ivo://org.gavo.dc/gedr3mock/q/pubdoi:10.21938/dBrplG8I1KR7RyfkMXTyYAThe GAVO DC teamRybizki, J.Demleitner, M.Bailer-Jones, C.Tio, P. D.Cantat-Gaudin, T.Fouesneau, M.Chen, Y.Andrae, R.Girardi, L.Sharma, S.2020-11-25T08:41:00ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837astrostatistics-techniquesmilky-way-galaxyastronomical-simulations 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.2020PASP..132g4501Rhttp://dc.g-vo.org/browse/gedr3mock/qSimulationResearchIsServedByGAVO Data Center TAP servicehttp://dc.g-vo.org/taphttps://dc.g-vo.org/tapOpticalInfraredgedr3mock 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.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.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.rvs_sample_pi_rvs This table lists source_ids of gedr3mock objects that are drawn at random using to the selection function found in Gaia DR2 for stars with a full six-parameter solution as derived in bibcode`TODO`. It is intended to be used to test selection effects in observables on underlying stellar population parameter distributions. The completeness function was applied in spatial bins of HEALPix level 5, and bins of one each in GRVS magnitude and G-GRP color, yielding 7.2e6 sources. This table gives a selection biased so as to match its mean parallax to the the mean parallax of the RVS sample in Gaia DR2 in each bin. The gedr3mock.rvs_sample_pi_random table reflects an unbiased sample, and gedr3mock.rvs_sample_pi_all reflects a sample biased to match the mean parallax of the entire Gaia DR2 in each bin.7300000source_idIdentifier of a star within the unbiased RVS sample.meta.id;meta.main31610959298575.0547592736530234e+174.253777047802872e+186.68145365260706e+1869175284091657912321.0longindexedprimarygedr3mock.generated_datasource_idsource_idgedr3mock.rvs_sample_pi_all This table lists source_ids of gedr3mock objects that are drawn at random using to the selection function found in Gaia DR2 for stars with a full six-parameter solution as derived in bibcode`TODO`. It is intended to be used to test selection effects in observables on underlying stellar population parameter distributions. The completeness function was applied in spatial bins of HEALPix level 5, and bins of one each in GRVS magnitude and G-GRP color, yielding 7.2e6 sources. This table gives a selection biased so as to match its mean parallax to the the mean parallax of Gaia DR2 in each bin. The gedr3mock.rvs_sample_pi_random table reflects an unbiased sample, and gedr3mock.rvs_sample_pi_rvs reflects a sample biased to match the mean parallax of the RVS sample in Gaia DR2 in each bin.7300000source_idIdentifier of a star within the unbiased RVS sample.meta.id;meta.main31610959298575.0547592736530234e+174.253777047802872e+186.68145365260706e+1869175284091657912321.0longindexedprimarygedr3mock.generated_datasource_idsource_idgedr3mock.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.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.4-8um0.6610.6640.6651.3791.3791floatnullablegedr3mock.rvs_sample_unbiased This table lists source_ids of gedr3mock objects that are drawn at random using to the selection function found in Gaia DR2 for stars with a full six-parameter solution as derived in bibcode`TODO`. It is intended to be used to test selection effects in observables on underlying stellar population parameter distributions. The completeness function was applied in spatial bins of HEALPix level 5, and bins of one each in GRVS magnitude and G-GRP color, yielding 7.2e6 sources. This table gives an unbiased selection. The gedr3mock.rvs_sample_pi_rvs table reflects a sample biased to match the mean parallax of the RVS sample in each bin, and the gedr3mock.rvs_sample_pi_all reflects a sample biased to match the mean parallax of the entire Gaia DR2 in each bin.7300000source_idIdentifier of a star within the unbiased RVS sample.meta.id;meta.main31610959298575.0547592736530234e+174.253777047802872e+186.68145365260706e+1869175284091657912321.0longindexedprimarygedr3mock.generated_datasource_idsource_idgedr3mock.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.sensitivity17.820.420.720.720.71floatnullable