftcountstat.error;phot.flux;em.line.HalphafloatnullableharightFlat-normalised flux in the right Hα reference region, i.e., (100, 300) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).countphot.flux;em.line.Halphafloatnullableerr_harightUncertainty in harightcountstat.error;phot.flux;em.line.HalphafloatnullablecaiCa I λ=6572.80 Angstrom index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_caiUncertainty in caistat.error;spect.indexfloatnullablecai_8498Ca II λ=8498.02 index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_cai_8498Uncertainty in cai_8498stat.error;spect.indexfloatnullablecai_8542Ca II λ=8542.09 index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_cai_8542Uncertainty in cai_8542stat.error;spect.indexfloatnullablecai_8698Ca II λ=8662.14 index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_cai_8698Uncertainty in cai_8698stat.error;spect.indexfloatnullablenad1Na I D1 λ=5889.95 Angstrom index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_nad1Uncertainty in nad1stat.error;spect.indexfloatnullablenad2Na I D2 λ=5895.92 Angstrom index (-15,15) km/s; this is an indicator for stellar activity (cf. 2018A&A...609A..12Z).spect.indexfloatnullableerr_nad2Uncertainty in nad2stat.error;spect.indexfloatnullablespec_flagBit mask for spectral problems: bit 5 S/N too low, bit 6 S/N too high, bit 7 not within nautical twilight, bit 8 too close to the moon, bit 9 LED on during observationmeta.code.qualshortdriftDrift measure derived by the caracal pipeline.m/sinstr.calibfloatnullableerr_driftUncertainty in driftm/sstat.error;instr.calibfloatnullablebervBarycentric RV of the Earthm/sphys.velocdoublenullablesadriftDrift due to secular accelerationm/sinstr.calibfloatnullablespec_accrefThe access reference of the source spectrum.meta.id;meta.filecharnullablervmeanUndrifted mean radial velocitykm/sspect.dopplerVeloc;stat.meandoublenullableerr_rvmeanUncertainty in rvmeankm/sstat.error;spect.dopplerVeloc;stat.meanfloatnullablervmedUndrifted median radial velocitykm/sspect.dopplerVeloc;stat.mediandoublenullableerr_rvmedUncertainty in rvmedkm/sstat.error;spect.dopplerVeloc;stat.medianfloatnullablerv_orders_servalPer-order radial velocity estimates from serval, starting with order 118, ending at order 58km/sspect.dopplerVelocfloatnullableerr_rv_orders_servalErrors for rv_orders_servalkm/sstat.error;spect.dopplerVelocfloatnullabledlw_orders_servalPer-order differential line width from serval, starting with order 118, ending at order 58m**2/s**2spect.line.width;arith.difffloatnullableerr_dlw_orders_servalErrors for dlw_orders_servalkm/sstat.error;spect.line.width;arith.difffloatnullablerv_orders_racoonPer-order radial velocity estimates from racoon, starting with order 118, ending at order 58km/sspect.dopplerVelocfloatnullableerr_rv_orders_racoonErrors for rv_orders_racoonkm/sstat.error;spect.dopplerVelocfloatnullablefwhm_orders_racoonPer-order FWHM estimates from racoon, starting with order 118, ending at order 58floatnullableerr_fwhm_orders_racoonErrors for fwhm_orders_racoonfloatnullablecontrast_orders_racoonPer-order FWHM estimates from racoon, starting with order 118, ending at order 58floatnullableerr_contrast_orders_racoonErrors for contrast_orders_racoonfloatnullablebis_orders_racoonPer-order BIS estimates from racoon, starting with order 118, ending at order 58floatnullableerr_bis_orders_racoonErrors for bis_orders_racoonfloatnullablecarmenes.ts_ssa The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The service publishes the radial velocities derived from the CARMENES guaranteed time observations (GTO), spanning from 2016 to 2020. This results in 362 individual time series mapping time to radial velocities.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Sizelongnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.Versioncharnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wl;obs.atmoscharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typetimeseriescharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionCARMENES DR1 timeseriescharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcetheorycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationRELATIVEcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime-6146.555450.156458.35814959214.20.620126doublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime-6146.5562865762658738.163023.50.620108doublenullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullabledatalinkA link to a datalink document for this spectrum.meta.ref.urlcharnullablechianti CHIANTI consists of a critically evaluated set of up-to-date atomic data and derived spectral lines. At http://www.chiantidatabase.org/, many tools for this data set are available. The present resource only takes the line data and makes it available in standard LineTAP. This is the state as of CHIANTI 10.1.chianti.lines CHIANTI consists of a critically evaluated set of up-to-date atomic data and derived spectral lines. At http://www.chiantidatabase.org/, many tools for this data set are available. The present resource only takes the line data and makes it available in standard LineTAP. This is the state as of CHIANTI 10.1.ivo://ivoa.net/std/linetap#lines-1.02200000titleHuman-readable line designation.meta.idcharvacuum_wavelengthVacuum wavelength of the transitionAngstromem.wl0.59016.1778165.6042999.731e+081doubleindexedvacuum_wavelength_errorTotal error in vacuum_wavelengthAngstromstat.error;em.wl0doublenullablemethodMethod the wavelength was obtained with (XSAMS controlled vocabulary)meta.code.classobservedtheoryritzcharnullableelementElement name for atomic transitions, NULL otherwise.phys.atmol.elementcharindexednullableion_chargeTotal charge (ionisation level) of the emitting particle.phys.electCharge02.011.024.0281.0intindexedmass_numberNumber of nucleons in the atom or moleculephys.atmol.weight0.0intnullableupper_energyEnergy of the upper stateJphys.energy;phys.atmol.initial3.26115e-227.94895e-188.17621e-171.53852e-153.36628e-151doublenullablelower_energyEnergy of the lower stateJphys.energy;phys.atmol.final01.13668e-185.49717e-171.25788e-153.35751e-151doublenullableinchiInternational Chemical Identifier InChI.meta.id;phys.atmol;meta.maincharindexedinchikeyThe InChi key (hash) generated from inchi.meta.id;phys.atmolcharindexedeinstein_aEinstein A coefficient of the radiative transition.phys.atmol.transProb1e-3073502.88.52e+072.81e+111.63e+151doublenullablexsams_uriA URI for a full XSAMS description of this line.meta.refcharnullableline_referenceReference to the source of the line data; this could be a bibcode, a DOI, or a plain URI.meta.refcharcitigbot This archive collects and re-publishes third-party, mostly amateur, images of the Gaia astrometry satellite to complemement the Ground Based Optical Tracking (GBOT) effort. Until Gaia passivation, there is a temporary upload facility at https://dc.g-vo.org/citigbot/q/upload/form.citigbot.main This archive collects and re-publishes third-party, mostly amateur, images of the Gaia astrometry satellite to complemement the Ground Based Optical Tracking (GBOT) effort. Until Gaia passivation, there is a temporary upload facility at https://dc.g-vo.org/citigbot/q/upload/form.14dataproduct_typeHigh level scientific classification of the data product, taken from an enumerationmeta.code.classobscore:obsdataset.dataproducttypeimagecharnullabledataproduct_subtypeData product specific typemeta.code.classobscore:obsdataset.dataproductsubtypecharnullablecalib_levelAmount of data processing that has been applied to the datameta.code;obs.calibobscore:obsdataset.caliblevel22.02.02.021.00123shortobs_collectionName of a data collection (e.g., project name) this data belongs tometa.idobscore:dataid.collectioncitizen GBOTcharnullableobs_idUnique identifier for an observationmeta.idobscore:DataID.observationIDcharnullableobs_titleFree-from title of the data setmeta.title;obsobscore:dataid.titlecharnullableobs_publisher_didDataset identifier assigned by the publisher.meta.ref.ivoidobscore:curation.publisherdidcharindexednullableobs_creator_didDataset identifier assigned by the creator.meta.idobscore:dataid.creatordidcharnullableaccess_urlThe URL at which to obtain the data set.meta.ref.urlobscore:access.referencecharnullableaccess_formatMIME type of the resource at access_urlmeta.code.mimeobscore:access.formatcharnullableaccess_estsizeEstimated size of data productkbytephys.size;meta.fileobscore:access.size29673011.0721328.556624.92999999999602181.0longnullabletarget_nameObject a targeted observation targetedmeta.id;srcobscore:Target.Namecharnullabletarget_classClass of the target object (star, QSO, ...)src.classobscore:target.classspace-probescharnullables_raRA of (center of) observation, ICRSdegpos.eq.raobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c112.85160.8483149.352173.074173.1751doubleindexednullables_decDec of (center of) observation, ICRSdegpos.eq.decobscore:char.spatialaxis.coverage.location.coord.position2d.value2.c2-17.6189-9.188817.9261110.77111.05951doubleindexednullables_fovApproximate spatial extent for the region covered by the observationdegphys.angSize;instr.fovobscore:char.spatialaxis.coverage.bounds.extent.diameter0.3303510.4001250.7911542.569262.625611floatnullables_regionRegion covered by the observation, as a polygonpos.outline;obs.fieldobscore:char.spatialaxis.coverage.support.areacharnullables_resolutionBest spatial resolution within the data setarcsecpos.angResolutionobscore:Char.SpatialAxis.Resolution.refval.value0.001448720.01478450.53091.994242.280121floatnullablet_minLower bound of times represented in the data setdtime.start;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.starttime54702.3570416071160738.9607391doublenullablet_maxUpper bound of times represented in the data setdtime.end;obs.exposureobscore:char.timeaxis.coverage.bounds.limits.stoptime54702.3570416071160738.9607391doublenullablet_exptimeTotal exposure timestime.duration;obs.exposureobscore:char.timeaxis.coverage.support.extent4550.85901112.414401floatnullablet_resolutionMinimal significant time interval along the time axisstime.resolutionobscore:char.timeaxis.resolution.refval.value0floatnullableem_minMinimal wavelength represented within the data setmem.wl;stat.minobscore:char.spectralaxis.coverage.bounds.limits.lolimit0floatnullableem_maxMaximal wavelength represented within the data setmem.wl;stat.maxobscore:char.spectralaxis.coverage.bounds.limits.hilimit0floatnullableem_res_powerSpectral resolving power lambda/delta lambdaspect.resolutionobscore:char.spectralaxis.resolution.resolpower.refval0floatnullableo_ucdUCD for the product's observablemeta.ucdobscore:char.observableaxis.ucdcharnullablepol_statesList of polarization states in the data setmeta.code;phys.polarizationobscore:Char.PolarizationAxis.stateListcharnullablefacility_nameName of the facility at which data was takenmeta.id;instr.telobscore:Provenance.ObsConfig.facility.nameNULLcharnullableinstrument_nameName of the instrument that produced the datameta.id;instrobscore:Provenance.ObsConfig.instrument.nameNULLcharnullables_xel1Number of elements (typically pixels) along the first spatial axis.meta.numberobscore:Char.SpatialAxis.numBins113751437.792947.06250.4462521.0intnullables_xel2Number of elements (typically pixels) along the second spatial axis.meta.numberobscore:Char.SpatialAxis.numBins210241053.642095.04176.041761.0intnullablet_xelNumber of elements (typically pixels) along the time axis.meta.numberobscore:Char.TimeAxis.numBins11.01.01.011.0intnullableem_xelNumber of elements (typically pixels) along the spectral axis.meta.numberobscore:Char.SpectralAxis.numBins11.01.01.011.0intnullablepol_xelNumber of elements (typically pixels) along the polarization axis.meta.numberobscore:Char.PolarizationAxis.numBins0.0intnullables_pixel_scaleSampling period in world coordinate units along the spatial axisarcsecphys.angSize;instr.pixelobscore:Char.SpatialAxis.Sampling.RefVal.SamplingPeriod0.001448720.01478450.53091.994242.280121floatnullableem_ucdNature of the product's spectral axis (typically, em.freq, em.wl, or em.energy)meta.ucdobscore:Char.SpectralAxis.ucdcharnullablesource_tableName of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details.meta.id;meta.tablecharnullableupload_dateTimestamp the dataset was uploaded to the GAVO data centre.time.release60613.5977750328760648.8747780612860718.5671117572960739.395212653660739.650059644331.0charnullablenickObserver nickname; this is some free string they put in during upload.obs.observercharnullablegcpmsA proper-motion catalogue of 5080236 stars in 49 OGLE-II Galactic bulge (GB) fields, covering a range of -11°<l<11° and -6°<b<3°. Some columns have been left out from the original source.gcpms.dataA proper-motion catalogue of 5080236 stars in 49 OGLE-II Galactic bulge (GB) fields, covering a range of -11°<l<11° and -6°<b<3°. Some columns have been left out from the original source.5100000fieldOGLE field numbermeta.id;obs.field12.025.046.0491.0shortogleOGLE numbermeta.id;meta.main115728.0323517.5744645.05999999969573781.0intnpointNumber of data pointsmeta.number;stat.fit2026.0213.0412.05551.0shortpmraProper motion in right ascension (mu(RA)cos(DE)deg/yrpos.pm;pos.eq.ra-0.000105-3.76944e-06-2.77778e-093.7e-060.0001504861floatnullablee_pmrarms uncertainty on pmRAdeg/yrstat.error;pos.pm;pos.eq.ra6.38889e-081.25e-075.05556e-073.62778e-063.14417e-051floatnullablepmdeProper motion in declination (mu(DE))deg/yrpos.pm;pos.eq.dec-0.000121358-3.53611e-06-2.77778e-093.425e-065.94472e-051floatnullablee_pmderms uncertainty on pmDEdeg/yrstat.error;pos.pm;pos.eq.dec5.55556e-081.16667e-074.86111e-073.51667e-062.4375e-051floatnullabledrefcDifferential refraction coefficientdeg-9.38306e-05-7.10833e-06-5.55556e-097.41389e-068.98306e-051floatnullablesdevStandard deviation of data points in the fittingdegstat.stdev;pos1.11111e-062.54444e-068.23056e-062.52444e-057.25111e-051floatnullableimagI magnitudemagphot.mag;em.opt.I10.36813.7716.96117.963181floatnullablev_iV-I colour indexmagphot.color;em.opt.V;em.opt.I-2.9471.1491.8473.2998.5760.930408floatnullableraj2000Right ascension in decimal degrees (J2000)degpos.eq.ra;meta.main261.611263.724270.174275.159276.1371doubleindexednullabledej2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.main-40.7431-37.4675-29.2275-22.3358-21.32751doubleindexednullablexposx pixel coordinate in template imagepixpos.cartesian.x;instr.det064.171017.871982.172047.51floatnullableyposy pixel coordinate in template imagepixpos.cartesian.y;instr.det0.03274.064181.697938.078191.481floatnullablehamburg_eso The Hamburg/ESO survey (HES) is a digital objective prism survey covering the total southern extragalactic sky. It is based on Kodak IIIa-J plates which have been taken with the 1m ESO Schmidt telescope and its 4° prism. The spectral coverage is 3200-5300 Å, at an resolution of 15 Å at H gamma. The magnitude range covered is roughly between 18.5 and 11 mag in B_J. This is a collection of uniformly reduced spectra prepared by Norbert Christlieb. It is also intended as a sort-of resolver for HES names (“identifiers“) like ”HE 2301-7732”; unfortunately, these identifiers are not unique. You will need to apply domain knowledge in order to find the object actually being referred to when resolving an identifier of this sort.hamburg_eso.data The Hamburg/ESO survey (HES) is a digital objective prism survey covering the total southern extragalactic sky. It is based on Kodak IIIa-J plates which have been taken with the 1m ESO Schmidt telescope and its 4° prism. The spectral coverage is 3200-5300 Å, at an resolution of 15 Å at H gamma. The magnitude range covered is roughly between 18.5 and 11 mag in B_J. This is a collection of uniformly reduced spectra prepared by Norbert Christlieb. It is also intended as a sort-of resolver for HES names (“identifiers“) like ”HE 2301-7732”; unfortunately, these identifiers are not unique. You will need to apply domain knowledge in order to find the object actually being referred to when resolving an identifier of this sort.accrefAccess key for the datameta.ref.url;meta.datasetssa:Access.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimessa:Access.FormatcharnullableaccsizeSize of the data in bytesbytessa:Access.Size1000010000.010000.010000.0100001.0longnullablessa_dstitleA compact and descriptive designation of the dataset.meta.title;meta.datasetssa:DataID.Titlecharssa_creatordidDataset identifier assigned by the creatormeta.idssa:DataID.CreatorDIDcharnullablessa_pubdidDataset identifier assigned by the publishermeta.ref.ivoidssa:Curation.PublisherDIDcharindexednullablessa_cdateProcessing/Creation datetime;meta.datasetssa:DataID.Datecharnullablessa_pdateDate last published.ssa:Curation.Datecharnullablessa_bandpassBandpass (i.e., rough spectral location) of this dataset; this should be the most appropriate term from the vocabulary http://www.ivoa.net/rdf/messenger.instr.bandpassssa:DataID.BandpassOpticalcharnullablessa_cversionCreator assigned version for this dataset (will be incremented when this particular item is changed).meta.version;meta.datasetssa:DataID.VersionDR 6charnullablessa_targnameCommon name of object observed.meta.id;srcssa:Target.Namecharssa_targclassObject class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible)src.classssa:Target.Classstarcharnullablessa_redshiftRedshift of target objectsrc.redshiftssa:Target.Redshiftfloatnullablessa_targetposEquatorial (ICRS) position of the target object.pos.eq;srcssa:Target.pos.spointdoublenullablessa_snrSignal-to-noise ratio estimated for this datasetstat.snrssa:Derived.SNRfloatnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_apertureAngular diameter of aperturedegphys.angSize;instr.fovssa:Char.SpatialAxis.Coverage.Bounds.Extentfloatnullablessa_dateobsMidpoint of exposure (MJD)dtime.epochssa:Char.TimeAxis.Coverage.Location.Valuedoublenullablessa_timeextExposure durationstime.durationssa:Char.TimeAxis.Coverage.Bounds.Extentfloatnullablessa_specmidMidpoint of region covered in this datasetminstr.bandpassssa:Char.SpectralAxis.Coverage.Location.Valuefloatnullablessa_specextWidth of the spectrumminstr.bandwidthssa:Char.SpectralAxis.Coverage.Bounds.Extentfloatnullablessa_specstartLower value of spectral coordinatemem.wl;stat.minssa:Char.SpectralAxis.Coverage.Bounds.Startfloatnullablessa_specendUpper value of spectral coordinatemem.wl;stat.maxssa:Char.SpectralAxis.Coverage.Bounds.Stopfloatnullablessa_lengthNumber of points in the spectrumssa:Dataset.Lengthintnullablessa_modelData model name and versionssa:Dataset.DataModelSpectrum-1.0charssa_csysnameSystem RA and Dec are given inssa:CoordSys.SpaceFrame.NameICRScharssa_timesiTime conversion factor in Osuna-Salgado convention.ssa:Dataset.TimeSIcharnullablessa_spectralsiSpectral conversion factor in Osuna-Salgado conventionssa:Dataset.SpectralSIcharnullablessa_spectralucdUCD of the spectral column in the spectra served; when you have wavelengths, use em.wl for vacuum wavelengths, em.wl;obs.atmos for air wavelengths.meta.ucdssa:Char.SpectralAxis.Ucdem.wlcharssa_spectralunitUnit of the spectral columnmeta.unitssa:Char.SpectralAxis.UnitAngstromcharssa_fluxsiFlux/magnitude conversion factor in Osuna-Salgado conventionssa:Dataset.FluxSIcharnullablessa_fluxucdUCD of the flux columnmeta.ucdssa:Char.FluxAxis.Ucdphot.flux.density;em.wlcharssa_fluxunitUnit of the flux columnmeta.unitssa:Char.FluxAxis.Unitcharssa_dstypeType of data (spectrum, time series, etc)ssa:Dataset.Typespectrumcharnullablessa_publisherPublisher of the datasets included here.meta.curationssa:Curation.Publishercharssa_creatorCreator of the datasets included here.ssa:DataID.CreatorunicodeCharnullablessa_collectionA short handle naming the collection this spectrum belongs to.ssa:DataID.CollectionHamburg-ESO Surveycharnullablessa_instrumentInstrument or code used to produce these datasetsmeta.id;instrssa:DataID.InstrumentVIMOScharnullablessa_datasourceMethod of generation for the data (one of survey, pointed, theory, custom, artificial).ssa:DataID.DataSourcesurveycharnullablessa_creationtypeProcess used to produce the data (archival, cutout, filtered, mosaic, projection, spectralExtraction, or catalogExtraction)ssa:DataID.CreationTypearchivalcharnullablessa_referenceURL or bibcode of a publication describing this data.meta.bib.bibcodessa:Curation.Referencecharnullablessa_fluxstaterrorStatistical error in fluxstat.error;phot.flux.density;emssa:Char.FluxAxis.Accuracy.StatErrorfloatnullablessa_fluxsyserrorSystematic error in fluxstat.error.sys;phot.flux.density;emssa:Char.FluxAxis.Accuracy.SysErrorfloatnullablessa_fluxcalibType of flux calibration (ABSOLUTE, CALIBRATED, RELATIVE, NORMALIZED, or UNCALIBRATED).ssa:Char.FluxAxis.CalibrationUncalibratedcharnullablessa_binsizeBin size in wavelengthmem.wl;spect.binSizessa:Char.SpectralAxis.Accuracy.BinSizefloatnullablessa_spectstaterrorStatistical error in wavelengthmstat.error;emssa:Char.SpectralAxis.Accuracy.StatErrorfloatnullablessa_spectsyserrorSystematic error in wavelengthmstat.error.sys;emssa:Char.SpectralAxis.Accuracy.SysErrorfloatnullablessa_speccalibType of wavelength calibrationmeta.code.qualssa:Char.SpectralAxis.CalibrationABSOLUTEcharnullablessa_specresResolution (in meters of wavelength) on the spectral axismspect.resolution;em.wlssa:Char.SpectralAxis.Resolutionfloatnullablessa_spaceerrorStatistical error in positiondegstat.error;pos.eqssa:Char.SpatialAxis.Accuracy.StatErrorfloatnullablessa_spacecalibType of calibration in spatial coordinatesmeta.code.qualssa:Char.SpatialAxis.Calibrationcharnullablessa_spaceresSpatial resolution of datadegpos.angResolutionssa:Char.SpatialAxis.Resolutionfloatnullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablehes_nameHES designation, consisting of the letters 'HE', the first four digits of the right ascension at equinox B1950.0, and the first four digits of the declination at equinox B1950.0. Example: HE 2301-7732.meta.id;meta.maincharindexednullablehes_idAlternative, more precise HES identifier consisting of the first seven digits of the right ascension at equinox 2000.0, the first six digits of the declination at equinox 2000.0, the plate quarter (a, b, c, or d), and the HES plate number. Example: For HE 0107−5240, which is located on quarter c of plate 2052 and at coordinates α = 01h09m29s.1, δ = −52◦24'34'', the HESid is HE0109291m522434c2052.meta.idcharindexednullablefieldField number in the ESO/SRC (or ESO/SERC) sky atlas.meta.id;obs.field49105.0506.0866.08941.0intplatePlate number of the HES objective prism plate in the ESO archive.meta.id;instr.plate11388.02042.09890.099221.0intquadrantHES plate quadrant (i.e., a, b, c, or d).meta.id;instr.platecharobjtypeMorphological source type [stars/ext/bright], discriminating between different extraction schemes used for the spectra, also impacting the sizes of the actual extraction apertures. 'stars' means point source, 'ext' means extended object (mostly galaxies), 'bright' means sources with partly saturated spectra, typically occuring for stars brighter than B_J ≈ 14 magsrc.classcharnullableraRight ascension for equinox J2000. The coordinates were derived from the DSS-I, and they are typically accurate to within 1 arcsec (rms).degpos.eq.ra;meta.main06.83417182.367354.8973601doublenullabledecDeclination for equinox J2000. The coordinates were derived from the DSS-I, and they are typically accurate to within 1 arcsec (rms).degpos.eq.dec;meta.main-77.3433-63.9478-24.63720.7458332.853891doublenullableovlBinary flag [0/1]. A value of 1 signals that the spectrum suffers contamination from another object located in dispersion direction.meta.code.qual00.00.01.011.0shortbj_dssMagnitude in the B_J band, measured on the relevant DSS-I plate and calibrated to a small number of reference stars.magphot.mag;em.opt.B-19.5212.0617.2519.921.241floatnullablesn_bjAverage signal to noise ratio per pixel of the HES spectra in the B_J band. See Christlieb et al. (2001, 2001A&A...366..898C) for a description of how this parameter was estimated.stat.snr01.896.1825.64309.661floatnullableb_v_hesApproximate B-V colour derived from the spectrum and calibrated against stellar samples with known multiband photometry. For details see Christlieb et al. (2001, 2001A&A...366..898C).magphot.color;em.opt.b;em.opt.v0floatnullableu_b_hesApproximate U-B colour derived from the spectrum and calibrated against stellar samples with known multiband photometry. For details see Christlieb et al. (2001, 2001A&A...366..898C).magphot.color;em.opt.u;em.opt.b0floatnullablemag_b_hesApproximate photographic magnitude in the Johnson B band derived by combining the B_J magnitude and the B-V colour.magphot.mag;em.opt.b0floatnullablestrc1Stroemgren c1 index measured in the HES spectrum.spect.index;em.opt-22.6-2.680.362.9214.440.969524floatnullablebalmsumSum of equivalent widths of Hbeta, Hgamma and Hdelta, measured in the HES spectrum by means of fits of Gaussians to these lines.spect.index;em.opt-99516-20.610.9818.069980101floatnullablekphesLine index for the Ca II K line measured in the HES spectrum (for details, see Christlieb et al. 2008, 2008A&A...484..721C).spect.index;em.opt-99851-64.927.799.449.450.999934floatnullablegphesLine index for the G band of CH measured in the HES spectrum (for details, see Christlieb et al. 2008, 2008A&A...484..721C).spect.index;em.opt-68524-8.484.4314.46902560.999999floatnullablec2idx1Band index for the C2 feature at 5165Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-89453-33.86-5.4330.071762670.999997floatnullablec2idx2Band index for the C2 feature at 4737Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-98398-39.280.7637.447055391floatnullablecnidx1Band index for the CN feature at 4216Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-98952-165.3-16.3359.153198370.999851floatnullablecnidx3Band index for the CN feature at 3883Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.uv-98841-71.84-1.2527.18849950.999914floatnullablehamburg_eso.meta The Hamburg/ESO survey (HES) is a digital objective prism survey covering the total southern extragalactic sky. It is based on Kodak IIIa-J plates which have been taken with the 1m ESO Schmidt telescope and its 4° prism. The spectral coverage is 3200-5300 Å, at an resolution of 15 Å at H gamma. The magnitude range covered is roughly between 18.5 and 11 mag in B_J. This is a collection of uniformly reduced spectra prepared by Norbert Christlieb. It is also intended as a sort-of resolver for HES names (“identifiers“) like ”HE 2301-7732”; unfortunately, these identifiers are not unique. You will need to apply domain knowledge in order to find the object actually being referred to when resolving an identifier of this sort.13000000accrefAccess key for the datameta.ref.urlAccess.ReferencecharindexednullableownerOwner of the datacharnullableembargoDate the data will become/became publicyrcharnullablemimeMIME type of the file servedmeta.code.mimeAccess.FormatcharnullableaccsizeSize of the data in bytesbyteVOX:Image_FileSizeAccess.Size1000010000.010000.010000.0100001.0longnullablessa_locationICRS location of aperture centerdegpos.eqssa:Char.SpatialAxis.Coverage.Location.Valuedoubleindexednullablessa_regionRough coverage based on location and aperture.pos.outline;obs.fielddoubleindexednullablehes_nameHES designation, consisting of the letters 'HE', the first four digits of the right ascension at equinox B1950.0, and the first four digits of the declination at equinox B1950.0. Example: HE 2301-7732.meta.id;meta.maincharindexednullablehes_idAlternative, more precise HES identifier consisting of the first seven digits of the right ascension at equinox 2000.0, the first six digits of the declination at equinox 2000.0, the plate quarter (a, b, c, or d), and the HES plate number. Example: For HE 0107−5240, which is located on quarter c of plate 2052 and at coordinates α = 01h09m29s.1, δ = −52◦24'34'', the HESid is HE0109291m522434c2052.meta.idcharindexednullablefieldField number in the ESO/SRC (or ESO/SERC) sky atlas.meta.id;obs.field49105.0506.0866.08941.0intplatePlate number of the HES objective prism plate in the ESO archive.meta.id;instr.plate11388.02042.09890.099221.0intquadrantHES plate quadrant (i.e., a, b, c, or d).meta.id;instr.platecharobjtypeMorphological source type [stars/ext/bright], discriminating between different extraction schemes used for the spectra, also impacting the sizes of the actual extraction apertures. 'stars' means point source, 'ext' means extended object (mostly galaxies), 'bright' means sources with partly saturated spectra, typically occuring for stars brighter than B_J ≈ 14 magsrc.classcharnullableraRight ascension for equinox J2000. The coordinates were derived from the DSS-I, and they are typically accurate to within 1 arcsec (rms).degpos.eq.ra;meta.main06.83417182.367354.8973601doublenullabledecDeclination for equinox J2000. The coordinates were derived from the DSS-I, and they are typically accurate to within 1 arcsec (rms).degpos.eq.dec;meta.main-77.3433-63.9478-24.63720.7458332.853891doublenullableovlBinary flag [0/1]. A value of 1 signals that the spectrum suffers contamination from another object located in dispersion direction.meta.code.qual00.00.01.011.0shortbj_dssMagnitude in the B_J band, measured on the relevant DSS-I plate and calibrated to a small number of reference stars.magphot.mag;em.opt.B-19.5212.0617.2519.921.241floatnullablesn_bjAverage signal to noise ratio per pixel of the HES spectra in the B_J band. See Christlieb et al. (2001, 2001A&A...366..898C) for a description of how this parameter was estimated.stat.snr01.896.1825.64309.661floatnullableb_v_hesApproximate B-V colour derived from the spectrum and calibrated against stellar samples with known multiband photometry. For details see Christlieb et al. (2001, 2001A&A...366..898C).magphot.color;em.opt.b;em.opt.v0floatnullableu_b_hesApproximate U-B colour derived from the spectrum and calibrated against stellar samples with known multiband photometry. For details see Christlieb et al. (2001, 2001A&A...366..898C).magphot.color;em.opt.u;em.opt.b0floatnullablemag_b_hesApproximate photographic magnitude in the Johnson B band derived by combining the B_J magnitude and the B-V colour.magphot.mag;em.opt.b0floatnullablestrc1Stroemgren c1 index measured in the HES spectrum.spect.index;em.opt-22.6-2.680.362.9214.440.969524floatnullablebalmsumSum of equivalent widths of Hbeta, Hgamma and Hdelta, measured in the HES spectrum by means of fits of Gaussians to these lines.spect.index;em.opt-99516-20.610.9818.069980101floatnullablekphesLine index for the Ca II K line measured in the HES spectrum (for details, see Christlieb et al. 2008, 2008A&A...484..721C).spect.index;em.opt-99851-64.927.799.449.450.999934floatnullablegphesLine index for the G band of CH measured in the HES spectrum (for details, see Christlieb et al. 2008, 2008A&A...484..721C).spect.index;em.opt-68524-8.484.4314.46902560.999999floatnullablec2idx1Band index for the C2 feature at 5165Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-89453-33.86-5.4330.071762670.999997floatnullablec2idx2Band index for the C2 feature at 4737Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-98398-39.280.7637.447055391floatnullablecnidx1Band index for the CN feature at 4216Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.opt-98952-165.3-16.3359.153198370.999851floatnullablecnidx3Band index for the CN feature at 3883Á measured in the HES spectrum (for details, see Christlieb et al. 2001, 2001A&A...375..366C).magspect.index;em.uv-98841-71.84-1.2527.18849950.999914floatnullabletaptestData for regression teststaptest.mainA table containing nonsensical data. Do not use except for experiments.radegpos.eq.ra;meta.mainfloatindexednullablededegpos.eq.dec;meta.mainfloatindexednullablespectralinstr.bandpasscharnullableucdc The Ultracool Dwarf Companion Catalogue consists of 278 multiple systems, 32 of which are newly discovered, each with at least one spectroscopically confirmed Ultracool Dwarf, within a 100 pc volume-limited sample. This catalogue is compiled using the Gaia Catalogue of Nearby Stars for stellar primaries and the Gaia Ultracool Dwarf Sample for low-mass companions and includes 241 doubles, 33 triples, and 4 higher-order systems established from positional, proper motion, and parallax constraints.ucdc.main The Ultracool Dwarf Companion Catalogue consists of 278 multiple systems, 32 of which are newly discovered, each with at least one spectroscopically confirmed Ultracool Dwarf, within a 100 pc volume-limited sample. This catalogue is compiled using the Gaia Catalogue of Nearby Stars for stellar primaries and the Gaia Ultracool Dwarf Sample for low-mass companions and includes 241 doubles, 33 triples, and 4 higher-order systems established from positional, proper motion, and parallax constraints.598sys_numIdentifier of the system in the UCDCmeta.id;meta.main19.91150.0274.02781.0intnum_compTotal number of objects that make up the systemmeta.number22.02.03.051.0shortnullableshort_nameShort (and unique) name used in this cataloguemeta.idcharnullablediscovery_nameKnown identifier from literaturemeta.id.crosscharnullablebd_refBinarity discovery bibcodemeta.bib.bibcodecharnullablesource_idUnique source identifier for Gaia DR3meta.id.cross15118286476804.59792466834312e+174.280400489214347e+186.707472532802898e+1869175289932832044801.0longnullablefppFalse-Positive Probability - Probability of the system being a False-Positive matchstat.fit.goodness1.37e-104.7591e-094.89e-050.0285690.07730.464883floatnullableang_sepAngular Separation between companion and the ultracool dwarfarcsecpos.angDistance0.0870.7218758.26971696.952404.710.531773floatnullableprojected_sepProjected physical separation between companion and the ultracool dwarfAUpos.distance1.0597518.301237592885.9992210.528428floatnullableplx_diffDifference in Parallax between companion and the ultracool dwarfmaspos.parallax;arith.diff1.65e-060.0020840.4012834.094116.8980.523411floatnullablepm_diffProper Motion difference between companion and the ultracool dwarf, absolute valuemas/apos.pm;arith.diff1e-060.2011094.4807338.431356.06930.523411floatnullablepma_diffProper Motion difference between companion and the ultracool dwarf, position angledegpos.posAng;arith.diff1e-060.01737610.7744469.8377811.7950.520067floatnullableraRight Ascension from epoch_refdegpos.eq.ra;meta.main0.825896.1841192.563346.932358.5371doubleindexednullabledecDeclination from epoch-refdegpos.eq.dec;meta.main-81.7629-68.148217.010263.45885.44871doubleindexednullableepochEpoch of object positionatime.epoch1997.81999.982016.52016.52016.51floatnullableepoch_refBibcode for the source of the epoch positionmeta.bib.bibcode;poscharnullableparallaxParallax taken from parallax_refmaspos.parallax8.179579.7260721.9315101.316274.841floatnullableparallax_errError in parallaxmasstat.error;pos.parallax0.009260.01458840.174732.510116.71floatnullableparallax_refBibcode for the source of the parallax valuemeta.bib.bibcode;pos.parallaxcharnullablepmraProper motion in Right Ascension from pm_refmas/apos.pm;pos.eq.ra-1159.52-619.945-39.1145373.2993981.981floatnullableerr_pmraError in the proper motion in Right Ascensionmas/astat.error;pos.pm;pos.eq.ra-112.50.01111160.1884652.8101.40.993311floatnullablepmdecProper motion in Declination from pm_refmas/apos.pm;pos.eq.dec-2536.19-704.947-46.561232.519695.9561floatnullableerr_pmdecError in proper motion in Declinationmas/astat.error;pos.pm;pos.eq.dec0.008760.01357850.1652.7033592.60.993311floatnullablepm_refBibcode for the source of the proper motionsmeta.bib.bibcode;pos.pmcharnullablemag_gG-band mean magnitudemagphot.mag;em.opt.V4.0616.8198916.876620.748521.07770.897993floatnullableerr_mag_gError in G-band mean magnitudemagstat.error;phot.mag;em.opt.V9.2e-050.000187320.0015610.01188440.0298720.897993floatnullablemag_rpRP mean magnitudemagphot.mag;em.opt.R3.95166.1327215.361719.16519.91210.869565floatnullableerr_mag_rpError in RP mean magnitudemagstat.error;phot.mag;em.opt.R0.0001640.0003260.0040710.06945050.1587610.87291floatnullablemag_g_rpG-RP colourmagphot.color;em.opt.V;em.opt.R-0.23250.4069311.431241.908372.44770.869565floatnullablemag_j2MASS J-band mean magnitudemagphot.mag;em.ir.j3.6635.3112513.12216.64325.420.822742floatnullableerr_mag_jError in 2MASS J-band mean magnitudemagstat.error;phot.mag;em.ir.j0.010.0190.0290.210421.20.814381floatnullablemag_h2MASS H-band mean magnitudemagphot.mag;em.ir.h3.0855.0965212.45615.790925.290.817726floatnullableerr_mag_hError in 2MASS H-band mean magnitudemagphot.mag;em.ir.h0.0150.0180.03450.170250.2560.812709floatnullablemag_k2MASS K_s-band mean magnitudemagphot.mag;em.ir.K3.0485.0115212.10215.317418.970.811037floatnullableerr_mag_kError in 2MASS K_s-band mean magnitudemagstat.error;phot.mag;em.ir.K0.0140.0160.0270.1549.9950.804348floatnullablesptoptOptical Spectral Type from sptopt_refsrc.sptypecharnullablesptopt_refReference for the optical spectral typemeta.bib.bibcode;src.sptypecharnullablesptnirNear Infrared Spectral Type from sptnir_refsrc.sptypecharnullablesptnir_refReference for the near infrared spectral typemeta.bib.bibcode;src.sptypecharnullableastrometric_n_obs_alTotal number of observations in the along the Gaia scan (AL) directionmeta.number66148.16343.0662.43999999999978160.8979933shortnullablephot_g_n_obsNumber of observations contributing to G photometrymeta.number0159.05370.5685.84999999999988650.89632106shortnullablephot_rp_n_obsNumber of observations contributing to RP photometrymeta.number03.050000000000000739.076.0940.89632106shortnullablephot_rp_n_blended_transitsNumber of RP blended transitsmeta.number00.00.045.29000000000002930.8695652shortnullableruweRenormalised Unit Weight Errorstat.error0.6599830.9106291.0941713.700246.03790.884615floatnullableluweLocal Unit Weight Error as per 2022MNRAS.513.5270Pstat.error2.116152.209975.8182626.866634.86980.0468227floatnullableipd_gof_harmonic_amplitudeAmplitude of the IPD GoF versus position angle of scandegstat.value0.0013390.004179750.0212340.1756940.4314050.896321floatnullableipd_frac_multi_peakPercent of successful-IPD windows with more than one peak%stat.value00.00.056.74999999999966950.89632106shortnullablervRadial Velocity from rv_refkm/sphys.veloc;pos.heliocentric-214.18-71.115-3.6309543.37461770.434783floatnullableerr_rvError in radial velocitykm/sstat.error;phys.veloc;pos.heliocentric000.5919.944500.423077floatnullablerv_refBibcode of the source of rvmeta.bib.bibcode;phys.veloc;pos.heliocentriccharnullablev_tanTangential Velocitykm/sphys.veloc.transverse3.896576.7450132.310598.3736402.6090.983278floatnullablet_effEffective temperature from t_eff_refKphys.temperature.effective1395.291902.112553.486053.3910146.80.56689floatnullableerr_t_eff_lowerLower error in effective temperatureKstat.error;phys.temperature.effective2858.32999.084562.16334.4410113.40.219064floatnullableerr_t_effupperUpper error in effective temperatureKstat.error;phys.temperature.effective2874.53000.274569.16338.7610176.60.219064floatnullableerr_t_eff_espucdError in T_eff from ESP-UCDKstat.error;phys.temperature.effective1.665.220556.935307.0612744.40.347826floatnullablet_eff_ref1 = GSP-Phot, 2 = ESP-UCDmeta.bibcharnullablelogg_gspphotSurface gravity from GSP-Phot (DR3) (Median of MCMC values)log(cm/s**2)phys.gravity3.75773.922014.48425.08125.14460.227425floatnullableerr_logg_gspphot_lowerLower error in Surface gravitylog(cm/s**2)stat.error;phys.gravity3.75463.901384.47035.057885.14130.227425floatnullableerr_logg_gspphotupperUpper error in Surface gravitylog(cm/s**2)stat.error;phys.gravity3.763.954814.5135.081895.1450.227425floatnullablemh_gspphotIron abundance from GSP-Phot (DR3) (Median of MCMC values, log relative to solar)phys.abund.Fe-1.6294-1.03184-0.19750.3963720.4650.229097floatnullableerr_mh_gspphot_lowerLower error in Iron abundancestat.error;phys.abund.Fe-1.6332-1.05148-0.233150.3486350.42350.227425floatnullableerr_mh_gspphotupperUpper error in Iron abundancestat.error;phys.abund.Fe-1.6216-0.889515-0.183550.455390.51470.227425floatnullableluminosityBolometric luminositysolLumphys.luminosity-6.383-4.68724-3.415-2.88328-2.5560.128763floatnullableerr_luminosity_lowerLower error in Bolometric luminositysolLumstat.error;phys.luminosity-6.531-4.80125-3.493-2.9285-2.60.12709floatnullableerr_luminosityupperUpper error in Bolometric luminositysolLumstat.error;phys.luminosity-6.234-4.598-3.334-2.837-2.5120.12709floatnullablemassMass of the object from mass_refsolMassphys.mass0.00670.012050.6541.3712.2420.210702floatnullableerr_mass_lowerLower error in object masssolMassstat.error;phys.mass0.00770.0101010.080850.706390.8390.09699floatnullableerr_massupperUpper error in object masssolMassstat.error;phys.mass0.00910.0112750.084850.71290.740.09699floatnullablemass_refMass reference: 1 = gaia FLAME, 2 = White Dwarf, 3 = BANYAN Sigmameta.bibcharnullableageAge of the object from age_refGyrtime.age0.010.0352.1812.894713.3240.254181floatnullableerr_age_lowerLower error in Age of the objectGyrstat.error;time.age0.0070.030.6510.0311.7510.254181floatnullableerr_ageupperUpper error in Age of the objectGyrstat.error;time.age0.0130.043.4213.513.660.254181floatnullableage_refAge reference: 1 = gaia FLAME, 2 = White Dwarf, 3 = BANYAN Sigmameta.bibcharnullableveronqsos This catalogue (with updates to the pervious version) contains 11358 (+2759) quasars (defined as brighter than absolute B magnitude -23), 3334 (+501) AGNs (defined as fainter than absolute B magnitude -23) and 357 (+137) BL Lac objects from 1863 (+201) references.veronqsos.data This catalogue (with updates to the pervious version) contains 11358 (+2759) quasars (defined as brighter than absolute B magnitude -23), 3334 (+501) AGNs (defined as fainter than absolute B magnitude -23) and 357 (+137) BL Lac objects from 1863 (+201) references.11358notradio'*' if not detected in radiometa.notecharnullablenameMost common name of the objectmeta.idcharnullableraj2000Right Ascension J2000degpos.eq.ra;meta.main0.01177.33856160.019348.038359.9971doubleindexednullabledej2000Declination J2000degpos.eq.dec;meta.main-83.0161-47.8081-1.77657.935785.19891doubleindexednullablen_rahPosition origin: O=optical, R=radio, A=approximativemeta.notecharnullablel_z*=redshift from slitless spectroscopymeta.code.errorcharnullablezRedshiftsrc.redshift0.030.2631.773.14.8970.994981floatnullablespSpectrum classificationsrc.spTypecharnullablen_vmag'*' for photographic, 'R' for red Vmagmeta.notecharnullablevmagmagnitude, V or other (see n_Vmag)magphot.mag;em.opt.V12.1916.218.82520.9531240.979398floatnullabler_zReference of the redshiftmeta.ref11100.0729.01785.018601.0shortnullablevlastripe82 This is a high-resolution radio survey of the Sloan Digital Sky Survey (SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey was conducted with the Very Large Array (VLA) primarily in the A-configuration, with supplemental B-configuration data to increase sensitivity to extended structure. The survey has an angular resolution of 1.''8 and achieves a median rms noise of 52 μJy per beam over 92 deg^2. The catalog contains 17,969 isolated radio components, for an overall source density of ∼195 sources/deg^2. See also J.A. Hodge et al, :bibcode:`2011AJ....142....3H` .vlastripe82.stripe82 This is a high-resolution radio survey of the Sloan Digital Sky Survey (SDSS) Southern Equatorial Stripe, a.k.a. Stripe 82. This 1.4 GHz survey was conducted with the Very Large Array (VLA) primarily in the A-configuration, with supplemental B-configuration data to increase sensitivity to extended structure. The survey has an angular resolution of 1.''8 and achieves a median rms noise of 52 μJy per beam over 92 deg^2. The catalog contains 17,969 isolated radio components, for an overall source density of ∼195 sources/deg^2. See also J.A. Hodge et al, :bibcode:`2011AJ....142....3H` .17969raj2000Right Ascension, J2000degpos.eq.ra;meta.main9.8081711.06232.6184348.932350.1821doubleindexednullabledej2000Declination, J2000degpos.eq.dec;meta.main-1.39151-1.212730.0009555561.218081.4011doubleindexednullablep_sProbability that the source is spurious (e.g., because of a sidelobe of a nearby bright source).stat.likelihood;obs0.0140.0140.1620.70.8771floatnullablef_peakPeak flux density derived by fitting an elliptical Gaussian model to the source. The uncertainty is given in the rms_nose column.mJy/beamphot.flux.density;em.radio.1500-3000MHz;stat.max0.30.320.7417.0181838.761floatindexednullablef_intIntegrated flux density in mJy derived from the elliptical Gaussian model fit.mJyphot.flux.density;em.radio.1500-3000MHz0.120.341.6934.9762348.241floatnullablerms_noiseLocal noise estimate at the source position, calculated by combining the measured noise from all grid images contributing to the coadded map at the source position.mJystat.error;phot.flux.density0.0360.0520.0640.37515.0581floatnullablesmaj_axFWHM semimajor axis of the elliptical Gaussian model for the source after beam deconvolution. This is zero when the fitted value prior to deconvolution to is smaller than the beam (1.8'') due to noise.degphys.angSize.smajAxis;meta.modelled000.0002444440.001083330.00828751floatnullablesmin_axFWHM semiminor axis of the elliptical Gaussian model for the source after beam deconvolution. This is zero when the fitted value prior to deconvolution to is smaller than the beam due to noise.degphys.angSize.sminAxis;meta.modelled000.0001486110.0006693890.002931941floatnullablepaPosition angle of the elliptical Gaussian model for the source after beam deconvolution, east of north.degpos.posAng;meta.modelled00901801801floatnullablesmaj_ax_rawFWHM semimajor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.smajAxis0.000150.0002472220.000350.001112440.008291671floatnullablesmin_ax_rawFWHM semiminor axis of the elliptical Gaussian model before beam deconvolution.degphys.angSize.sminAxis0.0001472220.0001902780.0002902780.0007152220.002943061floatnullablepa_rawPosition angle of the elliptical Gaussian model for the source before beam deconvolution, east of north.degpos.posAng00901801801floatnullablefieldThe field name is the name of the coadded image containing the source. Note that the field name encodes the center of the field; field hhmmm+ddmmm is centered at RA = hh mm.m, Dec = +dd mm.m. The letter appended to the field name indicates the last catalog release in which the image was modified.meta.id;obs.fieldcharnullablen_sdssNumber of matching SDSS DR6 objects within 8 arcsec.meta.number00.01.04.0251.0intd_sdssSeparation of the closest match in SDSS DR6.degpos.angDistance00.050.557.5180.554566floatnullableimagSDSS i-band magnitude of the closest match in SDSS DR6.magphot.mag;em.opt.I-114.339220.3323.3928.10.554566floatindexednullablec_sdssSDSS morphological class of the closest match in SDSS DR6; s = stellar, g = nonstellar/galaxy.src.morph.typecharnullablectRow count; this is not part of the original table but was added to satisfy SCS requirements.meta.id;meta.main0539.048984.017428.96179681.0int