RAdial Velocity Experiment: RAVE DR5rave.mainivo://org.gavo.dc/rave/q/mainThe GAVO DC teamKordopatis,G.Gilmore, G.Steinmetz, M.Boeche, C.Seabroke, G.M.Siebert, A.Zwitter, T.Binney, J.de Laverny, P.Recio−Blanco, A.Williams, M.E.K.Piffl, T.Enke, H.Roeser, S.Bijaoui, A.Wyse, R.F.G.Freeman, K.Munari, U.Carillo, I.Anguiano, B.Burton, D.Campbell, R.Cass, C.J.P.Fiegert, K.Hartley, M.Parker, Q.A.Reid, W.Ritter, A.Russell, K.S.Stupart, M.Watson, F.G.Bienayme, ́O.Bland−Hawthorn, J.Gerhard, O.Gibson, B.K.Grebel, E.K.Helmi, A.Navarro, J.F.Conrad, C.Famaey, B.Faure, C.Just, A.Kos, J.Matijevic, G.McMillan, P.J.Minchev, I.Scholz, R.Sharma, S.Siviero, A.Wylie de Boer, E.Zerjal, M.2016-09-22T00:00:00ZData Release 5GAVO Data Center TeamMönchhofstrasse 12-14, D-69120 Heidelberggavo@ari.uni-heidelberg.de++49 6221 54 1837surveysstarsradial-velocitymilky-way-galaxyThe 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.http://dc.zah.uni-heidelberg.de/tableinfo/rave.mainUK Schmidt AAO6dF0/8,11 1/16,24,42-43
2/68,72,80,82,88,100,104,113,120,144,146,149,151-152,154,156-157,159-160,162,165
3/7,276-278,280-282,292-294,296,324-326,332,335,340,356,360-362,367,404,406,408,410,420-422,424-426,448,450-451,458,464-465,468-469,484-485,488-490,580-582,588,590,592-593,595,601-603,612,614,620,622,632-633,635,644-645,656-657,659,667,670-671
4/0-1,27,256,265,267-268,270,282,285,292-293,295,514,552,576,776,809,814,1116-1118,1136,1180-1181,1188-1190,1192-1194,1196,1207-1209,1216,1308,1310,1332,1334-1335,1338,1344-1345,1347-1349,1351,1357,1365,1368,1370,1374,1377,1379,1382,1386,1428-1430,1432-1434,1436,1452,1454,1456,1460,1463,1506,1512,1620-1622,1636-1638,1648,1653-1654,1659,1692,1708,1710,1728,1796-1798,1825,1829,1838-1841,1844,1850-1851,1854,1864-1865,1868-1870,1880-1881,1887-1888,1890,1893,1908,1944-1946,1964-1965,1968,1976,1992,2332-2334,2356,2358,2364,2376-2377,2379,2401-2403,2455,2463,2485-2487,2492-2494,2536-2537,2539,2584-2586,2588-2589,2591,2610,2618-2619,2621-2623,2632,2635,2656-2657,2660,2664,2666-266752741 56386OpticalraveRAdial Velocity Experiment: RAVE DR5 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.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.maindoubleindexednullabledej2000Declination (J2000.0)degpos.eq.dec;meta.maindoubleindexednullableglonGalactic longitudedegpos.galactic.londoublenullableglatGalactic latitudedegpos.galactic.latdoublenullablervHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloatindexednullablee_rvError in heliocentric radial velocitykm/sstat.error;spect.dopplerVeloc;pos.heliocentricfloatnullableobsdateObservation date.dtime.epoch;obsdoublenullablefield_nameName of RAVE field (RA/DE)meta.id;obs.fieldcharnullableplate_numberNumber of field plate [1..3]meta.id;obs.fieldshortfiber_numberNumber of optical fiber used to obtain the spectrum [1,150].meta.number;instr.setupshortteff_kEffective temperature from the stellar parameter pipeline.Kphys.temperature.effectivefloatnullablee_teff_kError in the effective temperature from the stellar parameter pipeline.Kstat.error;phys.temperature.effectivefloatnullablelogg_kLog gravity as determined by the stellar pipeline.phys.gravityfloatnullablee_logg_kError in logg_k.stat.error;phys.gravityfloatnullablemet_kMetallicity [m/H] from the stellar parameter pipeline.phys.abund.Zfloatnullablemet_n_kCalibrated metallicity [m/H] from the stellar parameter pipeline.phys.abund.Zfloatnullablee_met_kError in metallicity [m/H] from the stellar parameter pipeline.stat.error;phys.abund.Zfloatnullablesnr_kSignal to noise value for the stellar parameter pipeline.stat.snrfloatindexednullablealgo_conv_kQuality flag for stellar parameter pipeline [0..4].meta.code.qualfloatnullablealAbundance of Al [Al/H]phys.abundfloatnullableal_nNumber of spectral lines used for the computation of Al abundance.phys.abundintnullablesiAbundance of Si [Si/H]phys.abundfloatnullablesi_nNumber of spectral lines used for the computation of Si abundance.phys.abundintnullablefeAbundance of Fe [Fe/H]phys.abund.Fefloatnullablefe_nNumber of spectral lines used for the computation of Fe abundance.phys.abundintnullabletiNumber of spectral lines used for the computation of Ti abundance.phys.abundfloatnullableti_nNumber of used spectral lines for calculation of Ti abundance.phys.abundintnullableniAbundance of Ni [Ni/H]phys.abundfloatnullableni_nNumber of spectral lines used for the computation of Ni abundance.phys.abundintnullablemgAbundance of Mg [Mg/H]phys.abundfloatnullablemg_nNumber of spectral lines used for the computation of Mg abundance.phys.abundintnullablejmag2MASS J magnitudemagphot.mag;em.IR.Jfloatindexednullablee_jmag2MASS J total magnitude uncertaintymagstat.error;phot.mag;em.IR.Jfloatnullablehmag2MASS H magnitudemagphot.mag;em.IR.Hfloatnullablee_hmag2MASS H total magnitude uncertaintymagstat.error;phot.mag;em.IR.Hfloatnullablekmag2MASS K_s magnitudemagphot.mag;em.IR.Kfloatnullablee_kmag2MASS K_s total magnitude uncertaintymagstat.error;phot.mag;em.IR.Kfloatnullablechisq_cχ² of the Chemical Pipelinestat.fit.chi2floatnullableid_2mass2MASS Target designationmeta.idcharnullableid_denisDENIS Target designationmeta.idcharnullableid_usnob1USNOB1 Target designationmeta.idcharnullableid_tycho2TYCHO2 target designationmeta.idcharnullableid_ucac4UCAC4 target designationmeta.idcharnullableid_ppmxlPPMXL target designation.meta.idlongnullableparallaxParallax (from 2014MNRAS.437..351B)maspos.parallaxfloatnullablee_parallaxError Parallax (from 2014MNRAS.437..351B)masstat.error;pos.parallaxfloatnullabledist_binneyDistance (from 2014MNRAS.437..351B)kpcpos.distancefloatnullablee_distError in Distance (from 2014MNRAS.437..351B)kpcstat.error;pos.distancefloatnullabledistance_modulusDistance modulus (from 2014MNRAS.437..351B)phot.mag.distModfloatnullablee_distance_modulusDistance modulus (from 2014MNRAS.437..351B)stat.error;phot.mag.distModfloatnullablelog_avExtinction (from 2014MNRAS.437..351B)phys.absorptionfloatnullablee_log_avError in extinction (from 2014MNRAS.437..351B)stat.error;phys.absorptionfloatnullablemin_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.heliocentricfloatnullablemad_rvMedian absolute deviation in HRV from 10 resampled spectrakm/sstat.fit.residual;spect.dopplerVeloc;pos.heliocentric;stat.medianfloatnullablestddev_teff_kStandard deviation in Teff_K from 10 resampled spectraKstat.stdev;phys.temperature.effectivefloatnullablemad_teff_kMedian absolute deviation in Teff_K from 10 resampled spectraKstat.fit.residual;phys.temperature.effective;stat.medianfloatnullablestddev_logg_kStandard deviation in Teff_K from 10 resampled spectrastat.stdev;phys.gravityfloatnullablemad_logg_kMedian absolute deviation in metallicity from 10 resampled spectrastat.fit.residual;phys.abund.Z;stat.medianfloatnullablestddev_met_kStandard deviation in metallicity from 10 resampled spectrastat.stdev;phys.abund.Zfloatnullablechisq_kχ² of the Stellar Parameter Pipelinestat.fit.chi2floatnullableteff_irEffective temperature from infrared flux methodKphys.temperature.effectivefloatnullablee_teff_irError in the effective temperature from infrared flux methodKstat.error;phys.temperature.effectivefloatnullableir_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.abundfloatnullablefrac_cFraction of spectrum used for calculation of abundancesstat.valuefloatnullableav_schlegelTotal Extinction in V-band from 1998ApJ...500..525Smagphys.absorptionfloatnullablen_gauss_fitNumber of components required for multi-Gaussian distance modulus fit.meta.numbershortnullablegauss_mean_1Gaussian number 1 in the estimated PDF of the object distance, width.stat.fit.paramfloatnullablegauss_frac_1Gaussian number 1 in the estimated PDF of the object distance, weight.stat.fit.paramfloatnullablegauss_mean_2Gaussian number 2 in the estimated PDF of the object distance, width.stat.fit.paramfloatnullablegauss_frac_2Gaussian number 2 in the estimated PDF of the object distance, weight.stat.fit.paramfloatnullablegauss_mean_3Gaussian number 3 in the estimated PDF of the object distance, width.stat.fit.paramfloatnullablegauss_frac_3Gaussian number 3 in the estimated PDF of the object distance, weight.stat.fit.paramfloatnullablerep_flagTrue if the object was observed multiple timesmeta.code.qualbooleancluster_flagTrue if this was a targeted cluster observationmeta.code.qualbooleanid_tgasTGAS target designationmeta.id.crosslongnullable