Table Description:
This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
For a list of all services and tables belonging to this table's resource, see Information on resource 'Gaia early DR3 Mock Catalogue (gedr3mock)'
Resource Reference URL: http://dc.zah.uni-heidelberg.de/tableinfo/gedr3mock.main
This table has an associated publication. If you use data from it, it may be appropriate to reference 2020PASP..132g4501R (ADS BibTeX entry for the publication) either in addition to or instead of the service reference.
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:gedr3mock_genera, year=2019, title={Gaia early DR3 Mock Catalogue (gedr3mock)}, author={Rybizki, J. and Demleitner, M. and Bailer-Jones, C. and Tio, P. D. and Cantat-Gaudin, T. and Fouesneau, M. and Chen, Y. and Andrae, R. and Girardi, L. and Sharma, S.}, url={https://dc.zah.uni-heidelberg.de/tableinfo/gedr3mock.generated_data}, howpublished={{VO} resource provided by the {GAVO} Data Center}, doi = {10.21938/dBrplG8I1KR7RyfkMXTyYA} }
Sorted alphabetically. [Sort by DB column index]
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
a0 | A_0 | monochramatic Extinction at lambda=547.7nm | mag | N/A |
a_bp | A_BP | Extinction in BP | mag | N/A |
a_g | A_G | Extinction in G | mag | N/A |
a_rp | A_RP | Extinction in RP | mag | N/A |
a_rvs | A_RVS | Extinction in RVS | mag | N/A |
age | Age | Age of the star | Gyr | N/A |
b | b | Galactic latitude | deg | N/A |
d11y | Det% | [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). | N/A | stat.likelihood;obs |
dec | Dec (ICRS) | Barycentric Declination in ICRS at ref_epoch | deg | pos.eq.dec;meta.main |
feh | [Fe/H] | log of metallicity in solar units ('dex') | N/A | N/A |
index_parsec | Phot. | [GeDR3mock only] Foreign key into the photometry/extinction table, . | N/A | meta.id.cross |
l | l | Galactic longitude | deg | N/A |
logg | log(g) | Surface gravity of star | log(cm/(s**2)) | N/A |
lum | Luminosity | Stellar luminosity | solLum | N/A |
mact | Mass_actual | actual (present) mass in solar masses | solMass | N/A |
parallax | parallax | parallax in mas | mas | N/A |
parallax_error | error_parallax | parallax uncertainty in mas | mas | N/A |
phot_bp_mean_mag | BP | apparent BP mag including extinction | mag | N/A |
phot_g_mean_mag | G | apparent G mag including extinction | mag | N/A |
phot_g_mean_mag_error | error_G | error in G | mag | N/A |
phot_g_n_obs | Nobs | Number of photometric observations (trained from DR2 scaled to DR3 time) | N/A | N/A |
phot_rp_mean_mag | RP | apparent RP mag including extinction | mag | N/A |
phot_rvs_mean_mag | RVS | apparent RVS mag including extinction | mag | N/A |
pm_dec | pm_delta | Proper motion in declination | mas/yr | N/A |
pm_ra | pm_alpha | Proper motion in projection of right ascension | mas/yr | N/A |
popid | PopID | Population ID according to the Besancon model. Including SMC/LMC = 10 and stellar clusters = 11 | N/A | N/A |
ra | RA (ICRS) | Barycentric Right Ascension in ICRS at ref_epoch | deg | pos.eq.ra;meta.main |
radial_velocity | V_rad | Radial velocity in km/s | km/s | N/A |
radial_velocity_error | error_rvs | Radial velocity uncertainty in km/s | km/s | N/A |
random_index | Random | Random index that can be used to deterministically select subsets | N/A | N/A |
smass | Mass_initial | initial mass in solar masses | solMass | N/A |
source_id | ID | Healpix 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. | N/A | meta.id;meta.main |
teff | Teff | effective Temperature | K | N/A |
visibility_periods_used | VPU | Number of observations effectively used for the astrometric solutions (trained from DR2 scaled to DR3) | N/A | N/A |
Columns that are parts of indices are marked like this.
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