Further access options are discussed below
For a list of all services and tables belonging to this service's resource, see Information on resource 'The Henry Draper Catalog with Gaia IDs'
This resource grew out of the realisation just how hard it is to do useful things with HD numbers in the VO. In provides the original Henry Draper catalog together with Gaia DR2 source ids for the stars identified in Fabricius et al's Tycho 2-HD match (2002A&A...386..709F)
It was generated as follows (cf. sources):
create a database table for the HD catalog with empty columns for the Gaia counterparts. While doing this, precess the B1900 positions to J2000. We haven't bothered with diffrences in the reference catalogs; at the 1 arcminute precision of the HD, this doesn't matter at all. All astrometry coming from HD is for debugging only.
Get a mapping from HD numbers to standard Tycho-2 ids from VizieR:
select HD, n_HD, n_TYC, TYC1 || '-' || TYC2 || '-' || TYC3 as tycho_id from "IV/25/tyc2_hd"
Turn the Tycho 2 identifier to a Gaia DR2 source_id using the dr2_tycho_best_neighbour table. It does not exist on VizieR, so we used the ARI-Gaia service:
select hd, n_hd, n_tyc, source_id from gaiadr2.tycho2_best_neighbour join TAP_UPLOAD.tyc on (tycho_id=original_ext_source_id)
After this procedure, HD 45900, HD 260686, and HD 121169 did not have unique matches. It seemed excessive to complicate the data model just for these three objects. We have randomly dropped one possible match for each of them; in addition, HD 121169 should have had an second match, which did not work out in Gaia DR2. These doubtful cases can be identified by n_TYC=2.
Add a Gaia eDR3 source_id by matching the DR2 source_id gaiaedr3.dr2neighbourhood. This frequently has multiple eDR3 objects for a DR2 source_id. In this case, we blindly chose the brightest match, ignoring, for instance, component information that might be present in the DM number. Again, relatively close binaries may be trouble in this catalogue.
Complete the source_id, gaia_ra, gaia_dec, n_hd, and n_tyc columns of the table created in step (a) with the data obtained in steps (c) and (d) using the local edr3lite table.
You can access this service using:
This service is published as follows:
local means it is listed on our front page, ivo_managed means it has a record in the VO registry.
The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
DEC | Delta (ICRS) | Declination (ICRS decimal) | deg | pos.eq.dec |
hd | Hd | HD number for this object | N/A | meta.id;meta.main |
hscs_pos | Position/Name | Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object | N/A | N/A |
hscs_sr | Search radius | Search radius in arcminutes | N/A | N/A |
m_v | m_V | Photovisual magnitude or the star, except for magnitudes >= 20, which are object type flags (see note). | mag | phot.mag;em.opt.V |
maxrec | Match limit | Maximum number of records returned. Pass 0 to retrieve service parameters. | N/A | N/A |
RA | Alpha (ICRS) | Right Ascension (ICRS decimal) | deg | pos.eq.ra |
responseformat | Output Format | File format requested for output. | N/A | meta.code.mime |
spectral | Spectral | Spectral type, given in upper and lower case as in the published catalog. | N/A | src.sptype |
SR | Search Radius | Search radius | deg | N/A |
verb | Verbosity | Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. | N/A | N/A |
The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
_r | Dist. | Distance to cone center | deg | pos.distance |
dm | DM | Durchmusterung 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. Note d | N/A | meta.id.cross |
gaia_dec | Dec Gaia | ICRS Declination from Gaia eDR3 (i.e., Epoch J2016) | deg | pos.eq.dec;meta.main |
gaia_ra | RA Gaia | ICRS Right Ascension from Gaia eDR3 (i.e., Epoch J2016) | deg | pos.eq.ra;meta.main |
hd | Hd | HD number for this object | N/A | meta.id;meta.main |
m_pg | m_pg | Photographic magnitude or the star, except for magnitudes >= 20, which are object type flags (see note). Note m | mag | phot.mag;em.opt.B |
m_v | m_V | Photovisual magnitude or the star, except for magnitudes >= 20, which are object type flags (see note). Note m | mag | phot.mag;em.opt.V |
mpg_comb | Comb? | C if m_pg is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise. | N/A | meta.code |
mv_comb | Comb? | C if m_v is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise. | N/A | meta.code |
n_hd | #HD | Number of HD stars matched to a Tycho 2 source by Fabricius et al, 2002A&A...386..709F. | N/A | meta.number |
n_tyc | #Tyc | Number of Tycho 2 stars matched to a HD source by Fabricius et al, 2002A&A...386..709F. | N/A | meta.number |
remarks | Rem | Remarks. See note for what the letters mean. Note r | N/A | meta.code |
source_id | DR2 source_id | Gaia 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). | N/A | meta.id.cross |
source_id3 | Gaia source_id | Gaia 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. | N/A | meta.id.cross |
spectral | Spectral | Spectral type, given in upper and lower case as in the published catalog. | N/A | src.sptype |
The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.
Name | Table Head | Description | Unit | UCD | Verb. Level |
---|---|---|---|---|---|
hd | Hd | HD number for this object | N/A | meta.id;meta.main | 1 |
spectral | Spectral | Spectral type, given in upper and lower case as in the published catalog. | N/A | src.sptype | 1 |
source_id3 | Gaia source_id | Gaia 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. | N/A | meta.id.cross | 1 |
m_v | m_V | Photovisual magnitude or the star, except for magnitudes >= 20, which are object type flags (see note). Note m | mag | phot.mag;em.opt.V | 5 |
m_pg | m_pg | Photographic magnitude or the star, except for magnitudes >= 20, which are object type flags (see note). Note m | mag | phot.mag;em.opt.B | 5 |
gaia_ra | RA Gaia | ICRS Right Ascension from Gaia eDR3 (i.e., Epoch J2016) | deg | pos.eq.ra;meta.main | 5 |
gaia_dec | Dec Gaia | ICRS Declination from Gaia eDR3 (i.e., Epoch J2016) | deg | pos.eq.dec;meta.main | 5 |
_r | Dist. | Distance to cone center | deg | pos.distance | 10 |
dm | DM | Durchmusterung 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. Note d | N/A | meta.id.cross | 15 |
mv_comb | Comb? | C if m_v is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise. | N/A | meta.code | 15 |
mpg_comb | Comb? | C if m_pg is a combined magnitude (with a neighbouring star given in this catalogue), NULL otherwise. | N/A | meta.code | 15 |
remarks | Rem | Remarks. See note for what the letters mean. Note r | N/A | meta.code | 15 |
n_hd | #HD | Number of HD stars matched to a Tycho 2 source by Fabricius et al, 2002A&A...386..709F. | N/A | meta.number | 15 |
n_tyc | #Tyc | Number of Tycho 2 stars matched to a HD source by Fabricius et al, 2002A&A...386..709F. | N/A | meta.number | 15 |
source_id | DR2 source_id | Gaia 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). | N/A | meta.id.cross | 15 |
ra_orig | Ra_orig | Original right ascension for equinox J1900.0. Note that this position is only good to about an arcminute. | N/A | pos.eq.ra | 21 |
dec_orig | Dec_orig | Original declination for equinox J1900.0. Note that this position is only good to about an arcminute. | N/A | pos.eq.dec | 21 |
ra_orig_2000 | Ra_orig_2000 | Original right ascension for equinox J2000.0 (precession done by DC staff). Note that this position is only good to about an arcminute. | N/A | pos.eq.ra | 21 |
dec_orig_2000 | Dec_orig_2000 | Original declination for equinox J2000.0 (precession done by DC staff). Note that this position is only good to about an arcminute. | N/A | pos.eq.dec | 21 |
mv_meas | m_V? | '0' if the m_v is a measured value, '1' if it's a value inferred from m_pg and the spectral type. | N/A | meta.code | 25 |
mpg_meas | Meas? | '0' if the m_pg is a measured value, '1' if it's a value inferred from m_v and the spectral type. | N/A | meta.code | 25 |
pg_intensity | Intensity | Photographic 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. | N/A | meta.code.qual | 25 |
VOResource XML (that's something exclusively for VO nerds)
The Durchmusterung identifier includes, in place 10, a component identifier if there are two or more HD stars with the same DM number. For multiple systems included in the Washington Catalog of Visual Double Stars (WDS, Worley 1984) the same designations are given.
In place 11, there is a lower case letter identification for BD supplemental stars (Warren and Kress 1980).
The following special values photovisual magnitude indicate unusual object types:
20.0 | nebula (Neb in published catalog) |
30.0 | variable (var. in published catalog) |
40.0 | nova (Nov. in published catalog) |
50.0 | cluster (Cl. in published catalog) |
NULL | no value in published catalog |
The following codes are used in the remarks: