gaiafprThe Gaia Focused Product Release presents five data products which showcase a subset of the improvements and new data products expected for Gaia DR4.gaiafpr.crowded_field_sourceSources based on Service Interface Function (SIF) images of very dense regions in the sky.solution_idSolution Identifiermeta.versionlongdesignationUnique source designation (unique across all Data Releases)meta.id;meta.maincharregion_nameName of the designated CrowdedField region in the skymeta.idcharsource_idUnique source identifier (unique within a particular Data Release) providing the CrowdedField-nature of the source via location bitmeta.id;meta.reflongref_epochReference epochyrmeta.ref;time.epochdoubleraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallax.trigdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallax.trigfloatparallax_over_errorParallax divided by its standard errorstat.snr;pos.parallax.trigfloatpmTotal proper motionmas.yr**-1pos.pm;pos.eqfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloatra_dec_corrCorrelation between right ascension and declinationstat.correlationfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatn_scansNumber of CrowdedField scans of the source locationmeta.numbershortastrometric_n_obs_alTotal number of observations in the along-scan (AL) directionmeta.numbershortastrometric_n_obs_acTotal number of observations in the across-scan (AC) directionmeta.numbershortastrometric_n_good_obs_alNumber of good observations in the along-scan (AL) directionmeta.numbershortastrometric_n_bad_obs_alNumber of bad observations in the along-scan (AL) directionmeta.numbershortastrometric_gof_alGoodness of fit statistic of model wrt along-scan observationsstat.fit.goodnessfloatastrometric_chi2_alAL chi-square valuestat.fit.chi2floatastrometric_excess_noiseExcess noise of the sourcemasstat.valuefloatastrometric_excess_noise_sigSignificance of excess noisestat.valuefloatastrometric_params_solvedWhich parameters have been solved for?meta.numbershortpseudocolourAstrometrically estimated pseudocolour of the sourceum**-1em.wavenumberfloatpseudocolour_errorStandard error of the pseudocolour of the sourceum**-1stat.error;em.wavenumberfloatra_pseudocolour_corrCorrelation between right ascension and pseudocolourstat.correlation;em.wavenumber;pos.eq.rafloatdec_pseudocolour_corrCorrelation between declination and pseudocolourstat.correlation;em.wavenumber;pos.eq.decfloatparallax_pseudocolour_corrCorrelation between parallax and pseudocolourstat.correlation;em.wavenumber;pos.parallaxfloatpmra_pseudocolour_corrCorrelation between proper motion in right asension and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.rafloatpmdec_pseudocolour_corrCorrelation between proper motion in declination and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.decfloatastrometric_matched_transitsMatched FOV transits used in the AGIS solutionmeta.numbershortvisibility_periods_usedNumber of visibility periods used in Astrometric solutionmeta.numbershortastrometric_sigma5d_maxThe longest semi-major axis of the 5-d error ellipsoidmasstat;pos.errorEllipsefloatmatched_transitsThe number of transits matched to this sourcemeta.numbershortipd_gof_harmonic_amplitudeAmplitude of the IPD GoF versus position angle of scanstat.valuefloatipd_gof_harmonic_phasePhase of the IPD GoF versus position angle of scandegpos.posAng;stat.valuefloatscan_direction_strength_k1Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k2Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k3Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k4Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_mean_k1Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k2Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k3Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k4Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatastrometric_primary_flagPrimary or secondarymeta.codebooleanphot_g_n_obsNumber of observations contributing to G photometrymeta.numbershortphot_g_mean_fluxG-band mean flux"electron".s**-1phot.flux;em.optdoublephot_g_mean_flux_errorError on G-band mean flux"electron".s**-1stat.error;phot.flux;em.optfloatphot_g_mean_flux_over_errorG-band mean flux divided by its errorstat.snr;phot.flux;em.optfloatphot_g_mean_magG-band mean magnitudemagphot.mag;em.optfloatphot_g_flux_uwvUnit weight variance of fluxesstat.weightdoublephot_g_flux_medianMedian flux"electron".s**-1phot.flux;stat.medianfloatphot_g_flux_skewnessMeasure of the skewness of the flux distributionphot.flux;stat.valuefloatphot_g_flux_kurtosisMeasure of the kurtosis of the flux distributionphot.flux;stat.valuefloatphot_g_flux_madMAD of the flux distribution"electron".s**-1phot.flux;stat.valuefloatphot_g_flux_first_quartileFirst quartile of the flux distribution"electron".s**-1phot.flux;stat.valuefloatphot_g_flux_third_quartileThird quartile of the flux distribution"electron".s**-1phot.flux;stat.valuefloatphot_g_flux_minMinimum flux value"electron".s**-1phot.flux;stat.minfloatphot_g_flux_maxMaximum flux value"electron".s**-1phot.flux;stat.maxfloatphot_proc_modePhotometry processing modemeta.codeshortlGalactic longitudedegpos.galactic.londoublebGalactic latitudedegpos.galactic.latdoubleecl_lonEcliptic longitudedegpos.ecliptic.londoubleecl_latEcliptic latitudedegpos.ecliptic.latdoubleposchargaiafpr.interstellar_medium_paramsThis is the main table of DIB parameters from DIB-Spec, derived from spectra binned in galactic latitude, longitude and distance.solution_idSolution Identifiermeta.versionlonghealpixHEALPix identificationpos.healpixintlcCentral galactic longitude of voxeldegpos.galactic.lonfloatbcCentral galactic latitude of voxeldegpos.galactic.latfloatdcCentral heliocentric distance of voxelkpcpos.distancefloatn_targetsNumber of target stars in a voxelmeta.numberintsnrSNR of the stacked ISM spectrum at 862.0 nmstat.snrfloatew8620DIB equivalent width at 862.0 nmnmspect.line.eqWidthfloatew8620_lowerLower confidence level (16%) of DIB equivalent width at 862.0 nmnmspect.line.eqWidth;stat.valuefloatew8620_upperUpper confidence level (84%) of DIB equivalent width at 862.0 nmnmspect.line.eqWidth;stat.valuefloatflags8620Quality flag of DIB parameters at 862.0 nmmeta.code.qualintp08620p0 parameter at 862.0 nmstat.value;spect.linefloatp08620_lowerLower confidence level (16%) of p0 parameter at 862.0 nmstat.value;spect.linefloatp08620_upperUpper confidence level (84%) of p0 parameter at 862.0 nmstat.value;spect.linefloatp18620p1 parameter at 862.0 nmnmstat.value;spect.linefloatp18620_lowerLower confidence level (16%) of p1 parameter at 862.0 nmnmstat.value;spect.linefloatp18620_upperUpper confidence level (84%) of p1 parameter at 862.0 nmnmstat.value;spect.linefloatp28620p2 parameter at 862.0 nmnmstat.value;spect.linefloatp28620_lowerLower confidence level (16%) of p2 parameter at 862.0 nmnmstat.value;spect.linefloatp28620_upperUpper confidence level (84%) of p2 parameter at 862.0 nmnmstat.value;spect.linefloatew8648DIB equivalent width at 864.8 nmnmspect.line.eqWidthfloatew8648_lowerLower confidence level (16%) of DIB equivalent width at 864.8 nmnmspect.line.eqWidth;stat.valuefloatew8648_upperUpper confidence level (84%) of DIB equivalent width at 864.8 nmnmspect.line.eqWidth;stat.valuefloatflags8648Quality flag of DIB parameters at 864.8 nmmeta.code.qualintp08648p0 parameter at 864.8 nmstat.value;spect.linefloatp08648_lowerLower confidence level (16%) of p0 parameter at 864.8 nmstat.value;spect.linefloatp08648_upperUpper confidence level (84%) of p0 parameter at 864.8 nmstat.value;spect.linefloatp18648p1 parameter at 864.8 nmnmstat.value;spect.linefloatp18648_lowerLower confidence level (16%) of p1 parameter at 864.8 nmnmstat.value;spect.linefloatp18648_upperUpper confidence level (84%) of p1 parameter at 864.8 nmnmstat.value;spect.linefloatp28648p2 parameter at 864.8 nmnmstat.value;spect.linefloatp28648_lowerLower confidence level (16%) of p2 parameter at 864.8 nmnmstat.value;spect.linefloatp28648_upperUpper confidence level (84%) of p2 parameter at 864.8 nmnmstat.value;spect.linefloatdibcont_a0Slope a0 of the global continuum fit of the full stacked spectrumstat.fit.param;spect.continuumfloatdibcont_a0_lowerLower confidence level (16%) of the slope a0 of the global continuum fitstat.fit.param;spect.continuumfloatdibcont_a0_upperUpper confidence level (84%) of the slope a0 of the global continuum fitstat.fit.param;spect.continuumfloatdibcont_a1Intercept a1 of the global continuum fit of the full stacked spectrumstat.fit.param;spect.continuumfloatgaiafpr.interstellar_medium_spectraTable of the stacked Interstellar Medium Spectrasolution_idSolution Identifiermeta.versionlonghealpixThe HEALPix Identificationpos.healpixintlcCentral galactic longitude of voxeldegpos.galactic.lonfloatbcCentral galactic latitude of voxeldegpos.galactic.latfloatdcCentral heliocentric distance of voxelkpcpos.distancefloatlambdaWavelengthangstromem.wlfloatfluxNormalised fluxphot.fluxfloatflux_uncertaintyUncertainty in the flux parameterstat.error;phot.fluxfloatgaiafpr.lens_candidatesThis table contains the sources identified as possible gravitational lens candidates.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnameThe name of the gravitational lens candidatemeta.idcharflagGravLens flagmeta.code.statusshortn_componentsNumber of componentsmeta.numberintcomponent_idIndex of the component for this sourceIdmeta.id.associntn_obs_componentNumber of valid observations used for this componentmeta.numbershortcomponent_flagComponent object flagmeta.code.statusshortra_componentMean right ascension of the componentdegpos.eq.radoublera_std_componentStandard deviation of the right ascension of the componentmasstat.error;pos.eq.rafloatdec_componentMean declination of the clusters of measurementsdegpos.eq.decdoubledec_std_componentStandard deviation of the declination measurementsmasstat.error;pos.eq.decfloatg_flux_componentMean G flux of the component"electron".s**-1phot.flux;em.optdoubleg_flux_component_errorUncertainty of the mean flux value for this component"electron".s**-1stat.error;phot.fluxfloatg_mag_componentMean onboard G magnitude of the componentmagphot.mag;em.optfloatg_mag_std_componentStandard deviation of the onboard G magnitude of the componentmagstat.error;em.optfloatposchargaiafpr.lens_catalogue_nameThis table provides the list of input catalogues that have been used to select any given source that was analysed by the Gravitational Lens module and published in the lens candidate table.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongcatalogue_idThe unique identifier for the catalogue(s) used to select the sources in the gravitational lenses analysismeta.id.assocshortgaiafpr.lens_observationThis table contains the observations associated with the components found in the lens candidates table.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongcomponent_idIndex of the component for this sourceIdmeta.id.associntobservation_idCounter for the observations of each componentmeta.numberintra_obsRight ascension of each individual observation belonging to this component, as decoded from the transitIddegpos.eq.radoubledec_obsDeclination of each individual observation belonging to this component, as decoded from the transitIddegpos.eq.decdoubleg_flux_obsFlux value of each individual observation belonging to this component"electron".s**-1phot.flux;em.optdoubleg_flux_obs_errorFlux error value of each individual observation belonging to this component"electron".s**-1stat.error;phot.fluxfloatg_mag_obsOnboard G magnitudes of each individual observation belonging to this componentmagphot.mag;em.optfloatepoch_obsEpoch of the individual observation belonging to this componentdstat.error;phot.magdoubleposchargaiafpr.lens_outlierThis table contains the individual observations that have been discarded from the analysis of the gravitational lenses.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongoutlier_idCounter for the outliers of each componentmeta.numberintra_obsRight ascension of each individual outlier observationdegpos.eq.radoubledec_obsDeclination of each individual outlier observationdegpos.eq.decdoubleg_flux_obsFlux value of each individual outlier observation"electron".s**-1phot.flux;em.optdoubleg_flux_obs_errorFlux error value of each individual outlier observation"electron".s**-1stat.error;phot.fluxfloatg_mag_obsOnboard G magnitudes of each individual outlier observationmagphot.mag;em.optfloatepoch_obsEpoch of the individual outlier observationdstat.error;phot.magdoublegaiafpr.sso_observationSolar System object observations.solution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongdenominationstandard MPC denomination of the asteroidmeta.id.crosschartransit_idTransit Identifiermeta.idlongobservation_idObservation Identifiermeta.idlongnumber_mpMinor Planet numbermeta.id.crosslongepochGaia-Centric epoch TCB(Gaia)dtime.epochdoubleepoch_errError in Gaia-Centric epochdstat.error;time.epochdoubleepoch_utcGaia-Centric TCB epoch converted to UTCdtime.epochdoubleraRight ascension of the sourcedegpos.eq.radoubledecDeclination of the sourcedegpos.eq.decdoublera_error_systematicStandard error of right ascension, systematicmasstat.error;pos.eq.radoubledec_error_systematicStandard error of declination, systematicmasstat.error;pos.eq.decdoublera_dec_correlation_systematicCorrelation of ra and dec errors, systematicstat.correlation;pos.eqdoublera_error_randomStandard error of right ascension, randommasstat.error;pos.eq.radoubledec_error_randomStandard error of declination, randommasstat.error;pos.eq.decdoublera_dec_correlation_randomCorrelation of ra and dec errors, randomstat.correlation;pos.eqdoublex_gaiaBarycentric x position of GaiaAUpos.cartesian.x;pos.barycenterdoubley_gaiaBarycentric y position of GaiaAUpos.cartesian.y;pos.barycenterdoublez_gaiaBarycentric z position of GaiaAUpos.cartesian.z;pos.barycenterdoublevx_gaiaBarycentric x velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.xdoublevy_gaiaBarycentric y velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.ydoublevz_gaiaBarycentric z velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.zdoublex_gaia_geocentricGeocentric x position of GaiaAUpos.cartesian.x;pos.geocentricdoubley_gaia_geocentricGeocentric y position of GaiaAUpos.cartesian.y;pos.geocentricdoublez_gaia_geocentricGeocentric z position of GaiaAUpos.cartesian.z;pos.geocentricdoublevx_gaia_geocentricGeocentric x velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.xdoublevy_gaia_geocentricGeocentric y velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.ydoublevz_gaia_geocentricGeocentric z velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.zdoubleposition_angle_scanPosition angle of the scanning directiondegpos.posAngdoubleastrometric_outcome_ccdResult of processing the CCDsmeta.code.statusintastrometric_outcome_transitResult of processing the transitmeta.code.statusintfovField of viewphys.angSize;instr.fovshortis_rejectedFlag indicating if rejected by the orbital fitmeta.code.statusbooleanposchargaiafpr.sso_sourceThis table contains data related to Solar System objects observed by Gaia.solution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongnum_of_obsnumber of observationsmeta.numberintnumber_mpMinor Planet numbermeta.id.crosslongdenominationstandard MPC denomination of the asteroidmeta.id.crosscharepoch_state_vectorReference epoch of the state vector, mid-point of the time interval spanned by the observations of the Solar System Object (TCB) with origin at the epoch JD2455197.5 TCBdtime.epochdoubleorbital_elements_var_covar_matrixVar-covar matrix on elliptical elements at reference Epoch.stat.covariancecharh_state_vectorHeliocentric State Vector at reference Epochposcharh_state_vector_var_covar_matrixCovariance matrix of the State Vectorstat.covariancechargaiafpr.vari_epoch_radial_velocityThis table contains the epoch radial velocity data points for a sub-set of variable stars.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongtransit_idTransit unique identifiermeta.idlongrv_obs_timeObserving time of the transitdtime.epochdoubleradial_velocityBarycentric radial velocitykm.s**-1spect.dopplerVeloc.optdoubleradial_velocity_errorBarycentric radial velocity errorkm.s**-1stat.error;spect.dopplerVeloc.optdoublerejected_by_variabilityRejected by DPAC variability processing (or variability analysis)meta.code.statusbooleangaiafpr.vari_long_period_variableThis table describes the Long Period Variable stars.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongfrequencyFrequency from G FoV time seriesd**-1src.var.pulsedoublefrequency_errorUncertainty on the frequency from G FoV time seriesd**-1stat.error;src.var.pulsefloatamplitudeVariability amplitude based on the best-fit model to the G FoV time seriesmagsrc.var.amplitudefloatmedian_delta_wl_rpMedian of the pseudo-wavelength separations between the two highest peaks in RP spectraem.wl;stat.medianfloatis_cstarFlag to mark C-starsmeta.code.classbooleanfrequency_rvFrequency from radial velocity time seriesd**-1src.var.pulsedoublefrequency_rv_errorUncertainty on the frequency from radial velocity time seriesd**-1stat.error;src.var.pulsefloatamplitude_rvVariability amplitude based on the best-fit model to the radial velocity time serieskm.s**-1src.var.amplitudefloatflag_rvFlag identifying a top-quality subsamplemeta.code.qualbooleangaiafpr.vari_rad_vel_statisticsStatistical parameters of radial velocity time series.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_selected_rvTotal number of radial velocity transits selected for variability analysismeta.numbershortmean_obs_time_rvMean observation time for radial velocity transitsdtime.epoch;stat.meandoubletime_duration_rvTime duration of the time series for radial velocity transitsdtime.durationfloatmin_rvMinimum radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.minfloatmax_rvMaximum radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.maxfloatmean_rvMean radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.meanfloatmedian_rvMedian radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.medianfloatrange_rvDifference between the highest and lowest radial velocity transitskm.s**-1spect.dopplerVeloc.opt;arith.difffloatstd_dev_rvSquare root of the unweighted radial velocity variancekm.s**-1stat.stdev;spect.dopplerVeloc.optfloatskewness_rvStandardized unweighted radial velocity skewnessspect.dopplerVeloc.opt;stat.paramfloatkurtosis_rvStandardized unweighted radial velocity kurtosisspect.dopplerVeloc.opt;stat.paramfloatmad_rvMedian Absolute Deviation (MAD) for radial velocity transitskm.s**-1spect.dopplerVeloc.opt;stat.paramfloatabbe_rvAbbe value for radial velocity transitsspect.dopplerVeloc.opt;stat.paramfloatiqr_rvInterquartile range for radial velocity transitskm.s**-1spect.dopplerVeloc.opt;stat.paramfloatgaiafpr_contribContributions using Gaia FPR catalog tablesgaiafpr_contrib.ism_gaiagal_to_eqThis table contains a mapping from Gaia's Galactic to equatorial coordinates.healpixThe HEALPix Identificationpos.healpixintraRight ascensiondegpos.eq.ra;meta.mainfloatdecDeclinationdegpos.eq.dec;meta.mainfloatlcCentral galactic longitude of voxeldegpos.galactic.lonfloatbcCentral galactic latitude of voxeldegpos.galactic.latfloatposThe point position of a source (ra, dec) in radian.[rad,rad](pos.eq.ra,pos.eq.dec)chargaiadr3Gaia Data Release 3gaiadr3.gaia_sourceThis table has an entry for every Gaia observed source as published with this data release. It contains the basic source parameters, in their final state as processed by the Gaia Data Processing and Analysis Consortium from the raw data coming from the spacecraft.solution_idSolution Identifiermeta.versionlongdesignationUnique source designation (unique across all Data Releases)meta.id;meta.maincharsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongrandom_indexRandom index for use when selecting subsetsmeta.codelongref_epochReference epochyrmeta.ref;time.epochdoubleraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallax.trigdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallax.trigfloatparallax_over_errorParallax divided by its standard errorstat.snr;pos.parallax.trigfloatpmTotal proper motionmas.yr**-1pos.pm;pos.eqfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloatra_dec_corrCorrelation between right ascension and declinationstat.correlationfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatastrometric_n_obs_alTotal number of observations in the along-scan (AL) directionmeta.numbershortastrometric_n_obs_acTotal number of observations in the across-scan (AC) directionmeta.numbershortastrometric_n_good_obs_alNumber of good observations in the along-scan (AL) directionmeta.numbershortastrometric_n_bad_obs_alNumber of bad observations in the along-scan (AL) directionmeta.numbershortastrometric_gof_alGoodness of fit statistic of model wrt along-scan observationsstat.fit.goodnessfloatastrometric_chi2_alAL chi-square valuestat.fit.chi2floatastrometric_excess_noiseExcess noise of the sourcemasstat.valuefloatastrometric_excess_noise_sigSignificance of excess noisestat.valuefloatastrometric_params_solvedWhich parameters have been solved for?meta.numbershortastrometric_primary_flagPrimary or secondaymeta.codebooleannu_eff_used_in_astrometryEffective wavenumber of the source used in the astrometric solutionum**-1em.wavenumberfloatpseudocolourAstrometrically estimated pseudocolour of the sourceum**-1em.wavenumberfloatpseudocolour_errorStandard error of the pseudocolour of the sourceum**-1stat.error;em.wavenumberfloatra_pseudocolour_corrCorrelation between right ascension and pseudocolourstat.correlation;em.wavenumber;pos.eq.rafloatdec_pseudocolour_corrCorrelation between declination and pseudocolourstat.correlation;em.wavenumber;pos.eq.decfloatparallax_pseudocolour_corrCorrelation between parallax and pseudocolourstat.correlation;em.wavenumber;pos.parallaxfloatpmra_pseudocolour_corrCorrelation between proper motion in right asension and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.rafloatpmdec_pseudocolour_corrCorrelation between proper motion in declination and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.decfloatastrometric_matched_transitsMatched FOV transits used in the AGIS solutionmeta.numbershortvisibility_periods_usedNumber of visibility periods used in Astrometric solutionmeta.numbershortastrometric_sigma5d_maxThe longest semi-major axis of the 5-d error ellipsoidmasstat;pos.errorEllipsefloatmatched_transitsThe number of transits matched to this sourcemeta.numbershortnew_matched_transitsThe number of transits newly incorporated into an existing source in the current cyclemeta.numbershortmatched_transits_removedThe number of transits removed from an existing source in the current cyclemeta.numbershortipd_gof_harmonic_amplitudeAmplitude of the IPD GoF versus position angle of scanstat.valuefloatipd_gof_harmonic_phasePhase of the IPD GoF versus position angle of scandegpos.posAng;stat.valuefloatipd_frac_multi_peakPercent of successful-IPD windows with more than one peakstat.valueshortipd_frac_odd_winPercent of transits with truncated windows or multiple gatestat.valueshortruweRenormalised unit weight errorstat.errorfloatscan_direction_strength_k1Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k2Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k3Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k4Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_mean_k1Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k2Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k3Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k4Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatduplicated_sourceSource with multiple source identifiersmeta.code.statusbooleanphot_g_n_obsNumber of observations contributing to G photometrymeta.numbershortphot_g_mean_fluxG-band mean flux"electron".s**-1phot.flux;em.optdoublephot_g_mean_flux_errorError on G-band mean flux"electron".s**-1stat.error;phot.flux;em.optfloatphot_g_mean_flux_over_errorG-band mean flux divided by its errorstat.snr;phot.flux;em.optfloatphot_g_mean_magG-band mean magnitudemagphot.mag;em.optfloatphot_bp_n_obsNumber of observations contributing to BP photometrymeta.numbershortphot_bp_mean_fluxIntegrated BP mean flux"electron".s**-1phot.flux;em.opt.Bdoublephot_bp_mean_flux_errorError on the integrated BP mean flux"electron".s**-1stat.error;phot.flux;em.opt.Bfloatphot_bp_mean_flux_over_errorIntegrated BP mean flux divided by its errorstat.snr;phot.flux;em.opt.Bfloatphot_bp_mean_magIntegrated BP mean magnitudemagphot.mag;em.opt.Bfloatphot_rp_n_obsNumber of observations contributing to RP photometrymeta.numbershortphot_rp_mean_fluxIntegrated RP mean flux"electron".s**-1phot.flux;em.opt.Rdoublephot_rp_mean_flux_errorError on the integrated RP mean flux"electron".s**-1stat.error;phot.flux;em.opt.Rfloatphot_rp_mean_flux_over_errorIntegrated RP mean flux divided by its errorstat.snr;phot.flux;em.opt.Rfloatphot_rp_mean_magIntegrated RP mean magnitudemagphot.mag;em.opt.Rfloatphot_bp_rp_excess_factorBP/RP excess factorarith.factor;phot.flux;em.optfloatphot_bp_n_contaminated_transitsNumber of BP contaminated transitsmeta.numbershortphot_bp_n_blended_transitsNumber of BP blended transitsmeta.numbershortphot_rp_n_contaminated_transitsNumber of RP contaminated transitsmeta.numbershortphot_rp_n_blended_transitsNumber of RP blended transitsmeta.numbershortphot_proc_modePhotometry processing modemeta.codeshortbp_rpBP - RP colourmagphot.color;em.opt.B;em.opt.Rfloatbp_gBP - G colourmagphot.color;em.opt.B;em.optfloatg_rpG - RP colourmagphot.color;em.opt;em.opt.Rfloatradial_velocityRadial velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatradial_velocity_errorRadial velocity errorkm.s**-1stat.error;spect.dopplerVeloc.opt;em.opt.Ifloatrv_method_usedMethod used to obtain the radial velocitymeta.code.classshortrv_nb_transitsNumber of transits used to compute the radial velocitymeta.numbershortrv_nb_deblended_transitsNumber of valid transits that have undergone deblendingmeta.numbershortrv_visibility_periods_usedNumber of visibility periods used to estimate the radial velocitymeta.numbershortrv_expected_sig_to_noiseExpected signal to noise ratio in the combination of the spectra used to obtain the radial velocitystat.snrfloatrv_renormalised_gofRadial velocity renormalised goodness of fitstat.fit.goodnessfloatrv_chisq_pvalueP-value for constancy based on a chi-squared criterionstat.fit.paramfloatrv_time_durationTime coverage of the radial velocity time seriesdtime.durationfloatrv_amplitude_robustTotal amplitude in the radial velocity time series after outlier removalkm.s**-1stat.error;spect.dopplerVeloc.opt;em.opt.Ifloatrv_template_teffTeff of the template used to compute the radial velocityKstat.fit.paramfloatrv_template_loggLogg of the template used to compute the radial velocitylog(cm.s**-2)stat.fit.paramfloatrv_template_fe_h[Fe/H] of the template used to compute the radial velocityy"dex"stat.fit.paramfloatrv_atm_param_originOrigin of the atmospheric parameters associated to the templatemeta.code.classshortvbroadSpectral line broadening parameterkm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatvbroad_errorUncertainty on the spectral line broadeningkm.s**-1stat.error;spect.dopplerVeloc.opt;em.opt.Ifloatvbroad_nb_transitsNumber of transits used to compute vbroadmeta.numbershortgrvs_magIntegrated Grvs magnitudemagphot.mag;em.optfloatgrvs_mag_errorGrvs magnitude uncertaintymagstat.error;phot.mag;em.optfloatgrvs_mag_nb_transitsNumber of transits used to compute Grvsmeta.numbershortrvs_spec_sig_to_noiseSignal to noise ratio in the mean RVS spectrumstat.snrfloatphot_variable_flagPhotometric variability flagmeta.code;src.varcharlGalactic longitudedegpos.galactic.londoublebGalactic latitudedegpos.galactic.latdoubleecl_lonEcliptic longitudedegpos.ecliptic.londoubleecl_latEcliptic latitudedegpos.ecliptic.latdoublein_qso_candidatesFlag indicating the availability of additional information in the QsoCandidates tablemeta.code.statusbooleanin_galaxy_candidatesFlag indicating the availability of additional information in the GalaxyCandidates tablemeta.code.statusbooleannon_single_starFlag indicating the availability of additional information in the various Non-Single Star tablesmeta.code.statusshorthas_xp_continuousFlag indicating the availability of mean BP/RP spectrum in continuous representation for this sourcemeta.code.statusbooleanhas_xp_sampledFlag indicating the availability of mean BP/RP spectrum in sampled form for this sourcemeta.code.statusbooleanhas_rvsFlag indicating the availability of mean RVS spectrum for this sourcemeta.code.statusbooleanhas_epoch_photometryFlag indicating the availability of epoch photometry for this sourcemeta.code.statusbooleanhas_epoch_rvFlag indicating the availability of epoch radial velocity for this sourcemeta.code.statusbooleanhas_mcmc_gspphotFlag indicating the availability of GSP-Phot MCMC samples for this sourcemeta.code.statusbooleanhas_mcmc_mscFlag indicating the availability of MSC MCMC samples for this sourcemeta.code.statusbooleanin_andromeda_surveyFlag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)meta.code.statusbooleanclassprob_dsc_combmod_quasarProbability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_galaxyProbability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_starProbability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatteff_gspphotEffective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effective;stat.minfloatteff_gspphot_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effective;stat.maxfloatlogg_gspphotSurface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravity;stat.minfloatlogg_gspphot_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravity;stat.maxfloatmh_gspphotIron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Zfloatmh_gspphot_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Z;stat.minfloatmh_gspphot_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Z;stat.maxfloatdistance_gspphotDistance from GSP-Phot Aeneas best library using BP/RP spectrapcpos.distance;pos.eqfloatdistance_gspphot_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectrapcpos.distance;pos.eqfloatdistance_gspphot_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectrapcpos.distance;pos.eqfloatazero_gspphotMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatazero_gspphot_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatazero_gspphot_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatag_gspphotExtinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatebpminrp_gspphotReddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excessfloatebpminrp_gspphot_lowerLower confidence level (16%) of reddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excess;stat.minfloatebpminrp_gspphot_upperUpper confidence level (84%) of reddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excess;stat.maxfloatlibname_gspphotName of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this tablemeta.notecharposThe point position of a source (ra, dec) in radian.[rad, rad](pos.eq.ra,pos.eq.dec)chargaiadr3.gaia_source_liteThis table has an entry for every Gaia observed source as published with this data release. It contains the basic source parameters, in their final state as processed by the Gaia Data Processing and Analysis Consortium from the raw data coming from the spacecraft.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongrandom_indexRandom index for use when selecting subsetsmeta.codelongraRight ascensiondegpos.eq.ra;meta.maindoubledecDeclinationdegpos.eq.dec;meta.maindoubleparallaxParallaxmaspos.parallax.trigdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallax.trigfloatparallax_over_errorParallax divided by its standard errorstat.snr;pos.parallax.trigfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloatastrometric_params_solvedWhich parameters have been solved for?meta.numbershortpseudocolourAstrometrically estimated pseudocolour of the sourceum**-1em.wavenumberfloatpseudocolour_errorStandard error of the pseudocolour of the sourceum**-1stat.error;em.wavenumberfloatipd_frac_multi_peakPercent of successful-IPD windows with more than one peakstat.valueshortipd_frac_odd_winPercent of transits with truncated windows or multiple gatestat.valueshortruweRenormalised unit weight errorstat.errorfloatphot_g_mean_flux_over_errorG-band mean flux divided by its errorstat.snr;phot.flux;em.optfloatphot_g_mean_magG-band mean magnitudemagphot.mag;em.optfloatphot_bp_mean_flux_over_errorIntegrated BP mean flux divided by its errorstat.snr;phot.flux;em.opt.Bfloatphot_bp_mean_magIntegrated BP mean magnitudemagphot.mag;em.opt.Bfloatphot_rp_mean_flux_over_errorIntegrated RP mean flux divided by its errorstat.snr;phot.flux;em.opt.Rfloatphot_rp_mean_magIntegrated RP mean magnitudemagphot.mag;em.opt.Rfloatphot_bp_rp_excess_factorBP/RP excess factorarith.factor;phot.flux;em.optfloatbp_rpBP - RP colourmagphot.color;em.opt.B;em.opt.Rfloatradial_velocityRadial velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatradial_velocity_errorRadial velocity errorkm.s**-1stat.error;spect.dopplerVeloc.opt;em.opt.Ifloatrv_nb_transitsNumber of transits used to compute the radial velocitymeta.numbershortrv_expected_sig_to_noiseExpected signal to noise ratio in the combination of the spectra used to obtain the radial velocitystat.snrfloatrv_renormalised_gofRadial velocity renormalised goodness of fitstat.fit.goodnessfloatrv_chisq_pvalueP-value for constancy based on a chi-squared criterionstat.fit.paramfloatphot_variable_flagPhotometric variability flagmeta.code;src.varcharlGalactic longitudedegpos.galactic.londoublebGalactic latitudedegpos.galactic.latdoublein_qso_candidatesFlag indicating the availability of additional information in the QsoCandidates tablemeta.code.statusbooleanin_galaxy_candidatesFlag indicating the availability of additional information in the GalaxyCandidates tablemeta.code.statusbooleannon_single_starFlag indicating the availability of additional information in the various Non-Single Star tablesmeta.code.statusshorthas_xp_continuousFlag indicating the availability of mean BP/RP spectrum in continuous representation for this sourcemeta.code.statusbooleanhas_xp_sampledFlag indicating the availability of mean BP/RP spectrum in sampled form for this sourcemeta.code.statusbooleanhas_rvsFlag indicating the availability of mean RVS spectrum for this sourcemeta.code.statusbooleanhas_epoch_photometryFlag indicating the availability of epoch photometry for this sourcemeta.code.statusbooleanhas_epoch_rvFlag indicating the availability of epoch radial velocity for this sourcemeta.code.statusbooleanhas_mcmc_gspphotFlag indicating the availability of GSP-Phot MCMC samples for this sourcemeta.code.statusbooleanhas_mcmc_mscFlag indicating the availability of MSC MCMC samples for this sourcemeta.code.statusbooleanin_andromeda_surveyFlag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)meta.code.statusbooleanteff_gspphotEffective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effectivefloatlogg_gspphotSurface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravityfloatmh_gspphotIron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Zfloatdistance_gspphotDistance from GSP-Phot Aeneas best library using BP/RP spectrapcpos.distance;pos.eqfloatag_gspphotExtinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatebpminrp_gspphotReddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excessfloatposchargaiadr3.dr2_neighbourhoodThis table provides the means to relate the astrophysical source identifier (`source_id`) from DR3 to DR2 via a precomputed crossmatch of such sources, taking into account the proper motions available at DR3.dr2_source_idSource identifier in Gaia DR2meta.id.crosslongdr3_source_idSource identifier in Gaia E/DR3meta.id.cross;meta.mainlongangular_distanceAngular distance between the two sourcesmaspos.angDistancefloatmagnitude_differenceG band magnitude difference between the sourcesmagphot.mag;arith.difffloatproper_motion_propagationFlag indicating whether E/DR3 coordinates were proper motion correctedmeta.code.statusbooleangaiadr3.astrophysical_parametersThis is the main table containing the 1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8 (see Chapter&nbsp;<a href="chap:cu8par">cu8par</a>). Additional parameters can be found in table <code>astrophysical_parameters_supp</code>.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongclassprob_dsc_combmod_quasarProbability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_galaxyProbability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_starProbability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_whitedwarfProbability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_binarystarProbability from DSC-Combmod of being a binary star (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_specmod_quasarProbability from DSC-Specmod of being a quasar (data used: BP/RP spectrum)stat.probabilityfloatclassprob_dsc_specmod_galaxyProbability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum)stat.probabilityfloatclassprob_dsc_specmod_starProbability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum)stat.probabilityfloatclassprob_dsc_specmod_whitedwarfProbability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum)stat.probabilityfloatclassprob_dsc_specmod_binarystarProbability from DSC-Specmod of being a binary star (data used: BP/RP spectrum)stat.probabilityfloatclassprob_dsc_allosmod_quasarProbability from DSC-Allosmod of being a quasar (data used: photometry, astrometry)stat.probabilityfloatclassprob_dsc_allosmod_galaxyProbability from DSC-Allosmod of being a galaxy (data used: photometry, astrometry)stat.probabilityfloatclassprob_dsc_allosmod_starProbability from DSC-Allosmod of being a star (data used: photometry, astrometry)stat.probabilityfloatteff_gspphotEffective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectraKstat.value;phys.temperature.effectivefloatteff_gspphot_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectraKstat.value;phys.temperature.effectivefloatlogg_gspphotSurface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspphot_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatmh_gspphotIron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Fefloatmh_gspphot_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatmh_gspphot_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatdistance_gspphotDistance from GSP-Phot Aeneas best library using BP/RP spectrapcpos.distancefloatdistance_gspphot_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectrapcstat.value;pos.distancefloatdistance_gspphot_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectrapcstat.value;pos.distancefloatazero_gspphotMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.opt.Vfloatazero_gspphot_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatazero_gspphot_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatag_gspphotExtinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.optfloatag_gspphot_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.optfloatabp_gspphotExtinction in G_BP band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.opt.Bfloatabp_gspphot_lowerLower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatabp_gspphot_upperUpper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatarp_gspphotExtinction in G_RP band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.opt.Rfloatarp_gspphot_lowerLower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatarp_gspphot_upperUpper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatebpminrp_gspphotReddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excess;em.optfloatebpminrp_gspphot_lowerLower confidence level (16%) of reddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatebpminrp_gspphot_upperUpper confidence level (84%) of reddening E(G_BP - G_RP) from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatmg_gspphotAbsolute magnitude M_G from GSP-Phot Aeneas best library using BP/RP spectramagphys.magAbs;em.optfloatmg_gspphot_lowerLower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatmg_gspphot_upperUpper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas best library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatradius_gspphotRadius from GSP-Phot Aeneas best library using BP/RP spectrasolRadphys.size.radiusfloatradius_gspphot_lowerLower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatradius_gspphot_upperUpper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatlogposterior_gspphotGoodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best librarystat.fit.goodnessfloatmcmcaccept_gspphotMCMC acceptance rate of GSP-Phot Aeneas MCMC best librarystat.valuefloatlibname_gspphotName of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this tablemeta.recordcharteff_gspspecEffective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationsKphys.temperature.effective;stat.medianfloatteff_gspspec_lower16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationsKstat.value;phys.temperature.effectivefloatteff_gspspec_upper84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationsKstat.value;phys.temperature.effectivefloatlogg_gspspecLogarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationslog(cm.s**-2)phys.gravity;stat.medianfloatlogg_gspspec_lower16th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationslog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspspec_upper84th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisationslog(cm.s**-2)stat.value;phys.gravityfloatmh_gspspecGlobal metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"phys.abund.Fe;stat.medianfloatmh_gspspec_lower16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatmh_gspspec_upper84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatalphafe_gspspecAbundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"phys.abund;stat.medianfloatalphafe_gspspec_lower16th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatalphafe_gspspec_upper84th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatfem_gspspecAbundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>femGspspecNlines</tt>"dex"phys.abund.Fe;stat.medianfloatfem_gspspec_lower16th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatfem_gspspec_upper84th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatfem_gspspec_nlinesNumber of lines used for [Fe/M] abundance estimationmeta.numbercharfem_gspspec_linescatterUncertainty estimation of [Fe/M] abundance using N lines of the element, given in <tt>femGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatsife_gspspecAbundance of Silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>sifeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatsife_gspspec_lower16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatsife_gspspec_upper84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatsife_gspspec_nlinesNumber of lines used for [Si/Fe] abundance estimationmeta.numbercharsife_gspspec_linescatterUncertainty estimation of [Si/Fe] abundance using N lines of the element, given in <tt>sifeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatcafe_gspspecAbundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>cafeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatcafe_gspspec_lower16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcafe_gspspec_upper84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcafe_gspspec_nlinesNumber of lines used for [Ca/Fe] abundance estimationmeta.numbercharcafe_gspspec_linescatterUncertainty estimation of [Ca/Fe] abundance using N lines of the element, given in <tt>cafeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloattife_gspspecAbundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>tifeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloattife_gspspec_lower16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloattife_gspspec_upper84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloattife_gspspec_nlinesNumber of lines used for [Ti/Fe] abundance estimationmeta.numberchartife_gspspec_linescatterUncertainty estimation of [Ti/Fe] abundance using N lines of the element, given in <tt>tifeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatmgfe_gspspecAbundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>mgfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatmgfe_gspspec_lower16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatmgfe_gspspec_upper84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatmgfe_gspspec_nlinesNumber of lines used for [Mg/Fe] abundance estimationmeta.numbercharmgfe_gspspec_linescatterUncertainty estimation of [Mg/Fe] abundance using N lines of the element, given in <tt>mgfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatndfe_gspspecAbundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>ndfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatndfe_gspspec_lower16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatndfe_gspspec_upper84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatndfe_gspspec_nlinesNumber of lines used for [Nd/Fe] abundance estimationmeta.numbercharndfe_gspspec_linescatterUncertainty estimation of [Nd/Fe] abundance using N lines of the element, given in <tt>ndfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatfeiim_gspspecAbundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>feiimGspspecNlines</tt>"dex"phys.abund.Fe;stat.medianfloatfeiim_gspspec_lower16th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatfeiim_gspspec_upper84th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Fefloatfeiim_gspspec_nlinesNumber of lines used for [FeII/M] abundance estimationmeta.numbercharfeiim_gspspec_linescatterUncertainty estimation of [FeII/M] abundance using N lines of the element, given in <tt>feiimGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatsfe_gspspecAbundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>sfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatsfe_gspspec_lower16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatsfe_gspspec_upper84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatsfe_gspspec_nlinesNumber of lines used for [S/Fe] abundance estimationmeta.numbercharsfe_gspspec_linescatterUncertainty estimation of [S/Fe] abundance using N lines of the element, given in <tt>sfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatzrfe_gspspecAbundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>zrfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatzrfe_gspspec_lower16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatzrfe_gspspec_upper84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatzrfe_gspspec_nlinesNumber of lines used for [Zr/Fe] abundance estimationmeta.numbercharzrfe_gspspec_linescatterUncertainty estimation of [Zr/Fe] abundance using N lines of the element, given in <tt>zrfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatnfe_gspspecAbundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>nfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatnfe_gspspec_lower16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatnfe_gspspec_upper84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatnfe_gspspec_nlinesNumber of lines used for [N/Fe] abundance estimationmeta.numbercharnfe_gspspec_linescatterUncertainty estimation of [N/Fe] abundance using N lines of the element, given in <tt>nfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatcrfe_gspspecAbundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>crfeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatcrfe_gspspec_lower16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcrfe_gspspec_upper84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcrfe_gspspec_nlinesNumber of lines used for [Cr/Fe] abundance estimationmeta.recordcharcrfe_gspspec_linescatterUncertainty estimation of [Cr/Fe] abundance using N lines of the element, given in <tt>crfeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatcefe_gspspecAbundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>cefeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatcefe_gspspec_lower16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcefe_gspspec_upper84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatcefe_gspspec_nlinesNumber of lines used for [Ce/Fe] abundance estimationmeta.numbercharcefe_gspspec_linescatterUncertainty estimation of [Ce/Fe] abundance using N lines of the element, given in <tt>cefeGspspecNlines</tt>"dex"stat.error;phys.abund.Zfloatnife_gspspecAbundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations, applied to the individual N lines of the element, given in <tt>nifeGspspecNlines</tt>"dex"phys.abund.Z;stat.medianfloatnife_gspspec_lower16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatnife_gspspec_upper84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abund.Zfloatnife_gspspec_nlinesNumber of lines used for [Ni/Fe] abundance estimationmeta.numbercharnife_gspspec_linescatterUncertainty estimation of [Ni/Fe] abundance using N lines of the element, given in <tt>nifeGspspecNlines</tt>"dex"stat.value;phys.abund.Zfloatcn0ew_gspspecEquivalent witdh of cyanogen absorption line, derived from RVS spectranmspect.line.eqWidthfloatcn0ew_gspspec_uncertaintyUncertainty of equivalent witdh of cyanogen absorption line, derived from RVS spectranmstat.error;spect.line.eqWidthfloatcn0_gspspec_centrallineCentral wavelength of cyanogen line, derived from RVS spectra using DIB algorithmnmspect.line.eqWidthfloatcn0_gspspec_widthWidth of cyoanogen line, derived from RVS spectra using DIB algorithmnmstat.error;spect.line.eqWidthfloatdib_gspspec_lambdaDIB central wavelength from GSP-Spec MatisseGauguin using RVS spectranmem.wl.centralfloatdib_gspspec_lambda_uncertaintyUncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectranmstat.error;em.wl.centralfloatdibew_gspspecEquivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectraangstromspect.line.eqWidthfloatdibew_gspspec_uncertaintyGlobal uncertainty on DIB equivalent width value using DIB algorithmangstromstat.value;spect.line.eqWidthfloatdibewnoise_gspspec_uncertaintyUncertainty on DIB equivalent width value occuring from noise partangstromstat.value;spect.line.eqWidthfloatdibp0_gspspecDepth (p₀ parameter) of the DIB derived from a Gaussian model fitfloatdibp2_gspspecWidth (p₂ parameter) of the DIB derived from a Gaussian model fitangstromstat.fit.paramfloatdibp2_gspspec_uncertaintyUncertainty on the <tt>dibp2Gspspec</tt> parameterangstromstat.fit.paramfloatdibqf_gspspecQuality flag of the DIB computationmeta.code.qualcharflags_gspspecCatalogue flags for GSP-Spec MatisseGauguinmeta.code.statuscharlogchisq_gspspecLogarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parametersstat.fit.chi2floatew_espels_halphaHalpha pseudo-equivalent width from ESP-ELSnmspect.line.eqWidthfloatew_espels_halpha_uncertaintyUncertainty of the Halpha pseudo-equivalent width from ESP-ELSnmstat.error;spect.line.eqWidthfloatew_espels_halpha_flagQuality flag of the Halpha pseudo-equivalent width from ESP-ELSmeta.code.qualcharew_espels_halpha_modelHalpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrumnmspect.line.eqWidthfloatclasslabel_espelsAdopted ELS class label from ESP-ELSmeta.code.classcharclasslabel_espels_flagQuality flag of the adopted ELS class label from ESP-ELSmeta.code.classcharclassprob_espels_wcstarProbability from ESP-ELS of being a Wolf-Rayet star of type WCstat.probabilityfloatclassprob_espels_wnstarProbability from ESP-ELS of being a Wolf-Rayet star of type WNstat.probabilityfloatclassprob_espels_bestarProbability from ESP-ELS of being a Be Starstat.probabilityfloatclassprob_espels_ttauristarProbability from ESP-ELS of being a T Tauri Starstat.probabilityfloatclassprob_espels_herbigstarProbability from ESP-ELS of being a Herbig Ae/Be Starstat.probabilityfloatclassprob_espels_dmestarProbability from ESP-ELS of being an active M dwarf Starstat.probabilityfloatclassprob_espels_pneProbability from ESP-ELS of being a planetary nebulastat.probabilityfloatazero_esphsMonochromatic interstellar extinction, A₀, from ESP-HSmagphys.absorption;em.opt.Vfloatazero_esphs_uncertaintyUncertainty at a 68% confidence level on A₀ from ESP-HSmagstat.error;phys.absorption;em.opt.Vfloatag_esphsIntersterstellar extinction in G band from ESP-HSmagphys.absorption;em.optfloatag_esphs_uncertaintyUncertainty on A_G from ESP-HSmagstat.error;phys.absorption;em.optfloatebpminrp_esphsReddening E(G_BP - G_RP) from ESP-HSmagphot.color.excess;em.optfloatebpminrp_esphs_uncertaintyUncertainty on E(G_BP - G_RP) from ESP-HSmagstat.error;phot.color.excess;em.optfloatteff_esphsEffective temperature from ESP-HSKphys.temperature.effectivefloatteff_esphs_uncertaintyUncertainty at a 68% confidence level on the effective temperature from ESP-HSKstat.error;phys.temperature.effectivefloatlogg_esphsSurface gravity from ESP-HSlog(cm.s**-2)phys.gravityfloatlogg_esphs_uncertaintyUncertainty at a 68% confidence level on the surface gravity from ESP-HSlog(cm.s**-2)stat.error;phys.gravityfloatvsini_esphsProjected rotational velocity from ESP-HSkm.s**-1phys.veloc.rotatfloatvsini_esphs_uncertaintyUncertainty on the projected rotational velocity from ESP-HSkm.s**-1stat.error;phys.veloc.rotatfloatflags_esphsQuality flag of the ESP-HS parametrisationmeta.code.qualcharspectraltype_esphsSpectral type from ESP-ELSsrc.spTypecharactivityindex_espcsChromospheric activity index from ESP-CS, measured on the calcium triplet using RVS spectranmspect.indexfloatactivityindex_espcs_uncertaintyUncertainty in the chromospheric activity index from ESP-CSnmstat.error;spect.indexfloatactivityindex_espcs_inputSource of input stellar parameters for the computation of the activity index by ESP-CScharteff_espucdEffective temperature estimate from ESP-UCD based on the RP spectrumKphys.temperature.effectivefloatteff_espucd_uncertaintyUncertainty of the effective temperature estimate produced by ESP-UCDKstat.error;phys.temperature.effectivefloatflags_espucdQuality flags of the ESP-UCD parameter estimatesmeta.code.statuscharradius_flameRadius of the star from FLAME using <tt>teffGspphot</tt> and <tt>lumFlame</tt>solRadphys.size.radiusfloatradius_flame_lowerLower confidence level (16%) of <tt>radiusFlame</tt>solRadstat.value;phys.size.radiusfloatradius_flame_upperUpper confidence level (84%) of <tt>radiusFlame</tt>solRadstat.value;phys.size.radiusfloatlum_flameLuminosity of the star from FLAME using G band magnitude, extinction (<tt>agGspphot</tt>), parallax or distance, and a bolometric correction <tt>bcFlame</tt>solLumphys.luminosityfloatlum_flame_lowerLower confidence level (16%) of <tt>lumFlame</tt>solLumstat.value;phys.luminosityfloatlum_flame_upperUpper confidence level (84%) of <tt>lumFlame</tt>solLumstat.value;phys.luminosityfloatmass_flameMass of the star from FLAME using stellar models, <tt>lumFlame</tt>, and <tt>teffGspphot</tt>solMassphys.massfloatmass_flame_lowerLower confidence level (16%) of <tt>massFlame</tt>solMassstat.value;phys.massfloatmass_flame_upperUpper confidence level (84%) of <tt>massFlame</tt>solMassstat.value;phys.massfloatage_flameAge of the star from FLAME using stellar models, see <tt>massFlame</tt> for detailsGyrtime.agefloatage_flame_lowerLower confidence level (16%) of <tt>ageFlame</tt>Gyrstat.value;time.agefloatage_flame_upperUpper confidence level (84%) of <tt>ageFlame</tt>Gyrstat.value;time.agefloatflags_flameFlags indicating quality and processing information from FLAMEmeta.code.qualcharevolstage_flameEvolutionary stage of the star from FLAME using stellar models, see <tt>massFlame</tt> for detailssrc.classchargravredshift_flameGravitational redshift from FLAME using <tt>radiusFlame</tt> and <tt>loggGspphot</tt>km.s**-1src.redshiftfloatgravredshift_flame_lowerLower confidence level (16%) of <tt>gravredshiftFlame</tt>km.s**-1stat.value;src.redshiftfloatgravredshift_flame_upperUpper confidence level (84%) of <tt>gravredshiftFlame</tt>km.s**-1stat.value;src.redshiftfloatbc_flameBolometric correction used to derive <tt>lumFlame</tt>magphot.mag.bcfloatmh_mscMetallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax"dex"phys.abundfloatmh_msc_upperUpper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax"dex"stat.value;phys.abundfloatmh_msc_lowerLower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax"dex"stat.value;phys.abundfloatazero_mscMonochromatic extinction A₀ at 547.7nm of the source treated as a binary system from MSC using BP/RP spectra and parallaxmagphys.absorption;em.opt.Vfloatazero_msc_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from MSC using BP/RP spectra and parallaxmagstat.value;phys.absorption;em.opt.Vfloatazero_msc_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from MSC using BP/RP spectra and parallaxmagstat.value;phys.absorption;em.opt.Vfloatdistance_mscDistance from MSC using BP/RP spectra and parallaxpcpos.distancefloatdistance_msc_upperUpper confidence level (84%) of distance from MSC using BP/RP spectra and parallaxpcstat.value;pos.distancefloatdistance_msc_lowerLower confidence level (16%) of distance from MSC using BP/RP spectra and parallaxpcstat.value;pos.distancefloatteff_msc1Effective temperature of the primary from MSC using BP/RP spectra and parallaxKphys.temperature.effectivefloatteff_msc1_upperUpper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallaxKstat.value;phys.temperature.effectivefloatteff_msc1_lowerLower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallaxKstat.value;phys.temperature.effectivefloatteff_msc2Effective temperature of the secondary from MSC using BP/RP spectra and parallaxKphys.temperature.effectivefloatteff_msc2_upperUpper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallaxKstat.value;phys.temperature.effectivefloatteff_msc2_lowerLower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallaxKstat.value;phys.temperature.effectivefloatlogg_msc1Surface gravity of the primary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)phys.gravityfloatlogg_msc1_upperUpper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)stat.value;phys.gravityfloatlogg_msc1_lowerLower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)stat.value;phys.gravityfloatlogg_msc2Surface gravity of the secondary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)phys.gravityfloatlogg_msc2_upperUpper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)stat.value;phys.gravityfloatlogg_msc2_lowerLower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallaxlog(cm.s**-2)stat.value;phys.gravityfloatag_mscExtinction in G band of the source treated as a binary system from MSC using BP/RP spectra and parallaxmagphys.absorption;em.optfloatag_msc_upperUpper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallaxmagstat.value;phys.absorptionfloatag_msc_lowerLower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallaxmagstat.value;phys.absorptionfloatlogposterior_mscGoodness-of-fit score (normalised log-posterior) of MSC MCMCstat.fit.goodnessfloatmcmcaccept_mscMean MCMC acceptance rate of MSC MCMCstat.fit.paramfloatmcmcdrift_mscMean drift of the MSC MCMC chain in units of parameter standard deviationstat.fit.paramfloatflags_mscFlag indicating quality information from MSCmeta.code.qualcharneuron_oa_idIdentifier of the OA SOM map neuron that represents the sourcestat.fit.paramlongneuron_oa_distDistance between the source XP spectra and the OA neuron XP prototype that represents the sourcestat.fit.paramfloatneuron_oa_dist_percentile_rankPercentile rank according to the distance distribution of the OA neuron that represents the sourcestat.fit.paramcharflags_oaFlags indicating quality and processing information from OAmeta.code.qualchargaiadr3.astrophysical_parameters_suppThis table contains additional parameters from the Apsis processing chain from modules that produce more than one result for a parameter.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflonglibname_best_gspphotName of library that achieves the highest mean log-posterior in MCMC samples from GSP-Phot Aeneasmeta.recordcharteff_gspphot_marcsEffective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_marcs_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectraKstat.value;phys.temperature.effectivefloatteff_gspphot_marcs_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectraKstat.value;phys.temperature.effectivefloatlogg_gspphot_marcsSurface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_marcs_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspphot_marcs_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatmh_gspphot_marcsIron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra"dex"phys.abund.Fefloatmh_gspphot_marcs_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatmh_gspphot_marcs_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatdistance_gspphot_marcsDistance from GSP-Phot Aeneas for MARCS library using BP/RP spectrapcpos.distancefloatdistance_gspphot_marcs_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectrapcstat.value;pos.distancefloatdistance_gspphot_marcs_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectrapcstat.value;pos.distancefloatazero_gspphot_marcsMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphys.absorption;em.opt.Vfloatazero_gspphot_marcs_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatazero_gspphot_marcs_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatag_gspphot_marcsExtinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_marcs_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.optfloatag_gspphot_marcs_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.optfloatabp_gspphot_marcsExtinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphys.absorption;em.opt.Bfloatabp_gspphot_marcs_lowerLower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatabp_gspphot_marcs_upperUpper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatarp_gspphot_marcsExtinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphys.absorption;em.opt.Rfloatarp_gspphot_marcs_lowerLower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatarp_gspphot_marcs_upperUpper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatebpminrp_gspphot_marcsReddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphot.color.excess;em.optfloatebpminrp_gspphot_marcs_lowerLower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatebpminrp_gspphot_marcs_upperUpper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatmg_gspphot_marcsAbsolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectramagphys.magAbs;em.optfloatmg_gspphot_marcs_lowerLower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatmg_gspphot_marcs_upperUpper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatradius_gspphot_marcsRadius from GSP-Phot Aeneas for MARCS library using BP/RP spectrasolRadphys.size.radiusfloatradius_gspphot_marcs_lowerLower confidence level (16%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatradius_gspphot_marcs_upperUpper confidence level (84%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatlogposterior_gspphot_marcsGoodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for MARCS librarystat.fit.goodnessfloatmcmcaccept_gspphot_marcsMCMC acceptance rate of GSP-Phot Aeneas MCMC for MARCS librarystat.fit.paramfloatteff_gspphot_phoenixEffective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_phoenix_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectraKstat.value;phys.temperature.effectivefloatteff_gspphot_phoenix_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectraKstat.value;phys.temperature.effectivefloatlogg_gspphot_phoenixSurface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_phoenix_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspphot_phoenix_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatmh_gspphot_phoenixIron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra"dex"phys.abund.Fefloatmh_gspphot_phoenix_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatmh_gspphot_phoenix_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatdistance_gspphot_phoenixDistance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrapcpos.distancefloatdistance_gspphot_phoenix_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrapcstat.value;pos.distancefloatdistance_gspphot_phoenix_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrapcstat.value;pos.distancefloatazero_gspphot_phoenixMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphys.absorption;em.opt.Vfloatazero_gspphot_phoenix_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatazero_gspphot_phoenix_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatag_gspphot_phoenixExtinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_phoenix_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.optfloatag_gspphot_phoenix_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.optfloatabp_gspphot_phoenixExtinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphys.absorption;em.opt.Bfloatabp_gspphot_phoenix_lowerLower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatabp_gspphot_phoenix_upperUpper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatarp_gspphot_phoenixExtinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphys.absorption;em.opt.Rfloatarp_gspphot_phoenix_lowerLower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatarp_gspphot_phoenix_upperUpper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatebpminrp_gspphot_phoenixReddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphot.color.excess;em.optfloatebpminrp_gspphot_phoenix_lowerLower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatebpminrp_gspphot_phoenix_upperUpper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatmg_gspphot_phoenixAbsolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagphys.magAbs;em.optfloatmg_gspphot_phoenix_lowerLower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatmg_gspphot_phoenix_upperUpper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatradius_gspphot_phoenixRadius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrasolRadphys.size.radiusfloatradius_gspphot_phoenix_lowerLower confidence level (16%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatradius_gspphot_phoenix_upperUpper confidence level (84%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatlogposterior_gspphot_phoenixGoodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for PHOENIX librarystat.fit.goodnessfloatmcmcaccept_gspphot_phoenixMCMC acceptance rate of GSP-Phot Aeneas MCMC for PHOENIX librarystat.fit.paramfloatteff_gspphot_obEffective temperature from GSP-Phot Aeneas for OB library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_ob_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectraKstat.value;phys.temperature.effectivefloatteff_gspphot_ob_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectraKstat.value;phys.temperature.effectivefloatlogg_gspphot_obSurface gravity from GSP-Phot Aeneas for OB library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_ob_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspphot_ob_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatmh_gspphot_obIron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra"dex"phys.abund.Fefloatmh_gspphot_ob_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatmh_gspphot_ob_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatdistance_gspphot_obDistance from GSP-Phot Aeneas for OB library using BP/RP spectrapcpos.distancefloatdistance_gspphot_ob_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectrapcstat.value;pos.distancefloatdistance_gspphot_ob_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectrapcstat.value;pos.distancefloatazero_gspphot_obMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectramagphys.absorption;em.opt.Vfloatazero_gspphot_ob_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatazero_gspphot_ob_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatag_gspphot_obExtinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_ob_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.optfloatag_gspphot_ob_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.optfloatabp_gspphot_obExtinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectramagphys.absorption;em.opt.Bfloatabp_gspphot_ob_lowerLower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatabp_gspphot_ob_upperUpper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatarp_gspphot_obExtinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectramagphys.absorption;em.opt.Rfloatarp_gspphot_ob_lowerLower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatarp_gspphot_ob_upperUpper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatebpminrp_gspphot_obReddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectramagphot.color.excess;em.optfloatebpminrp_gspphot_ob_lowerLower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatebpminrp_gspphot_ob_upperUpper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatmg_gspphot_obAbsolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectramagphys.magAbs;em.optfloatmg_gspphot_ob_lowerLower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatmg_gspphot_ob_upperUpper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatradius_gspphot_obRadius from GSP-Phot Aeneas for OB library using BP/RP spectrasolRadphys.size.radiusfloatradius_gspphot_ob_lowerLower confidence level (16%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatradius_gspphot_ob_upperUpper confidence level (84%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatlogposterior_gspphot_obGoodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for OB librarystat.fit.goodnessfloatmcmcaccept_gspphot_obMCMC acceptance rate of GSP-Phot Aeneas MCMC for OB librarystat.fit.paramfloatteff_gspphot_aEffective temperature from GSP-Phot Aeneas for A library using BP/RP spectraKphys.temperature.effectivefloatteff_gspphot_a_lowerLower confidence level (16%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectraKstat.value;phys.temperature.effectivefloatteff_gspphot_a_upperUpper confidence level (84%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectraKstat.value;phys.temperature.effectivefloatlogg_gspphot_aSurface gravity from GSP-Phot Aeneas for A library using BP/RP spectralog(cm.s**-2)phys.gravityfloatlogg_gspphot_a_lowerLower confidence level (16%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspphot_a_upperUpper confidence level (84%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectralog(cm.s**-2)stat.value;phys.gravityfloatmh_gspphot_aIron abundance from GSP-Phot Aeneas for A library using BP/RP spectra"dex"phys.abund.Fefloatmh_gspphot_a_lowerLower confidence level (16%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatmh_gspphot_a_upperUpper confidence level (84%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra"dex"stat.value;phys.abund.Fefloatdistance_gspphot_aDistance from GSP-Phot Aeneas for A library using BP/RP spectrapcpos.distancefloatdistance_gspphot_a_lowerLower confidence level (16%) of distance from GSP-Phot Aeneas for A library using BP/RP spectrapcstat.value;pos.distancefloatdistance_gspphot_a_upperUpper confidence level (84%) of distance from GSP-Phot Aeneas for A library using BP/RP spectrapcstat.value;pos.distancefloatazero_gspphot_aMonochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectramagphys.absorption;em.opt.Vfloatazero_gspphot_a_lowerLower confidence level (16%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatazero_gspphot_a_upperUpper confidence level (84%) of monochromatic extinction A₀ at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Vfloatag_gspphot_aExtinction in G band from GSP-Phot Aeneas for A library using BP/RP spectramagphys.absorption;em.optfloatag_gspphot_a_lowerLower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.optfloatag_gspphot_a_upperUpper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.optfloatabp_gspphot_aExtinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectramagphys.absorption;em.opt.Bfloatabp_gspphot_a_lowerLower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatabp_gspphot_a_upperUpper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Bfloatarp_gspphot_aExtinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectramagphys.absorption;em.opt.Rfloatarp_gspphot_a_lowerLower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatarp_gspphot_a_upperUpper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.absorption;em.opt.Rfloatebpminrp_gspphot_aReddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectramagphot.color.excess;em.optfloatebpminrp_gspphot_a_lowerLower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatebpminrp_gspphot_a_upperUpper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phot.color.excess;em.optfloatmg_gspphot_aAbsolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectramagphys.magAbs;em.optfloatmg_gspphot_a_lowerLower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatmg_gspphot_a_upperUpper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectramagstat.value;phys.magAbs;em.optfloatradius_gspphot_aRadius from GSP-Phot Aeneas for A library using BP/RP spectrasolRadphys.size.radiusfloatradius_gspphot_a_lowerLower confidence level (16%) of radius from GSP-Phot Aeneas for A library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatradius_gspphot_a_upperUpper confidence level (84%) of radius from GSP-Phot Aeneas for A library using BP/RP spectrasolRadstat.value;phys.size.radiusfloatlogposterior_gspphot_aGoodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for A librarystat.fit.goodnessfloatmcmcaccept_gspphot_aMCMC acceptance rate of GSP-Phot Aeneas MCMC for A librarystat.fit.paramfloatteff_gspspec_annEffective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisationsKphys.temperature.effectivefloatteff_gspspec_ann_lowerLower confidence level (16%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisationsKstat.value;phys.temperature.effectivefloatteff_gspspec_ann_upperUpper confidence level (84%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisationsKstat.value;phys.temperature.effectivefloatlogg_gspspec_annSurface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisationslog(cm.s**-2)phys.gravityfloatlogg_gspspec_ann_lowerLower confidence level (16%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisationslog(cm.s**-2)stat.value;phys.gravityfloatlogg_gspspec_ann_upperUpper confidence level (84%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisationslog(cm.s**-2)stat.value;phys.gravityfloatmh_gspspec_annGlobal metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"phys.abundfloatmh_gspspec_ann_lowerLower confidence level (16%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatmh_gspspec_ann_upperUpper confidence level (84%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatalphafe_gspspec_annAbundance of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"phys.abundfloatalphafe_gspspec_ann_lowerLower confidence level (16%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatalphafe_gspspec_ann_upperUpper confidence level (84%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations"dex"stat.value;phys.abundfloatlogchisq_gspspec_annLogarithm of the goodness-of-fit for the GSP-Spec ANN parametersstat.fit.chi2floatflags_gspspec_annCatalogue flags for GSP-Spec ANNmeta.code.statuscharradius_flame_specRadius of the star from FLAME using <tt>teffGspspec</tt> and <tt>lumFlameSpec</tt>solRadphys.size.radiusfloatradius_flame_spec_lowerLower confidence level (16%) of <tt>radiusFlameSpec</tt>solRadstat.value;phys.size.radiusfloatradius_flame_spec_upperUpper confidence level (84%) of <tt>radiusFlameSpec</tt>solRadstat.value;phys.size.radiusfloatlum_flame_specLuminosity of the star from FLAME using G band magnitude, extinction (<tt>agGspphot</tt>), parallax and a bolometric correction <tt>bcFlameSpec</tt>solLumphys.luminosityfloatlum_flame_spec_lowerLower confidence level (16%) of <tt>lumFlameSpec</tt>solLumstat.value;phys.luminosityfloatlum_flame_spec_upperUpper confidence level (84%) of <tt>lumFlameSpec</tt>solLumstat.value;phys.luminosityfloatmass_flame_specMass of the star from FLAME using stellar models, <tt>lumFlameSpec</tt> and <tt>teffGspspec</tt>solMassphys.massfloatmass_flame_spec_lowerLower confidence level (16%) of <tt>massFlameSpec</tt>solMassstat.value;phys.massfloatmass_flame_spec_upperUpper confidence level (84%) of <tt>massFlameSpec</tt>solMassstat.value;phys.massfloatage_flame_specAge of the star from FLAME using stellar models, see <tt>massFlameSpec</tt> for detailsGyrtime.agefloatage_flame_spec_lowerLower confidence level (16%) of <tt>ageFlameSpec</tt>Gyrstat.value;time.agefloatage_flame_spec_upperUpper confidence level (84%) of <tt>ageFlameSpec</tt>Gyrstat.value;time.agefloatflags_flame_specFlag indicating quality of parameters from FLAME using GSP-Spec parametersmeta.code.qualcharevolstage_flame_specEvolutionary stage of the star from FLAME using stellar models, see <tt>massFlameSpec</tt> for detailssrc.classchargravredshift_flame_specGravitational redshift from FLAME using GSP-Spec parameterskm.s**-1src.redshiftfloatgravredshift_flame_spec_lowerLower confidence interval of <tt>gravredshiftFlameSpec</tt>km.s**-1stat.value;src.redshiftfloatgravredshift_flame_spec_upperUpper confidence interval of <tt>gravredshiftFlameSpec</tt>km.s**-1stat.value;src.redshiftfloatbc_flame_specBolometric correction applied to derive <tt>lumFlameSpec</tt> using GSP-Spec parametersmagphot.mag.bcfloatgaiadr3.mcmc_samples_gsp_photThis table hosts Monte-Carlo Markov Chain (MCMC) samples for the posterior probability distribution of all parameters derived from the General Stellar Parametrizer from Photometry (GSP-Phot).solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongnsamplesNumber of samples in the chain from GSP-Photmeta.numbershortteffMCMC samples for T_eff from GSP-PhotKphys.temperature.effectivecharazeroMCMC samples for extinction A₀ from GSP-Photmagphys.absorption;em.optcharloggMCMC samples for log g from GSP-Photlog(cm.s**-2)phys.gravitycharmhMCMC samples for the metallicity from GSP-Phot"dex"phys.abundcharagMCMC samples for extinction in G band from GSP-Photmagphys.absorption;em.optcharmgMCMC samples for M_G from GSP-Photmagphys.magAbs;em.optchardistancepcMCMC samples for distance from GSP-Photpcpos.distancecharabpMCMC samples for extinction in G_BP band from GSP-Photmagphys.absorption;em.opt.BchararpMCMC samples for extinction in G_RP band from GSP-Photmagphys.absorption;em.opt.RcharebpminrpMCMC samples for reddening E(G_BP - G_RP) from GSP-Photmagphot.color.excess;em.optcharlog_posMCMC samples for the log-posterior from GSP-Photstat.probabilitycharlog_likMCMC samples for the log-likelihood from GSP-Photstat.likelihoodcharradiusMCMC samples for stellar radius from GSP-PhotsolRadphys.size.radiuschargaiadr3.mcmc_samples_mscThis table hosts Monte-Carlo Markov Chain (MCMC) samples for the posterior probability distribution of all parameters derived from the Multiple Source Classifier (MSC).source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongnsamplesNumber of samples in the chain from MSCmeta.numbershortteff1MCMC samples for T_{eff, 1} of primary from MSCKphys.temperature.effectivecharteff2MCMC samples for T_{eff, 2} of secondary from MSCKphys.temperature.effectivecharlogg1MCMC samples for log g₁ of primary from MSClog(cm.s**-2)phys.gravitycharlogg2MCMC samples for log g₂ of secondary from MSClog(cm.s**-2)phys.gravitycharazeroMCMC samples for extinction A₀ from MSCmagphys.absorption;em.optcharmhMCMC samples for the metallicity from MSC"dex"phys.abund.FechardistancepcMCMC samples for distance from MSCpcpos.distancecharlog_posMCMC samples for the log-posterior from MSCstat.probabilitycharlog_likMCMC samples for the log-likelihood from MSCstat.likelihoodchargaiadr3.oa_neuron_informationThis is the table hosting the content of a Self-Organized Map calculated from a dataset composed by outliers by the Apsis module OA.solution_idSolution Identifiermeta.versionlongsom_idSelf-Organized Map identifiermeta.idlongneuron_idNeuron identifiermeta.idlongneuron_row_indexRow index of the neuron in the Self-Organised Map latticemeta.idshortneuron_column_indexColumn index of the neuron in the Self-Organised Map latticemeta.idshorthitsNumber of sources populating the neuronmeta.numbercharclass_labelAstronomical class estimated for the neuronmeta.code.classcharcentroid_idIdentifier of the Gaia source that minimizes the classification distance to the neuronmeta.idlongcentroid_distanceSquared Euclidean distance between the centroid XP spectrum and the neuron XP prototypemeta.idfloattemplate_distanceSquared Euclidean distance between the reference XP template and the neuron XP prototypemeta.idfloatg_mag_meanMean G value for the sources that belong to the neuronmagphot.mag;em.optfloatg_mag_std_devStandard deviation of G values for the sources that belong to the neuronmagstat.error;phot.mag;em.optfloatg_mag_minMinimum G value for the sources that belong to the neuronmagphot.mag;stat.minfloatg_mag_maxMaximum G value for the sources that belong to the neuronmagphot.mag;stat.maxfloatbp_mag_meanMean G_BP value for the sources that belong to the neuronmagphot.mag;stat.meanfloatbp_mag_std_devStandard deviation of G_BP values for the sources that belong to the neuronmagstat.error;phot.mag;em.opt.Bfloatbp_mag_minMinimum value of G_BP for the sources that belong to the neuronmagphot.mag;stat.minfloatbp_mag_maxMaximum value of G_BP for the sources that belong to the neuronmagphot.mag;stat.maxfloatrp_mag_meanMean G_RP value for the sources that belong to the neuron neuronmagphot.mag;stat.meanfloatrp_mag_std_devStandard deviation of G_RP values for the sources that belong to the neuronmagstat.error;phot.mag;em.opt.Rfloatrp_mag_minMinimum value of G_RP for the sources that belong to the neuronmagphot.mag;stat.minfloatrp_mag_maxMaximum value of G_RP for the sources that belong to the neuronmagphot.mag;stat.maxfloatpm_ra_meanMean value of the proper motion in right ascension for the sources that belong to the neuronmas.yr**-1pos.pm;stat.meanfloatpm_ra_std_devStandard deviation of the proper motion in right ascension for the sources that belong to the neuronmas.yr**-1stat.error;pos.pmfloatpm_ra_minMinimum value of the proper motion in right ascension for the sources that belong to the neuronmas.yr**-1pos.pm;stat.minfloatpm_ra_maxMaximum value of the proper motion in right ascension for the sources that belong to the neuronmas.yr**-1pos.pm;stat.maxfloatpm_dec_meanMean value of the proper motion in declination for the sources that belong to the neuronmas.yr**-1pos.pm;stat.meanfloatpm_dec_std_devStandard deviation of the proper motion in declination for the sources that belong to the neuronmas.yr**-1stat.error;pos.pmfloatpm_dec_minMinimum value of the proper motion in declination for the sources that belong to the neuronmas.yr**-1pos.pm;stat.minfloatpm_dec_maxMaximum value of the proper motion in declination for the sources that belong to the neuronmas.yr**-1pos.pm;stat.maxfloatparallax_meanMean parallax value for the sources that belong to the neuronmaspos.parallax.trig;stat.meanfloatparallax_std_devStandard deviation of the parallax values for the sources that belong to the neuronmasstat.error;pos.parallax.trigfloatparallax_minMinimum parallax value for the sources that belong to the neuronmaspos.parallax.trig;stat.minfloatparallax_maxMaximum parallax value for the sources that belong to the neuronmaspos.parallax.trig;stat.maxfloatgal_latitude_meanMean galactic latitude for the sources that belong to the neurondegpos.galactic.lat;stat.meanfloatgal_latitude_std_devStandard deviation of the galactic latitude values for the sources that belong to the neurondegstat.error;pos.galactic.latfloatgal_latitude_minMinimum galactic latitude for the sources that belong to the neurondegpos.galactic.lat;stat.minfloatgal_latitude_maxMaximum galactic latitude for the sources that belong to the neurondegpos.galactic.lat;stat.maxfloatintra_neuron_distance_meanMean value of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototypestat.valuefloatintra_neuron_distance_std_devStandard deviation of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototypestat.valuefloatintra_neuron_distance_minMinimum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototypestat.valuefloatintra_neuron_distance_maxMaximum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototypestat.valuefloatinter_neuron_distance_meanMean value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighboursstat.valuefloatinter_neuron_distance_std_devStandard deviation of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighboursstat.valuefloatinter_neuron_distance_minMinimum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighboursstat.valuefloatinter_neuron_distance_maxMaximum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighboursstat.valuefloattemplate_nameName of the template used to describe the neuronmeta.recordchardistance_percentile2525th percentile value for the intra-neuron distance distributionstat.valuefloatdistance_percentile5050th percentile value for the intra-neuron distance distributionstat.valuefloatdistance_percentile6868th percentile value for the intra-neuron distance distributionstat.valuefloatdistance_percentile7575th percentile value for the intra-neuron distance distributionstat.valuefloatdistance_percentile9595th percentile value for the intra-neuron distance distributionstat.valuefloatdistance_fwhmFull Width at Half Maximum value for the intra-neuron distance distributionstat.valuefloatdistance_skewSkewness value for the intra-neuron distance distributionstat.valuefloatdistance_kurtosisKurtosis value for the intra-neuron distance distributionstat.valuefloatdistance_i_q_rInter-Quartile Range value for the intra-neuron distance distributionstat.valuefloatdistance_fwhm_normNormalized FWHM value for the intra-neuron distance distributionstat.valuefloatquality_categoryQuality category assigned to the neuron, where 0 corresponds to the most homogeneous neurons and 6 to the most heterogeneous onesmeta.code.qualshortbp_transits_meanMean value of the number of BP transits for the sources that belong to the neuronmeta.numberfloatbp_transits_std_devStandard deviation of the number of BP transits for the sources that belong to the neuronstat.stdevfloatbp_transits_minMinimum value of the number of BP transits for the sources that belong to the neuronmeta.number;stat.minfloatbp_transits_maxMaximum value of the number of BP transits for the sources that belong to the neuronmeta.number;stat.maxfloatrp_transits_meanMean value of the number of RP transits for the sources that belong to the neuronmeta.number;stat.meanfloatrp_transits_std_devStandard deviation of the number of RP transits for the sources that belong to the neuronstat.stdevfloatrp_transits_minMinimum value of the number of RP transits for the sources that belong to the neuronmeta.number;stat.minfloatrp_transits_maxMaximum value of the number of RP transits for the sources that belong to the neuronmeta.number;stat.maxfloatruwe_meanMean value of the renormalised unit weight error for the sources that belong to the neuronstat.weight;stat.meanfloatruwe_std_devStandard deviation of the renormalised unit weight error for the sources that belong to the neuronstat.stdevfloatruwe_minMinimum value of the renormalised unit weight error for the sources that belong to the neuronstat.weight;stat.minfloatruwe_maxMaximum value of the renormalised unit weight error for the sources that belong to the neuronstat.weight;stat.maxfloatbprp_mean_flux_excess_meanMean value of the BP/RP flux excess for the sources that belong to the neuronstat.valuefloatbprp_mean_flux_excess_std_devStandard deviation of the BP/RP flux excess for the sources that belong to the neuronstat.stdevfloatbprp_mean_flux_excess_minMinimum value of the BP/RP flux excess for the sources that belong to the neuronstat.valuefloatbprp_mean_flux_excess_maxMaximum value of the BP/RP flux excess for the sources that belong to the neuronstat.valuefloatbprp_colour_meanMean value of the G_BP - G_RP colour for the sources that belong to the neuronmagphot.color;stat.meanfloatbprp_colour_std_devStandard deviation of the G_BP - G_RP colour for the sources that belong to the neuronmagstat.stdevfloatbprp_colour_minMinimum value of the G_BP - G_RP colour for the sources that belong to the neuronmagphot.color;stat.minfloatbprp_colour_maxMaximum value of the G_BP - G_RP colour for the sources that belong to the neuronmagphot.color;stat.maxfloatgaiadr3.oa_neuron_xp_spectraThis is the table hosting the prototype BP/RP spectrum corresponding to each of the neurons of the Self-Organised-Map produced by the Apsis module (OA).solution_idSolution Identifiermeta.versionlongneuron_idNeuron identifiermeta.idlongneuron_row_indexRow index of the neuron in the Self-Organised Map latticemeta.idshortneuron_column_indexColumn index of the neuron in the Self-Organised Map latticemeta.idshortxp_spectrum_prototype_fluxNormalised flux at wavelength <tt>xpSpectrumPrototypeWavelength</tt> for the preprocessed XP spectrum that best represents the neuron (prototype)stat.fit.paramfloatxp_spectrum_prototype_wavelengthWavelength associated with the XP spectrum flux valuesnmem.wl.centralfloatxp_spectrum_template_fluxNormalised flux at wavelength <tt>xpSpectrumPrototypeWavelength</tt> for the preprocessed XP spectrum corresponding to the neuron templatestat.fit.paramfloatgaiadr3.total_galactic_extinction_mapThis table provides the Total Galactic Extinction (TGE) map for extinction parameters A₀ describing the effective total Galactic extinction and related uncertainties at four separate HEALPix levels, namely levels 6 to 9.solution_idSolution Identifiermeta.versionlonghealpix_idHEALPix identificationpos.healpixlonghealpix_levelHEALPix level usedpos.healpixshorta0Mean A₀ extinction parametermagphys.absorption.coefffloata0_uncertaintyUncertainty for the mean A₀magstat.error;phys.absorption.coefffloata0_minMinimum A₀ value used for the HEALPix of interestmagphys.absorption.coeff;stat.minfloata0_maxMaximum A₀ value used for the HEALPix of interestmagphys.absorption.coeff;stat.maxfloatnum_tracers_usedNumber of tracers usedmeta.numbercharoptimum_hpx_flagFlag to indicate whether a given HEALPix level is the optimum (True) or not (False)meta.code.classbooleanstatusExit status for TGEmeta.code.statusshortgaiadr3.total_galactic_extinction_map_optThis table provides an optimum version of the Total Galactic Extinction map, derived from the table <code>total_galactic_extinction_map</code> at a single HEALPix level 9.solution_idSolution Identifiermeta.versionlonghealpix_idHEALPix identificationpos.healpixlonga0Median A₀ extinction parametermagphys.absorption.coefffloata0_uncertaintyUncertainty for the mean A₀magstat.error;phys.absorption.coefffloatnum_tracers_usedNumber of tracers usedmeta.numbercharstatusExit status for TGEmeta.code.statusshortoptimum_hpx_levelNumber indicating which HEALPix level was chosen to populate this HEALPixmeta.code.classshortgaiadr3.xp_summaryThis tables contains auxiliary information about the mean BP/RP spectrum of a given source.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongbp_n_relevant_basesNumber of bases that are relevant for the representation of this mean BP spectrummeta.numbershortbp_relative_shrinkingMeasure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrummeta.numberfloatbp_n_measurementsNumber of measurements used for the BP spectrum generationstat.fit.paramshortbp_n_rejected_measurementsNumber of rejected measurements in the BP spectrum generationstat.fit.paramshortbp_standard_deviationStandard deviation for the BP spectrum representation"electron".s**-1.pixel**-1stat.stdevfloatbp_chi_squaredChi squared for the BP spectrum representationstat.fit.chi2floatbp_n_transitsNumber of transits contributing to the mean in BPstat.fit.paramshortbp_n_contaminated_transitsNumber of contaminated transits in BPstat.fit.paramshortbp_n_blended_transitsNumber of blended transits in BPstat.fit.paramshortrp_n_relevant_basesNumber of bases that are relevant for the representation of this mean RP spectrumstat.fit.paramshortrp_relative_shrinkingMeasure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrumstat.fit.paramfloatrp_n_measurementsNumber of measurements used for the RP spectrum generationstat.fit.paramshortrp_n_rejected_measurementsNumber of rejected measurements in the RP spectrum generationstat.fit.paramshortrp_standard_deviationStandard deviation for the RP spectrum representation"electron".s**-1.pixel**-1stat.stdevfloatrp_chi_squaredChi squared for the RP spectrum representationstat.fit.chi2floatrp_n_transitsNumber of transits contributing to the mean in RPstat.fit.paramshortrp_n_contaminated_transitsNumber of contaminated transits in RPstat.fit.paramshortrp_n_blended_transitsNumber of blended transits in RPstat.fit.paramshortgaiadr3.xp_sampled_mean_spectrumThis is the BP/RP externally calibrated sampled mean spectrum.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongraRight Ascensiondegpos.eq.radoubledecDeclinationdegpos.eq.decdoublefluxmean BP + RP combined spectrum fluxW.m**-2.nm**-1spectcharflux_errormean BP + RP combined spectrum flux errorW.m**-2.nm**-1stat.error;spectchargaiadr3.xp_continuous_mean_spectrumTable hosting the mean BP and RP spectra based on the continuous representation in basis functions.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongbp_basis_function_idIdentifier defining the set of basis functions for the BP spectrum representationmeta.idshortbp_degrees_of_freedomDegrees of freedom for the BP spectrum representationstat.fit.dofshortbp_n_parametersNumber of parameters for the BP spectrum representationstat.fit.paramshortbp_n_measurementsNumber of measurements used for the BP spectrum generationmeta.numbershortbp_n_rejected_measurementsNumber of rejected measurements in the BP spectrum generationmeta.numbershortbp_standard_deviationStandard deviation for the BP spectrum representationstat.stdevfloatbp_chi_squaredChi squared for the BP spectrum representationstat.fit.chi2floatbp_coefficientsBasis function coefficients for the BP spectrum representationstat.fit.paramcharbp_coefficient_errorsBasis function coefficient errors for the BP spectrum representationstat.errorcharbp_coefficient_correlationsCorrelation matrix for BP coefficientsstat.correlationcharbp_n_relevant_basesNumber of bases that are relevant for the representation of this mean BP spectrummeta.numbershortbp_relative_shrinkingMeasure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrumstat.fit.paramfloatrp_basis_function_idIdentifier defining the set of basis functions for the BP spectrum representationmeta.numbershortrp_degrees_of_freedomDegrees of freedom for the RP spectrum representationstat.fit.dofshortrp_n_parametersNumber of parameters for the RP spectrum representationstat.fit.paramshortrp_n_measurementsNumber of measurements used for the RP spectrum generationmeta.numbershortrp_n_rejected_measurementsNumber of rejected measurements in the RP spectrum generationmeta.numbershortrp_standard_deviationStandard deviation for the RP spectrum representationstat.stdevfloatrp_chi_squaredChi squared for the RP spectrum representationstat.fit.chi2floatrp_coefficientsBasis function coefficients for the RP spectrum representationstat.fit.paramcharrp_coefficient_errorsBasis function coefficient errors for the RP spectrum representationstat.errorcharrp_coefficient_correlationsCorrelation matrix for RP coefficientsstat.correlationcharrp_n_relevant_basesNumber of bases that are relevant for the representation of this mean RP spectrummeta.numbershortrp_relative_shrinkingMeasure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrummeta.numberfloatgaiadr3.rvs_mean_spectrumThis is the RVS mean sampled spectrum table. The spectra are in the rest frame, they are normalised and their wavelength grid ranges from 846 to 870 nm in steps of 0.01 nm (2401 elements).source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongraRight Ascensiondegpos.eq.ra;meta.maindoubledecDeclinationdegpos.eq.dec;meta.maindoublefluxarray of fluxesphot.flux;em.opt.Icharflux_errorarray of uncertainties in fluxstat.error;phot.flux;em.opt.Icharcombined_transitsnumber of combined transitsmeta.numbershortcombined_ccdsnumber of combined CCD spectrameta.numbershortdeblended_ccdsnumber of deblended CCD spectrameta.numbershortgaiadr3.epoch_photometryEpoch photometry. Each row in this table contains the light curve for a given object in bands G, BP and RP.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongn_transitsNumber of Gaia transitsmeta.numbershorttransit_idTransit unique identifiermeta.idcharg_transit_timeTransit averaged G band observing time (reference epoch (BJD) 2010-01-01T00:00:00)dtime.epochcharg_transit_fluxTransit averaged G band flux"electron".s**-1phot.flux;stat.meancharg_transit_flux_errorTransit averaged G band flux error"electron".s**-1stat.error;phot.flux;em.optcharg_transit_flux_over_errorTransit averaged G band flux divided by its errorstat.snr;phot.flux;em.optcharg_transit_magTransit averaged G band Vega magnitudemagphot.mag;em.optcharg_transit_n_obsNumber of CCD observations contributing to transit averaged G band fluxmeta.numbercharbp_obs_timeBP CCD transit observing time (reference epoch (BJD) 2010-01-01T00:00:00)dtime.epochcharbp_fluxBP band flux"electron".s**-1phot.flux;stat.meancharbp_flux_errorBP band flux error"electron".s**-1stat.error;phot.flux;em.opt.Bcharbp_flux_over_errorBP band flux divided by its errorstat.snr;phot.flux;em.opt.Bcharbp_magBP band Vega magnitudemagphot.mag;em.opt.Bcharrp_obs_timeRP CCD transit observing time (reference epoch (BJD) 2010-01-01T00:00:00)dtime.epochcharrp_fluxRP band flux"electron".s**-1phot.flux;stat.meancharrp_flux_errorRP band flux error"electron".s**-1stat.error;phot.flux;em.opt.Rcharrp_flux_over_errorRP band flux divided by its errorstat.snr;phot.flux;em.opt.Rcharrp_magRP band Vega magnitudemagphot.mag;em.opt.Rcharphotometry_flag_noisy_dataG band flux scatter larger than expected by photometry processing (all CCDs considered)meta.code.statuscharphotometry_flag_sm_unavailableSM transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af1_unavailableAF1 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af2_unavailableAF2 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af3_unavailableAF3 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af4_unavailableAF4 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af5_unavailableAF5 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af6_unavailableAF6 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af7_unavailableAF7 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af8_unavailableAF8 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af9_unavailableAF9 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_bp_unavailableBP transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_rp_unavailableRP transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_sm_rejectSM transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af1_rejectAF1 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af2_rejectAF2 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af3_rejectAF3 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af4_rejectAF4 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af5_rejectAF5 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af6_rejectAF6 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af7_rejectAF7 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af8_rejectAF8 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af9_rejectAF9 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_bp_rejectBP transit rejected by photometry processingmeta.code.statuscharphotometry_flag_rp_rejectRP transit rejected by photometry processingmeta.code.statuscharvariability_flag_g_rejectAverage G transit photometry rejected by variability processingmeta.code.statuscharvariability_flag_bp_rejectBP transit photometry rejected by variability processingmeta.code.statuscharvariability_flag_rp_rejectRP transit photometry rejected by variability processingmeta.code.statuschargaiadr3.binary_massesMasses derived from the non-single stars (NSS) solutions with orbital parameters in table <code>gaiadr3.nss_two_body_orbit</code>.source_idSource Identifiermeta.id;meta.main;meta.reflongm1Primary masssolMassphys.massfloatm1_lowerLower confidence level (16%) of the primary masssolMassphys.mass;stat.valuefloatm1_upperUpper confidence level (84%) of the primary masssolMassphys.mass;stat.valuefloatm2Secondary masssolMassphys.massfloatm2_lowerLower confidence level (16%) of the secondary masssolMassphys.mass;stat.valuefloatm2_upperUpper confidence level (84%) of the secondary masssolMassphys.mass;stat.valuefloatfluxratioFlux ratio of the secondary to the primary in the G-bandphys.luminosity;arith.ratiofloatfluxratio_lowerLower value of the flux ratiostat.value;phys.luminosity;arith.ratiofloatfluxratio_upperUpper value of the flux ratiostat.value;phys.luminosity;arith.ratiofloatcombination_methodCombination of NSS solutions usedmeta.recordcharm1_refReference for the primary massmeta.recordcharflagFlagmeta.recordchargaiadr3.chemical_cartographyOrbital parameters, actions, Galactocentric Cartesian coordinates and velocities for the sample of stars used in the DR3 chemical cartographic study of the Milky Way.solution_idSolution Identifierlongsource_idSource Identifiermeta.id;meta.mainlongjr_medMedian radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Median radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.medianfloatjz_medMedian vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Median vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.medianfloatjphi_medMedian azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc. Equivalent to the median vertical component of the angular momentum.Median azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc. Equivalent to the median vertical component of the angular momentum.phys;stat.medianfloatrplane_medMedian in-plane projection of the Galactocentric distance.kpcpos.distance;stat.medianfloatvrplane_medMedian Galactocentric radial velocity.km.s**-1phys.veloc;stat.medianfloatvz_medMedian vertical velocity.km.s**-1phys.veloc;stat.medianfloatvphi_medMedian Galactocentric azimuthal velocity (positive clockwise).km.s**-1phys.veloc.transverse;stat.medianfloatzmax_medMedian maximum Galactic height (in absolute value) computed assuming the Staeckel approximation.kpcpos.cartesian.z;stat.medianfloatrapo_medMedian of the maximum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.medianfloatrperi_medMedian of the minimum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.medianfloatecc_medMedian orbital eccentricity computed assuming the Staeckel approximation.stat;stat.medianfloatx_medMedian of the Cartesian coordinate X.kpcpos.cartesian.x;stat.medianfloaty_medMedian of the Cartesian coordinate Y.kpcpos.cartesian.y;stat.medianfloatz_medMedian of the Cartesian coordinate Z.kpcpos.cartesian.z;stat.medianfloatenergy_medTotal energy per unit mass assuming median coordinates and velocities.Total energy per unit mass assuming median coordinates and velocities.phys;stat.medianfloatjr_hiUpper confidence limit of the radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Upper confidence limit of the radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.maxfloatjz_hiUpper confidence limit of the vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Upper confidence limit of the vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.maxfloatjphi_hiUpper confidence limit of the azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc.Upper confidence limit of the azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc.phys;stat.maxfloatrplane_hiUpper confidence limit of the in-plane projection of the Galactocentric distance.kpcpos.distance;stat.maxfloatvrplane_hiUpper confidence limit of the Galactocentric radial velocity.km.s**-1phys.veloc;stat.maxfloatvz_hiUpper confidence limit of the vertical velocity.km.s**-1phys.veloc;stat.maxfloatvphi_hiUpper confidence limit of the Galactocentric azimuthal velocity (positive clockwise). Equivalent to the upper confidence limit of the vertical component of the angular momentum.km.s**-1phys.veloc.transverse;stat.maxfloatzmax_hiUpper confidence limit of the maximum Galactic height (in absolute value) computed assuming the Staeckel approximation.kpcpos.cartesian.z;stat.maxfloatrapo_hiUpper confidence limit of the of the maximum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.maxfloatrperi_hiUpper confidence limit of the of the minimum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.maxfloatecc_hiUpper confidence limit of the orbital eccentricity computed assuming the Staeckel approximation.stat;stat.maxfloatx_hiUpper confidence limit of the Cartesian coordinate X.kpcpos.cartesian.x;stat.maxfloaty_hiUpper confidence limit of the Cartesian coordinate Y.kpcpos.cartesian.y;stat.maxfloatz_hiUpper confidence limit of the Cartesian coordinate Z.kpcpos.cartesian.z;stat.maxfloatjr_loLower confidence limit of the radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Lower confidence limit of the radial action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.minfloatjz_loLower confidence limit of the vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.Lower confidence limit of the vertical action per unit mass in units of 1967.3865 km/s kpc computed assuming the Staeckel approximation.stat;stat.minfloatjphi_loLower confidence limit of the azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc. Equivalent to the lower confidence limit of the vertical component of the angular momentum.Lower confidence limit of the azimuthal action per unit mass (positive clockwise) in units of 1967.3865 km/s kpc. Equivalent to the lower confidence limit of the vertical component of the angular momentum.phys;stat.minfloatrplane_loLower confidence limit of the in-plane projection of the Galactocentric distance.kpcpos.distance;stat.minfloatvrplane_loLower confidence limit of the Galactocentric radial velocity.km.s**-1phys.veloc;stat.minfloatvz_loLower confidence limit of the vertical velocity.km.s**-1phys.veloc;stat.minfloatvphi_loLower confidence limit of the Galactocentric azimuthal velocity (positive clockwise).km.s**-1phys.veloc.transverse;stat.minfloatzmax_loLower confidence limit of the maximum Galactic height (in absolute value) computed assuming the Staeckel approximation.kpcpos.cartesian.z;stat;stat.minfloatrapo_loLower confidence limit of the of the maximum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.minfloatrperi_loLower confidence limit of the of the minimum Galactocentric distance computed assuming the Staeckel approximation.kpcpos.distance;stat.minfloatecc_loLower confidence limit of the orbital eccentricity computed assuming the Staeckel approximation.stat;stat.minfloatx_loLower confidence limit of the Cartesian coordinate X.kpcpos.cartesian.x;stat.minfloaty_loLower confidence limit of the Cartesian coordinate Y.kpcpos.cartesian.y;stat.minfloatz_loLower confidence limit of the Cartesian coordinate Z.kpcpos.cartesian.z;stat.minfloatgaiadr3.gold_sample_carbon_starsList of Gaia DR3 source IDs for carbon stars extracted from the main list of candidate carbon stars for having C2 and CN molecular bands significantly stronger than usual M stars <a href="doc:DR3-DPACP-123">DR3-DPACP-123</a>.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflonggaiadr3.gold_sample_fgkm_starsStellar astrophysical parameters of the golden sample of F, G, K, and M stars from <a href="ref:DR3-DPACP-123">DR3-DPACP-123</a>.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongteff_gspphotEffective temperature from GSP-Phot Aeneas best library using BP/RP spectraKphys.temperature.effectivefloatlogg_gspphotSurface gravity from GSP-Phot Aeneas best library using BP/RP spectralog(cm.s**-2)phys.gravityfloatmh_gspphotGlobal metallicity from GSP-Phot Aeneas best library using BP/RP spectra"dex"phys.abund.Zfloatag_gspphotExtinction in G band from GSP-Phot Aeneas best library using BP/RP spectramagphys.absorption;em.optfloatebpminrp_gspphotReddening E(BP-RP) from GSP-Phot Aeneas best library using BP/RP spectramagphot.color.excessfloatalphafe_gspspecMedian abundance of alpha-elements [alphe/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and monte carlo realizations"dex"phys.abund;stat.medianfloatteff_gspspecMedian value of the effective temperature from GSP-Spec MatisseGauguin monte carlo realizations using RVS spectraKphys.temperature.effective;stat.medianfloatlogg_gspspecMedian value of logarithm of the stellar surface gravity using RVS spectra and monte carlo realizationslog(cm.s**-2)phys.gravity;stat.medianfloatmh_gspspecMedian global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and monte carlo realizations"dex"phys.abund.Fe;stat.medianfloatradius_flameRadius of the star derived from FLAME using teffGspphot and lumFlamesolRadphys.size.radiusfloatlum_flameLuminosity of the star from FLAME using G band magnitude, extinction (agGspphot), parallax and a bolometric correction (bcFlame)solLumphys.luminosityfloatmass_flameMass of the star from FLAME using stellar models, lumFlame, and teffGspphotsolMassphys.massfloatage_flameAge of the star from FLAME using stellar models, see massFlame for detailsGyrtime.agefloatevolstage_flameEvolutionary stage of the star derived from FLAME using stellar models, see massFlame for detailssrc.classcharradius_flame_specRadius of the star from FLAME using teffGspspec and lumFlameSpecsolRadphys.size.radiusfloatlum_flame_specLuminosity of the star from FLAME using G band magnitude, extinction (agGspphot), parallax and a bolometric correction (bcFlameSpec)solLumphys.luminosityfloatmass_flame_specMass of the star from FLAME using stellar models, lumFlameSpec, and teffGspspecsolMassphys.massfloatage_flame_specAge of the star from FLAME using stellar models, see massFlameSpec for detailsGyrtime.agefloatevolstage_flame_specEvolutionary stage of the star derived from FLAME using stellar models, see massFlameSpec for detailssrc.classcharspectraltype_esphsSpectral type from ESP-HSsrc.spTypechargaiadr3.gold_sample_oba_starsList of Gaia DR3 source IDs of O, B, and A-type stars having an effective temperature estimate greater than 7,500~K.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongvtan_flagFlag indicating whether the tangential velocity is above 180 km/smeta.code.statuschargaiadr3.gold_sample_solar_analoguesGaia DR3 source IDs of candidates for solar analogues selected from GSP-Spec via effective temperature, surface gravity and metallicity and from FLAME via mass and radius.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflonggaiadr3.gold_sample_spssRecommended parameters for the Gaia Spectro-Photometric Standard stars <a href="https://doi.org/10.1093/mnras/stab766">(Pancino et al. 2021)</a>.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongspss_idSPSS identifiermeta.idcharspss_nameSPSS adopted namemeta.idcharspectraltypeSpectral typesrc.spTypecharbin_flagBinary flagmeta.code.statuscharvar_flagVariability flagmeta.code.statuscharteffBest effective temperatureKphys.temperature.effectivefloatteff_errorUncertainty of the best effective temperatureKstat.error;phys.temperature.effectivefloatloggBest surface gravitylog(cm.s**-2)phys.gravityfloatlogg_errorUncertainty on the best surface gravitylog(cm.s**-2)stat.error;phys.gravityfloatfehBest iron abundance"dex"phys.abund.Fefloatfeh_errorUncertainty on the best iron abundance"dex"stat.error;phys.abund.FefloatalphafeBest alpha enhancement"dex"phys.abundfloatalphafe_errorUncertainty on the best alpha enhancement"dex"stat.error;phys.abundfloatradiusBest radiussolRadphys.size.radiusfloatradius_errorUncertainty on the best radiussolRadstat.error;phys.size.radiusfloatlumBest luminositysolLumphys.luminosityfloatlum_errorUncertainty on the best luminositysolLumstat.error;phys.luminosityfloatmassBest masssolMassphys.massfloatmass_errorUncertainty on the best masssolMassstat.error;phys.massfloatageBest ageGyrtime.agefloatage_errorUncertainty on the best ageGyrstat.error;time.agefloatazeroBest extinction at 547.7 nmmagphys.absorption;em.optfloatazero_errorUncertainty on the best extinction at 547.7 nmmagstat.error;phys.absorption;em.optfloatagExtinction in the G bandmagphys.absorption;em.optfloatag_errorUncertainty on the extinction in the G bandmagstat.error;phys.absorption;em.optfloatebpminrpReddening in BP-RPmagphot.color.excess;em.optfloatebpminrp_errorUncertainty on the reddening in BP-RPmagstat.error;phot.color.excess;em.optfloatdistancepcBest distancepcpos.distancefloatdistancepc_errorUncertainty on the best distancepcstat.error;pos.distancefloatradial_velocityRadial velocitykm.s**-1spect.dopplerVelocfloatradial_velocity_errorUncertainty on the radial velocitykm.s**-1stat.error;spect.dopplerVelocfloatvsiniBest projected rotationkm.s**-1phys.veloc.rotatfloatvsin_errorUncertainty on the best projected rotationkm.s**-1stat.error;phys.veloc.rotatfloatnotesFree text notes on this objectmeta.notechargaiadr3.gold_sample_ucdThe table contains the bolometric luminosities and radii in solar units for a subset of ultracool dwarfs from the Gaia DR3 catalogue.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongftot_fobsCorrection factor applied to obtain the total SED fluxarith.factorfloatlumBolometric luminosity in solar unitssolLumphys.luminosityfloatlum_uncertaintyUncertainty in bolometric luminositysolLumstat.error;phys.luminosityfloatradiusRadius in solar unitsolRadphys.size.radiusfloatradius_uncertaintyUncertainty in radiussolRadstat.error;phys.size.radiusfloatreduced_chi2Reduced chi-square of the SED fitstat.fit.chi2floatgaiadr3.sso_orbitsOrbital parameters and uncertainties computed from the <code>sso_observation</code> astrometric data.number_mpSSO Numbermeta.id;meta.mainchardenominationSolar system object namemeta.idcharosc_epochReference epoch for osculating orbitdtime.epochdoublemean_anomalyMean anomalyradsrc.orbital.meanAnomalydoublearg_perihelionArgument of perihelionradsrc.orbital.periastrondoublelong_asc_nodeLongitude of ascending noderadsrc.orbital.nodedoubleinclinationInclinationradsrc.orbital.inclinationdoubleeccentricityEccentricitysrc.orbital.eccentricitydoublesemi_major_axisSemimajor axisAUpos.distance;src.orbitaldoubleorbital_elements_var_covar_matrixvar-covar matrix on elliptical elements at reference Epochstat.covariancecharstd_dev_semi_major_axisStandard deviation on Semimajor axisAUstat.stdevdoubleh_state_vectorHeliocentric State Vector at reference Epoch?AUAndAUPerDay?poscharh_state_vector_var_covar_matrixCovariance matrix of the State Vectorstat.covariancechararc_lengthOrbital arc length spanned by the observationsdtime.intervaldoublenum_observationsNumber of observationsmeta.numberchargaiadr3.synthetic_photometry_gspcThis is a catalogue of synthetic photometry generated from the Gaia BP/RP mean spectra.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongc_starBP/RP excess factor corrected for the expected colour dependencyphot.color;arith.ratiofloatu_jkc_fluxU flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1phot.flux;em.opt.Ufloatu_jkc_flux_errorError on the U flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Ufloatu_jkc_magU magnitude in the Johnson-Kron-Cousins systemmagphot.mag;em.opt.Ufloatu_jkc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortb_jkc_fluxB flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1phot.flux;em.opt.Bfloatb_jkc_flux_errorError on the B flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Bfloatb_jkc_magB magnitude in the Johnson-Kron-Cousins systemmagphot.mag;em.opt.Bfloatb_jkc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortv_jkc_fluxV flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1phot.flux;em.opt.Vfloatv_jkc_flux_errorError on the V flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Vfloatv_jkc_magV magnitude in the Johnson-Kron-Cousins systemmagphot.mag;em.opt.Vfloatv_jkc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortr_jkc_fluxR flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1phot.flux;em.opt.Rfloatr_jkc_flux_errorError on the R flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Rfloatr_jkc_magR magnitude in the Johnson-Kron-Cousins systemmagphot.mag;em.opt.Rfloatr_jkc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshorti_jkc_fluxI flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1phot.flux;em.opt.Ifloati_jkc_flux_errorError on the I flux in the Johnson-Kron-Cousins systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Ifloati_jkc_magI magnitude in the Johnson-Kron-Cousins systemmagphot.mag;em.opt.Ifloati_jkc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortu_sdss_fluxu flux in the SDSS systemW.m**-2.Hz**-1phot.flux;em.opt.Ufloatu_sdss_flux_errorError on the u flux in the SDSS systemW.m**-2.Hz**-1stat.error;phot.flux;em.opt.Ufloatu_sdss_magu magnitude in the SDSS systemmagphot.mag;em.opt.Ufloatu_sdss_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortg_sdss_fluxg flux in the SDSS systemW.m**-2.Hz**-1phot.flux;em.opt.Bfloatg_sdss_flux_errorError on the g flux in the SDSS systemW.m**-2.Hz**-1stat.error;phot.flux;em.opt.Bfloatg_sdss_magg magnitude in the SDSS systemmagphot.mag;em.opt.Bfloatg_sdss_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortr_sdss_fluxr flux in the SDSS systemW.m**-2.Hz**-1phot.flux;em.opt.Rfloatr_sdss_flux_errorError on the r flux in the SDSS systemW.m**-2.Hz**-1stat.error;phot.flux;em.opt.Rfloatr_sdss_magr magnitude in the SDSS systemmagphot.mag;em.opt.Rfloatr_sdss_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshorti_sdss_fluxi flux in the SDSS systemW.m**-2.Hz**-1phot.flux;em.opt.Ifloati_sdss_flux_errorError on the i flux in the SDSS systemW.m**-2.Hz**-1stat.error;phot.flux;em.opt.Ifloati_sdss_magi magnitude in the SDSS systemmagphot.mag;em.opt.Ifloati_sdss_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortz_sdss_fluxz flux in the SDSS systemW.m**-2.Hz**-1phot.flux;em.opt.Ifloatz_sdss_flux_errorError on the z flux in the SDSS systemW.m**-2.Hz**-1stat.error;phot.flux;em.opt.Ifloatz_sdss_magz magnitude in the SDSS systemmagphot.mag;em.opt.Ifloatz_sdss_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshorty_ps1_fluxy flux in the Pan-STARRS1 systemW.m**-2.Hz**-1phot.flux;em.IR.Jfloaty_ps1_flux_errorError on the y flux in the Pan-STARRS1 systemW.m**-2.Hz**-1stat.error;phot.flux;em.IR.Jfloaty_ps1_magy magnitude in the Pan-STARRS1 systemmagphot.mag;em.IR.Jfloaty_ps1_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortf606w_acswfc_fluxF606W flux in the HST ACS/WFC systemW.m**-2.nm**-1phot.flux;em.opt.Vfloatf606w_acswfc_flux_errorError on the F606W flux in the HST ACS/WFC systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Vfloatf606w_acswfc_magF606W magnitude in the HST ACS/WFC systemmagphot.mag;em.opt.Vfloatf606w_acswfc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortf814w_acswfc_fluxF814W flux in the HST ACS/WFC systemW.m**-2.nm**-1phot.flux;em.opt.Ifloatf814w_acswfc_flux_errorError on the F814W flux in the HST ACS/WFC systemW.m**-2.nm**-1stat.error;phot.flux;em.opt.Ifloatf814w_acswfc_magF814W magnitude in the HST ACS/WFC systemmagphot.mag;em.opt.Ifloatf814w_acswfc_flagFlag indicating if G mag and BP-RP color of the source lie in the validated rangemeta.code.qualshortgaiadr3.qso_candidatesThis table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as QSO candidates.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongastrometric_selection_flagFlag indicating if the source is part of the astrometric selectionmeta.code.statusbooleangaia_crf_sourceFlag indicative of whether the source was used define the Gaia-CRF3meta.code.statusbooleanvari_best_class_nameName of best class, see table VariClassifierClassDefinition for details of the classmeta.code.classcharvari_best_class_scoreScore of the best classstat.probabilityfloatfractional_variability_gFractional variability in the G bandsrc.var.amplitude;em.optfloatstructure_function_indexIndex of the first-order structure function in the G bandsrc.var.indexfloatstructure_function_index_scatterStandard deviation of the index of the structure functionstat.stdevdoubleqso_variabilityQuasar variability metric in the G bandsrc.varfloatnon_qso_variabilityNon-quasar variability metric in the G bandsrc.varfloatvari_agn_membership_scoreMembership score (0=lowest,1=highest) of source to be of AGN typestat.probabilitydoubleclassprob_dsc_combmod_quasarProbability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_galaxyProbability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclasslabel_dscClass assigned by DSC based on the probability from its Combmod classifiermeta.code.classcharclasslabel_dsc_jointClass assigned by DSC based on the probability from its Specmod and Allosmod classifiersmeta.code.classcharclasslabel_oaClass assigned by OA the neuron that represents the sourcemeta.code.classcharredshift_qsocRedshift from QSOCsrc.redshiftfloatredshift_qsoc_lowerRedshift lower confidence level from QSOCstat.value;src.redshiftfloatredshift_qsoc_upperRedshift upper confidence level from QSOCstat.value;src.redshiftfloatccfratio_qsocValue of the cross-correlation function used to derive the redshift from QSOC, relative to the maximum valuestat.valuefloatzscore_qsocRedshift zscore from QSOCstat.value;src.redshiftfloatflags_qsocProcessing flags for the analysis based on BP/RP Spectra from QSOCmeta.code.statuslongn_transitsNumber of transits used for the morphological analysismeta.numbercharintensity_quasarFitted intensity of the quasar at its center"electron".s**-1phot.flux;em.optdoubleintensity_quasar_errorError on the fitted intensity of the quasar at its center"electron".s**-1stat.error;phot.flux;em.optdoubleintensity_hostgalaxyFitted intensity of the host galaxy at the effective radius"electron".s**-1phot.flux;em.optdoubleintensity_hostgalaxy_errorError on the fitted intensity of the host galaxy at effective radius"electron".s**-1stat.error;phot.flux;em.optdoubleradius_hostgalaxyFitted effective radius of the host galaxymassrc.morph.paramdoubleradius_hostgalaxy_errorError on the fitted effective radius of the host galaxymasstat.errordoublesersic_indexFitted sersic Indexsrc.morph.paramfloatsersic_index_errorError on the fitted sersic Indexstat.errorfloatellipticity_hostgalaxyFitted ellipticity of the host galaxysrc.ellipticitydoubleellipticity_hostgalaxy_errorError on the fitted ellipticity of the host galaxystat.error;src.ellipticitydoubleposangle_hostgalaxyFitted position angle of the host galaxydegpos.posAngdoubleposangle_hostgalaxy_errorError on the fitted position angle of the host galaxydegstat.error;pos.posAngdoublehost_galaxy_detectedFlag indicating whether a host galaxy has been detectedstat.fit.parambooleanl2_normL2 norm for the fitted Sersic profilestat.fit.paramdoublemorph_params_corr_vecVector form of the upper triangle of the correlation matrix for the fitted morphological parametersstat.correlationcharhost_galaxy_flagFlag indicative of processing or scientific quality for the morphological parameters fittingmeta.code.qualshortsource_selection_flagsBit indicative of whether the input data from a given module met the source list eligibility criteria for the source of interestmeta.code.statuschargaiadr3.qso_catalogue_nameThis table provides the list of input catalogues that have been used to select any given source for which morphological analysis parameters are provided in table <code>qso_candidates</code>.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongcatalogue_idThe unique identifier for the catalogue(s) used to select the sources in the morphological analysismeta.id.assocshortgaiadr3.galaxy_candidatesThis table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as galaxy candidates.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongvari_best_class_nameName of best class, see table VariClassifierClassDefinition for details of the classmeta.code.classcharvari_best_class_scoreScore of the best classstat.probabilityfloatclassprob_dsc_combmod_galaxyProbability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclassprob_dsc_combmod_quasarProbability from DSC-Combmod of being a quasar (data used: BP/RP spectrum, photometry, astrometry)stat.probabilityfloatclasslabel_dscClass assigned by DSC based on the probability from its Combmod classifiermeta.code.classcharclasslabel_dsc_jointClass assigned by DSC based on the probability from its Specmod and Allosmod classifiersmeta.code.classcharclasslabel_oaClass assigned by OA the neuron that represents the sourcemeta.code.classcharredshift_ugcRedshift from UGCsrc.redshiftfloatredshift_ugc_lowerRedshift prediction lower limit from UGCstat.value;src.redshiftfloatredshift_ugc_upperRedshift prediction upper limit from UGCstat.value;src.redshiftfloatn_transitsNumber of transits used for the morphological analysismeta.numbercharposangle_sersicFitted position angle of the source for the Sersic Profiledegpos.posAngdoubleposangle_sersic_errorError on the fitted position angle of the source for the Sersic Profiledegstat.error;pos.posAngdoubleintensity_sersicFitted intensity of the source for the Sersic Profile"electron".s**-1phot.flux;em.optdoubleintensity_sersic_errorError on the fitted intensity of the source at effective radius radiusSersic"electron".s**-1stat.error;phot.flux;em.optdoubleradius_sersicFitted effective radius of the source for the Sersic Profilemasphys.angSizedoubleradius_sersic_errorError on the fitted effective radius of the source for the Sersic Profilemasstat.error;phys.angSizedoubleellipticity_sersicFitted ellipticity of source for the Sersic Profilesrc.ellipticitydoubleellipticity_sersic_errorError on the fitted ellipticity of the source for the Sersic Profilestat.error;src.ellipticitydoublen_sersicFitted Sersic Index for Sersic Profilestat.fit.paramfloatn_sersic_errorError on the fitted Sersic Index for Sersic Profilestat.errorfloatl2_sersicL2 norm for the Sersic Profilestat.fit.paramdoublemorph_params_corr_vec_sersicVector form of the upper triangle of the correlation matrix for the fitted parameters for the Sersic Profilestat.correlationcharflags_sersicFlag indicative of processing or scientific quality for the morphological parameters fitting for the Sersic Profilemeta.code.qualshortposangle_de_vaucouleursFitted position angle of the source for the de Vaucouleurs Profiledegpos.posAngdoubleposangle_de_vaucouleurs_errorError on the fitted position angle of the source for the de Vaucouleurs Profiledegstat.error;pos.posAngdoubleintensity_de_vaucouleursFitted intensity of the source for the de Vaucouleurs Profile"electron".s**-1phot.flux;em.optdoubleintensity_de_vaucouleurs_errorError on the fitted intensity of the bulge for the de Vaucouleurs Profile"electron".s**-1stat.error;phot.flux;em.optdoubleradius_de_vaucouleursFitted effective radius of the source for de Vaucouleurs Profilemasphys.angSizedoubleradius_de_vaucouleurs_errorError on the fitted effective radius of the source for the de Vaucouleurs Profilemasstat.error;phys.angSizedoubleellipticity_de_vaucouleursFitted ellipticity of source for the de Vaucouleurs Profilesrc.ellipticitydoubleellipticity_de_vaucouleurs_errorError on the fitted ellipticity of the source for the de Vaucouleurs Profilestat.error;src.ellipticitydoublel2_de_vaucouleursL2 norm for the de Vaucouleurs Profilestat.fit.paramdoublemorph_params_corr_vec_de_vaucouleursVector form of the upper triangle of the correlation matrix for the fitted parameters for the de Vaucouleurs Profilestat.correlationcharflags_de_vaucouleursFlag indicative of processing or scientific quality for the morphological parameters fitting for the de Vaucouleurs Profilemeta.code.qualshortsource_selection_flagsBit indicative of whether the input data from a given module met the source list eligibility criteria for the source of interestmeta.code.statuschargaiadr3.galaxy_catalogue_nameThis table provides the list of input catalogues that have been used to select any given source for which morphological analysis parameters are provided in table <code>galaxy_candidates</code>.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongcatalogue_idThe unique identifier for the catalogue(s) used to select the sources in the morphological analysismeta.id.assocshortgaiadr3.sso_observationSolar System object observations. Each table line contains data obtained during the transit of the source on a single CCD, during a single transit.solution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongdenominationstandard MPC denomination of the asteroidmeta.id.crosschartransit_idTransit Identifiermeta.idlongobservation_idObservation Identifiermeta.idlongnumber_mpMinor Planet numbermeta.id.crosslongepochGaia-centric epoch TCB(Gaia)dtime.epochdoubleepoch_errError in Gaiacentric epochdstat.error;time.epochdoubleepoch_utcGaia-centric TCB epoch converted to UTCdtime.epochdoubleraRight ascension of the sourcedegpos.eq.radoubledecDeclination of the sourcedegpos.eq.decdoublera_error_systematicStandard error of right ascension - systematicmasstat.error;pos.eq.radoubledec_error_systematicStandard error of declination - systematicmasstat.error;pos.eq.decdoublera_dec_correlation_systematicCorrelation of ra and dec errors - systematicstat.correlation;pos.eqdoublera_error_randomStandard error of right ascension - randommasstat.error;pos.eq.radoubledec_error_randomStandard error of declination - randommasstat.error;pos.eq.decdoublera_dec_correlation_randomCorrelation of ra and dec errors - randomstat.correlation;pos.eqdoubleg_magCalibrated G magmagphot.mag;em.optdoubleg_fluxAverage calibrated G flux for the transit"electron".s**-1phot.mag;stat.meandoubleg_flux_errorError on the G flux"electron".s**-1stat.error;phot.fluxdoublex_gaiaBarycentric x position of GaiaAUpos.cartesian.x;pos.barycenterdoubley_gaiaBarycentric y position of GaiaAUpos.cartesian.y;pos.barycenterdoublez_gaiaBarycentric z position of GaiaAUpos.cartesian.z;pos.barycenterdoublevx_gaiaBarycentric x velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.xdoublevy_gaiaBarycentric y velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.ydoublevz_gaiaBarycentric z velocity of GaiaAU.d**-1phys.veloc;pos.barycenter;pos.cartesian.zdoublex_gaia_geocentricGeocentric x position of GaiaAUpos.cartesian.x;pos.geocentricdoubley_gaia_geocentricGeocentric y position of GaiaAUpos.cartesian.y;pos.geocentricdoublez_gaia_geocentricGeocentric z position of GaiaAUpos.cartesian.z;pos.geocentricdoublevx_gaia_geocentricGeocentric x velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.xdoublevy_gaia_geocentricGeocentric y velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.ydoublevz_gaia_geocentricGeocentric z velocity of GaiaAU.d**-1phys.veloc;pos.geocentric;pos.cartesian.zdoubleposition_angle_scanPosition angle of the scanning directiondegpos.posAngdoubleastrometric_outcome_ccdResult of processing the CCDsmeta.code.statuscharastrometric_outcome_transitResult of processing the transitmeta.code.statuscharposchargaiadr3.sso_reflectance_spectrumThis table contains the mean BP/RP reflectance spectra of asteroids computed as the ratio between the asteroid flux and an averaged solar analogue flux.source_idSource identifiermeta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongnumber_mpMinor Planet numbermeta.id.crosslongdenominationstandard MPC denomination of the asteroidmeta.id.crosscharnb_samplesNb samples in spectrummeta.numbershortnum_of_spectranumber of epoch spectra used to compute the averagestat.valuecharreflectance_spectrumReflectance spectrumspectfloatreflectance_spectrum_errError in reflectance spectrumstat.errorfloatwavelengthInternally-calibrated wavelength of reflectance spectrumnmem.wlfloatreflectance_spectrum_flagReflectance spectrum value flagmeta.code.qualshortgaiadr3.sso_sourceThis table contains data related to Solar System objects observed by Gaia.solution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongnum_of_obsnumber of observationsmeta.numbercharnumber_mpMinor Planet numbermeta.id.crosslongdenominationstandard MPC denomination of the asteroidmeta.id.crosscharnum_of_spectraNumber of epoch spectra used to compute the averagestat.fit.paramchargaiadr3.nss_acceleration_astroThis table contains non-single-star (NSS) astrometric models for sources having a non-linear proper motion which is compatible with an acceleration solution.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongnss_solution_typeNSS model adoptedmeta.recordcharraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallaxdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloataccel_raAcceleration in RAmas.yr**-2phys.accelerationdoubleaccel_ra_errorStandard error of Acceleration in RAmas.yr**-2stat.error;phys.accelerationfloataccel_decAcceleration in DECmas.yr**-2phys.accelerationdoubleaccel_dec_errorStandard error of Acceleration in DECmas.yr**-2stat.error;phys.accelerationfloatderiv_accel_raTime derivative of the accel. in RAmas.yr**-3phys.accelerationdoublederiv_accel_ra_errorStandard error of Time derivative of the acceleration in RAmas.yr**-3stat.error;phys.accelerationfloatderiv_accel_decTime derivative of the accel. in DECmas.yr**-3phys.accelerationdoublederiv_accel_dec_errorStandard error of Time derivative of the acceleration in DECmas.yr**-3stat.error;phys.accelerationfloatastrometric_n_obs_alTotal astrometric CCD observations in AL consideredmeta.numbercharastrometric_n_good_obs_alTotal astrometric CCD observations in AL actually usedmeta.numbercharbit_indexBoolean mask for the fields above in the corrVec matrixmeta.code.statuslongcorr_vecVector form of the upper triangle of the correlation matrixstat.correlationcharobj_funcValue of the objective function at the solutionstat.fit.paramfloatgoodness_of_fitGoodness of fit in the Hipparcos sensestat.fit.goodnessfloatsignificanceThe significance of the solution (i.e. how worth keeping a model is)stat.fit.paramfloatflagsQuality flag for the achieved NSS solutionmeta.code.quallonggaiadr3.nss_non_linear_spectroThis table contains non-single-star (NSS) orbital models for spectroscopic binaries compatible with a trend.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongnss_solution_typeNSS model adoptedmeta.recordcharmean_velocityMean velocitykm.s**-1phys.velocdoublemean_velocity_errorStandard error of Mean velocitykm.s**-1stat.error;phys.velocfloatfirst_deriv_velocityFirst order derivative of the velocityKm.s**-1.d**-1phys.accelerationdoublefirst_deriv_velocity_errorStandard error of First order derivative of the velocityKm.s**-1.d**-1stat.error;phys.accelerationfloatsecond_deriv_velocitySecond order derivative of the velocityKm.s**-1.d**-2phys.accelerationdoublesecond_deriv_velocity_errorStandard error of Second order derivative of the velocityKm.s**-1.d**-2stat.error;phys.accelerationfloatrv_n_obs_primaryTotal number of radial velocities considered for the primarymeta.numbercharrv_n_good_obs_primaryTotal number of radial velocities actually used for the primarymeta.numbercharbit_indexBoolean mask for the fields above in the corrVec matrixmeta.code.statuslongcorr_vecVector form of the upper triangle of the correlation matrixstat.correlationcharobj_funcValue of the objective function at the solutionstat.fit.paramfloatgoodness_of_fitGoodness of fit in the Hipparcos sensestat.fit.goodnessfloatflagsQuality flag for the achieved NSS solutionmeta.code.statuslonggaiadr3.nss_two_body_orbitThis table contains non-single-star (NSS) orbital models for sources compatible with an orbital two-body solution.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongnss_solution_typeNSS model adoptedmeta.recordcharraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallaxdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloata_thiele_innesThiele-Innes element Amasphys.angSizedoublea_thiele_innes_errorStandard error of Thiele-Innes element Amasstat.error;phys.angSizefloatb_thiele_innesThiele-Innes element Bmasphys.angSizedoubleb_thiele_innes_errorStandard error of Thiele-Innes element Bmasstat.error;phys.angSizefloatf_thiele_innesThiele-Innes element Fmasphys.angSizedoublef_thiele_innes_errorStandard error of Thiele-Innes element Fmasstat.error;phys.angSizefloatg_thiele_innesThiele-Innes element Gmasphys.angSizedoubleg_thiele_innes_errorStandard error of Thiele-Innes element Gmasstat.error;phys.angSizefloatc_thiele_innesC element of Thiele-InnesAUphys.angSize;phys.angSize.smajAxisdoublec_thiele_innes_errorStandard error of C element of Thiele-InnesAUstat.error;phys.angSize;phys.angSize.smajAxisfloath_thiele_innesH element of Thiele-InnesAUphys.angSize;phys.angSize.smajAxisdoubleh_thiele_innes_errorStandard error of H element of Thiele-InnesAUstat.error;phys.angSize;phys.angSize.smajAxisfloatperiodOrbital Perioddtime.perioddoubleperiod_errorStandard error of Orbital Perioddstat.error;time.periodfloatt_periastronPeriastron epochdtime.epochdoublet_periastron_errorStandard error of Periastron epochdstat.error;time.epochfloateccentricityeccentricitysrc.orbital.eccentricitydoubleeccentricity_errorStandard error of eccentricitystat.error;src.orbital.eccentricityfloatcenter_of_mass_velocityThe velocity of the center of masskm.s**-1phys.velocdoublecenter_of_mass_velocity_errorStandard error of The velocity of the center of masskm.s**-1stat.error;phys.velocfloatsemi_amplitude_primarySemi-amplitude of the center of masskm.s**-1phys.velocdoublesemi_amplitude_primary_errorStandard error of Semi-amplitude of the center of masskm.s**-1stat.error;phys.velocfloatsemi_amplitude_secondaryThe semiamplitude of the radial velocity curve for second componentkm.s**-1phys.velocdoublesemi_amplitude_secondary_errorStandard error of The semiamplitude of the radial velocity curve for second componentkm.s**-1stat.error;phys.velocfloatmass_ratioMass ratiophys.mass;arith.ratiodoublemass_ratio_errorStandard error of Mass ratiostat.errorfloatfill_factor_primaryFill factor of primarysrc.morph.paramdoublefill_factor_primary_errorStandard error of Fill factor of primarystat.errorfloatfill_factor_secondaryFill factor of secondarysrc.morph.paramdoublefill_factor_secondary_errorStandard error of Fill factor of secondarystat.errorfloatinclinationOrbital inclinationdegsrc.orbital.inclinationdoubleinclination_errorStandard error of Orbital inclinationdegstat.error;src.orbital.inclinationfloatarg_periastronArgument of periastrondegsrc.orbital.periastrondoublearg_periastron_errorStandard error of Argument of periastrondegstat.error;src.orbital.periastronfloattemperature_ratioRatio of the effective temperaturesphys.temperature;arith.ratiodoubletemperature_ratio_errorStandard error of the ratio of the effective temperaturesstat.error;phys.temperaturedoubletemperature_ratio_definitionCode defining which fitting scenario did apply to the effective temperaturemeta.numbershortastrometric_n_obs_alTotal astrometric CCD observations in AL consideredmeta.numbercharastrometric_n_good_obs_alTotal astrometric CCD observations in AL actually usedmeta.numbercharrv_n_obs_primaryTotal number of radial velocities considered for the primarymeta.numbercharrv_n_good_obs_primaryTotal number of radial velocities actually used for the primarymeta.numbercharrv_n_obs_secondaryTotal number of radial velocities considered for the secondary in the case of SB2meta.numbercharrv_n_good_obs_secondaryTotal number of radial velocities actually used for the secondary in the case of SB2meta.numbercharphot_g_n_obsTotal number of G photometry measurements consideredmeta.numbercharphot_g_n_good_obsTotal number of G photometry measurements actually usedmeta.numbercharbit_indexboolean mask for the fields above in the corrVec matrixmeta.code.statuslongcorr_vecVector form of the upper triangle of the correlation matrix (column-major ordered)stat.correlationcharobj_funcvalue of the objective function at the solutionstat.fit.paramfloatgoodness_of_fitgoodness of fit in the Hipparcos sensestat.fit.goodnessfloatefficiencyEfficiency of the solutionstat.fit.paramfloatsignificanceThe significance of the solution (i.e. how worth keeping a model is)stat.fit.paramfloatflagsQuality flag for the achieved NSS solutionmeta.code.quallongconf_spectro_periodThe probability of the period for not being due to (gaussian white) noise. Relevant for SB1, SB1C, SB2 and SB2C models. To be ignored otherwise.stat.probabilityfloatr_pole_sumSum of the polar radii of primary and secondary (in units of the semi-major axis)phys.size.radiusdoubler_l1_point_sumL1-pointing radii of primary and secondary (in units of the semi-major axis)phys.size.radiusdoubler_spher_sumSum of the radii of sphere having the same volume as the primary and secondary (in units of the semi-major axisphys.size.radiusdoubleecl_time_primaryTime of mid-eclipse of the primary by the secondarydtime.crossingdoubleecl_time_secondaryTime of mid-eclipse of the secondary by the primarydtime.crossingdoubleecl_dur_primaryDuration of primary eclipse assuming spherical componentsdtime.durationdoubleecl_dur_secondaryDuration of secondary eclipse assuming spherical componentsdtime.durationdoubleg_luminosity_ratioRatio of the G-band luminosity of the secondary over the primaryphys.luminosity;arith.ratiodoubleinput_period_errorStandard error of the period taken from VariEclipsingBinary.frequencyErrordstat.error;time.periodfloatg_rankRank of the G-band solutionstat.fit.paramdoubleastrometric_jitterUncorrelated astrometric jitter termmasstat.valuedoublegaiadr3.nss_vim_flThis table contains non-single-star (NSS) models for sources compatible with an Variability Induced Mover (VIM) solution.solution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongnss_solution_typeNSS model adoptedmeta.code.classcharraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallaxdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallaxfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloatref_flux_gReference flux in the G band"electron".s**-1phot.flux;em.optfloatvim_d_raVIM coordinate in RAmaspos.eq.radoublevim_d_ra_errorStandard error of VIM coordinate in RAmasstat.error;pos.eq.rafloatvim_d_decVIM coordinate in DECmaspos.eq.decdoublevim_d_dec_errorStandard error of VIM coordinate in DECmasstat.error;pos.eq.decfloatastrometric_n_obs_alTotal astrometric CCD observations in AL consideredmeta.numbercharastrometric_n_good_obs_alTotal astrometric CCD observations in AL actually usedmeta.numbercharbit_indexBoolean mask for the fields above in the corrVec matrixmeta.code.statuslongcorr_vecVector form of the upper triangle of the correlation matrixstat.correlationcharobj_funcValue of the objective function at the solutionstat.fit.paramfloatgoodness_of_fitGoodness of fit in the Hipparcos sensestat.fit.goodnessfloatefficiencyEfficiency of the solutionstat.fit.paramfloatsignificanceThe significance of the solution (i.e. how worth keeping a model is)stat.fit.paramfloatflagsQuality flag for the achieved NSS solutionmeta.code.quallonggaiadr3.vari_agnThis table provides information on AGN properties.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongfractional_variability_gFractional variability in the G bandsrc.varfloatstructure_function_indexIndex of the first-order structure function in the G bandstat.paramfloatstructure_function_index_scatterStandard deviation of the index of the structure functionstat.paramfloatqso_variabilityQuasar variability metric in the G bandsrc.varfloatnon_qso_variabilityNon-quasar variability metric in the G bandsrc.varfloatgaiadr3.vari_cepheidThis table describes the Cepheid stars.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongpfPeriod corresponding to the fundamental pulsation mode in the G band time seriesdsrc.var;time.perioddoublepf_errorUncertainty of the <tt>pf</tt> perioddstat.error;time.periodfloatp1_oPeriod corresponding to the first overtone pulsation mode in the G band time seriesdsrc.var;time.perioddoublep1_o_errorUncertainty of the <tt>p1O</tt> perioddstat.error;time.periodfloatepoch_gEpoch of the maximum of the light curve in the G banddtime.epoch;stat.maxdoubleepoch_g_errorUncertainty on the epoch parameter <tt>epochG</tt>dstat.error;time.epochfloatepoch_bpEpoch of the maximum of the light curve in the BP banddtime.epoch;stat.maxdoubleepoch_bp_errorUncertainty on the epoch parameter <tt>epochBp</tt>dstat.error;time.epochfloatepoch_rpEpoch of the maximum of the light curve in the RP banddtime.epoch;stat.maxdoubleepoch_rp_errorUncertainty on the epoch parameter <tt>epochRp</tt>dstat.error;time.epochfloatepoch_rvEpoch of the minimum of the radial velocity curvedtime.epoch;stat.maxdoubleepoch_rv_errorUncertainty on the epoch parameter <tt>epochRv</tt>dstat.error;time.epochfloatint_average_gIntensity-averaged magnitude in the G bandmagphot.mag;em.optfloatint_average_g_errorUncertainty on <tt>intAverageG</tt> parametermagstat.error;phot.mag;em.optfloatint_average_bpIntensity-averaged magnitude in the BP bandmagstat.error;phot.magfloatint_average_bp_errorUncertainty on <tt>intAverageBp</tt> parametermagstat.error;phot.magfloatint_average_rpIntensity-averaged magnitude in the RP bandmagstat.error;phot.magfloatint_average_rp_errorUncertainty on <tt>intAverageRp</tt> parametermagstat.error;phot.magfloataverage_rvMean radial velocitykm.s**-1spect.dopplerVeloc;stat.meanfloataverage_rv_errorUncertainty on <tt>averageRv</tt> parameterkm.s**-1stat.error;spect.dopplerVeloc;stat.meanfloatpeak_to_peak_gPeak-to-peak amplitude of the G band light curvemagsrc.var.amplitude;em.optfloatpeak_to_peak_g_errorUncertainty on the <tt>peakToPeakG</tt> parametermagstat.error;src.var.amplitude;em.optfloatpeak_to_peak_bpPeak-to-peak amplitude of the BP band light curvemagsrc.var.amplitudefloatpeak_to_peak_bp_errorUncertainty on the <tt>peakToPeakBp</tt> parametermagstat.error;src.var.amplitudefloatpeak_to_peak_rpPeak-to-peak amplitude of the RP band light curvemagsrc.var.amplitudefloatpeak_to_peak_rp_errorUncertainty on the <tt>peakToPeakRp</tt> parametermagstat.error;src.var.amplitudefloatpeak_to_peak_rvPeak-to-peak amplitude of the radial velocity curvekm.s**-1spect.dopplerVeloc;stat.paramdoublepeak_to_peak_rv_errorUncertainty on the <tt>peakToPeakRv</tt> parameterkm.s**-1stat.errordoublemetallicityMetallicity of the star from the Fourier parameters of the light curve"dex"phys.abund.Zfloatmetallicity_errorUncertainty of the <tt>metallicity</tt> parameter"dex"stat.error;phys.abund.Zfloatr21_gFourier decomposition parameter <tt>r21G</tt>: A2/A1 (for G band)stat.Fourierfloatr21_g_errorUncertainty on the <tt>r21G</tt> parameter: A2/A1 (for G band)stat.errorfloatr31_gFourier decomposition parameter <tt>r31G</tt>: A3/A1 (for G band)stat.Fourierfloatr31_g_errorUncertainty on the <tt>r31G</tt> parameter: A3/A1 (for G band)stat.errorfloatphi21_gFourier decomposition parameter <tt>phi21G</tt>: phi2 - 2*phi1 (for G band)radstat.Fourierfloatphi21_g_errorUncertainty on the <tt>phi21G</tt> parameter: phi2 - 2*phi1 (for G band)radstat.errorfloatphi31_gFourier decomposition parameter <tt>phi31G</tt>: phi3 - 3*phi1 (for G band)radstat.Fourierfloatphi31_g_errorUncertainty on the <tt>phi31G</tt> parameter: phi3 - 3*phi1 (for G band)radstat.errorfloatnum_clean_epochs_gNumber of G FoV epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_bpNumber of BP epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_rpNumber of RP epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_rvNumber of radial velocity epochs used in the fitting algorithmmeta.numbershortzp_mag_gZero point (mag) of the final model of the G band light curvemagphot.calib;em.optfloatzp_mag_bpZero point (mag) of the final model of the BP band light curvemagphot.calib;em.opt.Bfloatzp_mag_rpZero point (mag) of the final model of the RP band light curvemagphot.calib;em.opt.Rfloatnum_harmonics_for_p1_gNumber of harmonics used to model the first periodicity of the G-band light curvemeta.numbershortnum_harmonics_for_p1_bpNumber of harmonics used to model the first periodicity of the BP-band light curvemeta.numbershortnum_harmonics_for_p1_rpNumber of harmonics used to model the first periodicity of the RP-band light curvemeta.numbershortnum_harmonics_for_p1_rvNumber of harmonics used to model the first periodicity of the radial velocity curvemeta.numbershortreference_time_gReference time of the Fourier modelled G-band light curvedtime.epochdoublereference_time_bpReference time of the Fourier modelled BP-band light curvedtime.epochdoublereference_time_rpReference time of the Fourier modelled RP-band light curvedtime.epochdoublereference_time_rvReference time of the Fourier modelled radial velocity curvedtime.epochdoublefund_freq1First frequency of the non-linear Fourier modellingd**-1stat.Fourierdoublefund_freq1_errorError of the first frequency of the non-linear Fourier modellingd**-1stat.Fourierfloatfund_freq2Second frequency of the non-linear Fourier modelling in the G bandd**-1stat.Fourierdoublefund_freq2_errorError of the second frequency of the non-linear Fourier modelling in the G bandd**-1stat.Fourierfloatfund_freq1_harmonic_ampl_gAmplitudes of the Fourier model for the first frequency in the G bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_g_errorErrors of the amplitudes of the Fourier model for the first frequency in the G bandmagstat.errorcharfund_freq1_harmonic_phase_gPhases of the Fourier model for the first frequency in the G bandradstat.Fouriercharfund_freq1_harmonic_phase_g_errorErrors of the phases of the Fourier model for the first frequency in the G bandradstat.errorcharfund_freq1_harmonic_ampl_bpAmplitudes of the Fourier model for the first frequency in the BP bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_bp_errorErrors of the amplitudes of the Fourier model for the first frequency in the BP bandmagstat.errorcharfund_freq1_harmonic_phase_bpPhases of the Fourier model for the first frequency in the BP bandradstat.Fouriercharfund_freq1_harmonic_phase_bp_errorErrors of the phases of the Fourier model for the first frequency in the BP bandradstat.errorcharfund_freq1_harmonic_ampl_rpAmplitudes of the Fourier model for the first frequency in the RP bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_rp_errorErrors of the amplitudes of the Fourier model for the first frequency in the RP bandmagstat.errorcharfund_freq1_harmonic_phase_rpPhases of the Fourier model for the first frequency in the RP bandradstat.Fouriercharfund_freq1_harmonic_phase_rp_errorErrors of the phases of the Fourier model for the first frequency in the RP bandradstat.errorcharfund_freq1_harmonic_ampl_rvAmplitudes of the Fourier model for the first frequency of the radial velocity curvekm.s**-1src.var.amplitudecharfund_freq1_harmonic_ampl_rv_errorErrors of the amplitudes of the Fourier model for the first frequency of the radial velocity curvekm.s**-1stat.errorcharfund_freq1_harmonic_phase_rvPhases of the Fourier model for the first frequency of the radial velocity curveradstat.Fouriercharfund_freq1_harmonic_phase_rv_errorErrors of the phases of the Fourier model for the first frequency of the radial velocity curveradstat.errorcharp2_oPeriod corresponding to the second overtone pulsation mode (for multi mode pulsators) in the G band time seriesdsrc.var;time.perioddoublep2_o_errorUncertainty of the p2O perioddstat.error;time.periodfloattype_best_classificationBest type classification estimate out of: `DCEP", `T2CEP", `ACEP"meta.code.class;src.classchartype2_best_sub_classificationBest subclassification estimate for typeBestClassification=`T2CEP" out of: `BL_HER", `W_VIR",`RV_TAU"meta.code.class;src.classcharmode_best_classificationBest mode classification estimate out of: `FUNDAMENTAL", `FIRST_OVERTONE", `SECOND_OVERTONE", `MULTI",`UNDEFINED", `NOT_APPLICABLE"meta.code.class;src.classcharmulti_mode_best_classificationBest multi mode DCEP classification out of: `F/1O", `F/2O", `1O/2O", `1O/3O", `2O/3O", `F/1O/2O", `1O/2O/3O"meta.code.class;src.classchargaiadr3.vari_classifier_class_definitionTable with detailed descriptions of published classes for each classifier described in <code>vari_classifier_definition</code> and used in table <code>vari_classifier_result</code>.solution_idSolution Identifiermeta.versionlongclassifier_nameName of the classifier that is detailed in this entrymeta.titlecharclass_nameName of the published class from this classifiermeta.code.classcharclass_descriptionDescription of the published class from this classifiermeta.notechargaiadr3.vari_classifier_definitionTable with detailed descriptions of all classifiers used in table <code>vari_classifier_result</code>.solution_idSolution Identifiermeta.versionlongclassifier_nameName of the classifier that is detailed in this entrymeta.titlecharclassifier_descriptionDescription of this classifiermeta.notechargaiadr3.vari_classifier_resultTable with variability classification results of all classifiers, which are identified by the <code>classifier_name</code> column.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongclassifier_nameClassifier name used to produce this result, use for lookup in <tt>VariClassifierDefinition</tt> tablemeta.titlecharbest_class_nameName of best class, see table <tt>VariClassifierClassDefinition</tt> for details of the classmeta.code.classcharbest_class_scoreScore of the best classmeta.code.qualfloatgaiadr3.vari_compact_companionThis table describes the compact companion candidates.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongperiodOrbital perioddtime.perioddoubleperiod_errorOrbital period errordstat.error;time.periodfloatt0_gG-band reference timedtime.epochdoublet0_g_errorG-band reference time errordstat.error;time.epochfloatt0_bpBP-band reference timedtime.epochdoublet0_bp_errorBP-band reference time errordstat.error;time.epochfloatt0_rpRP-band reference timedtime.epochdoublet0_rp_errorRP-band reference time errordstat.error;time.epochfloatharmonic_model_params_gG-band harmonicsmagstat.Fouriercharharmonic_model_params_g_errorG-band harmonics errorsmagstat.Fouriercharharmonic_model_params_bpBP-band harmonicsmagstat.Fouriercharharmonic_model_params_bp_errorBP-band harmonics errorsmagstat.Fouriercharharmonic_model_params_rpRP-band harmonicsmagstat.Fouriercharharmonic_model_params_rp_errorRP-band harmonics errorsmagstat.Fouriercharmodel_mean_gHarmonics model mean G-band magnitudemagphot.mag;stat.meanfloatmodel_mean_g_errorHarmonics model mean G-band magnitude errormagstat.errorfloatmodel_mean_bpHarmonics model mean BP-band magnitudemagphot.mag;stat.meanfloatmodel_mean_bp_errorHarmonics model mean BP-band magnitude errormagstat.errorfloatmodel_mean_rpHarmonics model mean RP-band magnitudemagphot.mag;stat.meanfloatmodel_mean_rp_errorHarmonics model mean RP-band magnitude errormagstat.errorfloatmod_min_mass_ratioModified minimum mass ratiophys.mass;arith.ratiofloatmod_min_mass_ratio_one_sigma15.9 percentile modified minimum mass ratiophys.mass;arith.ratiofloatmod_min_mass_ratio_three_sigma0.135 percentile modified minimum mass ratiophys.mass;arith.ratiofloatalphaalpha ellipsoidal coefficientstat.fit.paramfloatgaiadr3.vari_eclipsing_binaryThis table describes the properties of the eclipsing binaries resulting from the variability analysis.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongglobal_rankingNumber between 0 (worst) and 1 (best)stat.paramfloatreference_timeReference time used for the geometric model fitdtime.epochdoublefrequencyFrequency of geometric model of the eclipsing binary light curved**-1src.orbitaldoublefrequency_errorUncertainty of <tt>frequency</tt>d**-1stat.errorfloatgeom_model_reference_levelMagnitude reference level of geometric modelmagphot.mag;em.optfloatgeom_model_reference_level_errorUncertainty of <tt>geomModelReferenceLevel</tt>magstat.error;phot.mag;em.optfloatgeom_model_gaussian1_phasePhase of the Gaussian 1 componenttime.phasefloatgeom_model_gaussian1_phase_errorUncertainty of <tt>geomModelGaussian1Phase</tt>stat.error;time.phasefloatgeom_model_gaussian1_sigmaStandard deviation [phase] of Gaussian 1 componentstat.stdevfloatgeom_model_gaussian1_sigma_errorUncertainty of <tt>geomModelGaussian1Sigma</tt>stat.errorfloatgeom_model_gaussian1_depthMagnitude depth of Gaussian 1 componentmagsrc.var.amplitudefloatgeom_model_gaussian1_depth_errorUncertainty of <tt>geomModelGaussian1Depth</tt>magstat.error;src.var.amplitudefloatgeom_model_gaussian2_phasePhase of Gaussian 2 componenttime.phasefloatgeom_model_gaussian2_phase_errorUncertainty of <tt>geomModelGaussian2Phase</tt>stat.error;time.phasefloatgeom_model_gaussian2_sigmaStandard deviation [phase] of Gaussian 2 componentstat.stdevfloatgeom_model_gaussian2_sigma_errorUncertainty of <tt>geomModelGaussian2Sigma</tt>stat.errorfloatgeom_model_gaussian2_depthMagnitude depth of Gaussian2 componentmagsrc.var.amplitudefloatgeom_model_gaussian2_depth_errorUncertainty of <tt>geomModelGaussian2Depth</tt>magstat.error;src.var.amplitudefloatgeom_model_cosine_half_period_amplitudeAmplitude of the cosine component with half the period of the geometric modelmagsrc.var.amplitudefloatgeom_model_cosine_half_period_amplitude_errorUncertainty of <tt>geomModelCosineHalfPeriodAmplitude</tt>magstat.error;src.var.amplitudefloatgeom_model_cosine_half_period_phaseReference phase of the cosine component with half the period of the geometric modeltime.phasefloatgeom_model_cosine_half_period_phase_errorUncertainty of <tt>geomModelCosineHalfPeriodPhase</tt>stat.error;time.phasefloatmodel_typeType of geometrical model of the light curvemeta.code.classcharnum_model_parametersNumber of free parameters of the geometric modelstat.fit.paramshortreduced_chi2Reduced Chi2 of the geometrical model fitstat.fit.chi2floatderived_primary_ecl_phasePrimary eclipse: phase at geometrically deepest pointtime.phasefloatderived_primary_ecl_phase_errorPrimary eclipse: uncertainty of <tt>derivedPrimaryEclPhase</tt>stat.error;time.phasefloatderived_primary_ecl_durationPrimary eclipse: duration [phase fraction]time.durationfloatderived_primary_ecl_duration_errorPrimary eclipse: uncertainty of <tt>derivedPrimaryEclDuration</tt>stat.error;time.durationfloatderived_primary_ecl_depthPrimary eclipse: depthmagsrc.var.amplitudefloatderived_primary_ecl_depth_errorPrimary eclipse: uncertainty of <tt>derivedPrimaryEclDepth</tt>magstat.error;src.var.amplitudefloatderived_secondary_ecl_phaseSecondary eclipse: phase at geometrically second deepest pointtime.phasefloatderived_secondary_ecl_phase_errorSecondary eclipse: uncertainty of <tt>derivedSecondaryEclPhase</tt>stat.error;time.phasefloatderived_secondary_ecl_durationSecondary eclipse: duration [phase fraction]time.durationfloatderived_secondary_ecl_duration_errorSecondary eclipse: uncertainty of <tt>derivedSecondaryEclDuration</tt>stat.error;time.durationfloatderived_secondary_ecl_depthSecondary eclipse: depthmagsrc.var.amplitudefloatderived_secondary_ecl_depth_errorSecondary eclipse: uncertainty of <tt>derivedSecondaryEclDepth</tt>magstat.error;src.var.amplitudefloatgaiadr3.vari_epoch_radial_velocityThis table contains the epoch radial velocity data points for a sub-set of variable stars. Each entry is a radial velocity in the solar barycentric reference frame for a given object and observation time.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongtransit_idTransit unique identifiermeta.idlongrv_obs_timeObserving time of the transitdtime.epochdoubleradial_velocityBarycentric radial velocitykm.s**-1spect.dopplerVeloc.optdoubleradial_velocity_errorBarycentric radial velocity errorkm.s**-1stat.error;spect.dopplerVeloc.optdoublerejected_by_variabilityRejected by DPAC variability processing (or variability analysis)meta.code.statusbooleansolution_idSolution Identifiermeta.versionlonggaiadr3.vari_long_period_variableThis table describes the Long Period Variable stars.Some entries can be NaN when absent.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongfrequencyFrequency of the LPVd**-1src.var.pulsedoublefrequency_errorError on the frequencyd**-1stat.error;src.var.pulsefloatamplitudeAmplitude of the LPV variabilitymagsrc.var.amplitudefloatmedian_delta_wl_rpMedian of the pseudo-wavelength separations between the two highest peaks in RP spectraem.wl;stat.medianfloatis_cstarFlag to mark C-starsmeta.code.classbooleangaiadr3.vari_microlensingThis table describes the microlensing events.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongpaczynski0_g0G-band magnitude baseline (level 0)magphot.mag;em.optfloatpaczynski0_g0_errorError of G-band magnitude baseline (level 0)magstat.error;phot.mag;em.optfloatpaczynski0_bp0BP-band magnitude baseline (level 0)magphot.mag;em.opt.Bfloatpaczynski0_bp0_errorError of BP-band magnitude baseline (level 0)magstat.error;phot.mag;em.opt.Bfloatpaczynski0_rp0RP-band magnitude baseline (level 0)magphot.mag;em.opt.Rfloatpaczynski0_rp0_errorError of RP-band magnitude baseline (level 0)magstat.error;phot.mag;em.opt.Rfloatpaczynski0_u0Impact parameter (level 0)stat.paramdoublepaczynski0_u0_errorError of the impact parameter (level 0)stat.errordoublepaczynski0_teEvent timescale (level 0)dtime.epochfloatpaczynski0_te_errorError of event timescale (level 0)dstat.error;time.epochfloatpaczynski0_tmaxTime of maximum amplification (level 0)dtime;stat.maxdoublepaczynski0_tmax_errorError of time of maximum amplification (level 0)dstat.errordoublepaczynski0_chi2Chi square of level 0 Paczynski fitstat.fit.chi2floatpaczynski0_chi2_dofReduced chi square of level 0 Paczynski fitstat.fit.chi2floatpaczynski1_g0G-band magnitude baseline (level 1)magphot.mag;em.optfloatpaczynski1_g0_errorError of G-band magnitude baseline (level 1)magstat.error;phot.mag;em.optfloatpaczynski1_bp0BP-band magnitude baseline (level 1)magphot.mag;em.opt.Bfloatpaczynski1_bp0_errorError of BP-band magnitude baseline (level 1)magstat.error;phot.mag;em.opt.Bfloatpaczynski1_rp0RP-band magnitude baseline (level 1)magphot.mag;em.opt.Rfloatpaczynski1_rp0_errorError of RP-band magnitude baseline (level 1)magstat.error;phot.mag;em.opt.Rfloatpaczynski1_u0Impact parameter (level 1)stat.paramdoublepaczynski1_u0_errorError of the impact parameter (level 1)stat.errordoublepaczynski1_teEvent timescale (level 1)dtime.epochfloatpaczynski1_te_errorError of event timescale (level 1)dstat.error;time.epochfloatpaczynski1_tmaxTime of maximum amplification (level 1)dtime;stat.maxdoublepaczynski1_tmax_errorError of time of maximum amplification (level 1)dstat.error;timedoublepaczynski1_fs_gBlending factor in G-band (level 1)stat.paramfloatpaczynski1_fs_g_errorError of blending factor in G-band (level 1)stat.errorfloatpaczynski1_fs_bpBlending factor in BP-band (level 1)stat.paramfloatpaczynski1_fs_bp_errorError of blending factor in BP-band (level 1)stat.errorfloatpaczynski1_fs_rpBlending factor in RP-band (level 1)stat.paramfloatpaczynski1_fs_rp_errorError of blending factor in RP-band (level 1)stat.errorfloatpaczynski1_chi2Chi square of level 1 Paczynski fitstat.fit.chi2floatpaczynski1_chi2_dofReduced chi square of level 1 Paczynski fitstat.fit.chi2floatgaiadr3.vari_ms_oscillatorThis table describes the main-sequence (MS) oscillators.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongfrequency1Best frequencyd**-1src.var.pulsedoublefap_g_freq1False alarm probability corresponding to the best frequencystat.probabilityfloatamplitude_g_freq1Half peak-to-peak amplitude in the G band of the best frequencymagsrc.var.amplitudefloatphase_g_freq1Phase of the oscillation in the G band corresponding to best frequencyradtime.phasefloatnum_harmonicsNumber of significant harmonics of the best frequencymeta.numbershortamplitude_g_freq1_harm2Half peak-to-peak amplitude in the G band of the second harmonic of the best frequencymagstat.Fourier.amplitudefloatphase_g_freq1_harm2Phase of the oscillation in the G band corresponding to the second harmonic of the best frequencyradtime.phasefloatamplitude_g_freq1_harm3Half peak-to-peak amplitude in the G band of the third harmonic of the best frequencymagstat.Fourier.amplitudefloatphase_g_freq1_harm3Phase of the oscillation in the G band corresponding to the third harmonic of the best frequencyradtime.phasefloatgaiadr3.vari_planetary_transitThis table describes the Planetary Transit candidate events.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongtransit_reference_timeMid-transit reference timedtimedoubletransit_periodMost probable transit perioddtime.perioddoubletransit_depthTransit depthmmagphot.mag;src.var.amplitudefloattransit_durationTransit durationdtime.durationfloatnum_in_transitNumber of in-transit observationsmeta.numbershortgaiadr3.vari_spurious_signalsSeveral statistics which can help in the identification of sources that are affected by calibration issues.source_idSource Identifiermeta.id;meta.mainlongphot_variable_flagPhotometric variability flagmeta.code;src.varcharin_andromeda_surveyFlag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS)meta.code.statusbooleannum_obs_common_all_bandsNumber of observations in common for G, BP and RP bands, used in computation of the Spearman correlation excess factor fieldsmeta.numbershortnum_obs_g_fovNumber of selected observations of G FoV transits, used in the frequency fieldsmeta.numbershortgls_freq_g_fovFrequency identified by Generalised Least Squares period search on G FoV timeseriesd**-1stat.valuedoublegls_freq_ampl_g_fovNormalised amplitude of the frequency identified by Generalised Least Squares period search on G FoV timeseriesstat.valuefloatgls_freq_sde_g_fovSignal Detection Efficiency (SDE) of the frequency identified by Generalised Least Squares period search on G FoV timeseriesstat.snrfloatgls_freq_fap_g_fovFalse Alarm Probability (FAP) of the frequency identified by Generalised Least Squares period search on G FoV timeseriesstat.probabilitydoublenhm_fund_freq_g_fovFundamental frequency identified by non-linear harmonic modelling on G FoV timeseries, initialised by the Generalised Least Squares frequencyd**-1stat.valuedoublenhm_fund_freq_error_g_fovUncertainty of the fundamental frequency identified by non-linear harmonic modelling on G FoV timeseriesd**-1stat.errorfloatspearman_corr_exf_g_fovG-band FoV photometry Spearman correlation with corrected flux excess factorstat.correlationfloatnum_obs_excl_epsl_g_fovNumber of G-band FoV photometry observations excluding EPSL, used for the IPD correlation and scan angle modelling in the G bandmeta.numbershortspearman_corr_ipd_g_fovG-band FoV photometry Spearman correlation with IPD modelstat.correlationfloatscan_angle_model_offset_g_fovMagnitude offset of the scan angle model fit to G-band FoV photometrymagstat.fit.paramfloatscan_angle_model_ampl_g_fovAmplitude of the scan angle model fit to G-band FoV photometrymagstat.fit.paramfloatscan_angle_model_ampl_sig_g_fovSignificance of the amplitude of the scan angle model fit to G-band FoV photometrystat.fit.goodnessfloatscan_angle_model_phase_g_fovPhase of the scan angle model fit to G-band FoV photometrydegstat.fit.paramfloatscan_angle_model_red_chi2_g_fovReduced Chi2 of the scan angle model fit to G-band FoV photometrystat.fit.goodnessfloatscan_angle_model_f2_g_fovF2 goodness-of-fit of the scan angle model fit to G-band FoV photometrystat.fit.goodnessfloatspearman_corr_exf_bpBP-band photometry Spearman correlation with corrected flux excess factorstat.correlationfloatnum_obs_excl_epsl_bpNumber of BP-band photometry observations excluding EPSL, used for the IPD correlation and scan angle modelling in the BP bandmeta.numbershortspearman_corr_ipd_bpBP-band Spearman correlation with IPD modelstat.correlationfloatscan_angle_model_offset_bpMagnitude offset of the scan angle model fit to BP-band photometrymagstat.fit.paramfloatscan_angle_model_ampl_bpAmplitude of the scan angle model fit to BP-band photometrymagstat.fit.paramfloatscan_angle_model_ampl_sig_bpSignificance of the amplitude of the scan angle model fit to BP-band photometrystat.fit.goodnessfloatscan_angle_model_phase_bpPhase of the scan angle model fit to BP-band photometrydegstat.fit.paramfloatscan_angle_model_red_chi2_bpReduced Chi2 of the scan angle model fit to BP-band photometrystat.fit.goodnessfloatscan_angle_model_f2_bpF2 goodness-of-fit of the scan angle model fit to BP-band photometrystat.fit.goodnessfloatspearman_corr_exf_rpRP-band photometry Spearman correlation with corrected flux excess factorstat.correlationfloatnum_obs_excl_epsl_rpNumber of RP-band photometry observations excluding EPSL, used for the IPD correlation and scan angle modelling in the RP bandmeta.numbershortspearman_corr_ipd_rpRP-band Spearman correlation with IPD modelstat.correlationfloatscan_angle_model_offset_rpMagnitude offset of the scan angle model fit to RP-band photometrymagstat.fit.paramfloatscan_angle_model_ampl_rpAmplitude of the scan angle model fit to RP-band photometrymagstat.fit.paramfloatscan_angle_model_ampl_sig_rpSignificance of the amplitude of the scan angle model fit to RP-band photometrystat.fit.goodnessfloatscan_angle_model_phase_rpPhase of the scan angle model fit to RP-band photometrydegstat.fit.paramfloatscan_angle_model_red_chi2_rpReduced Chi2 of the scan angle model fit to RP-band photometrystat.fit.goodnessfloatscan_angle_model_f2_rpF2 goodness-of-fit of the scan angle model fit to RP-band photometrystat.fit.goodnessfloatgaiadr3.vari_rad_vel_statisticsStatistical parameters of radial velocity time series, using only transits not rejected, see <code>rejected_by_variability</code> column in <code>vari_epoch_radial_velocity</code>.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_selected_rvTotal number of radial velocity transits selected for variability analysismeta.numbershortmean_obs_time_rvMean observation time for radial velocity transitsdtime.epoch;stat.meandoubletime_duration_rvTime duration of the time series for radial velocity transitsdtime.durationfloatmin_rvMinimum radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.minfloatmax_rvMaximum radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.maxfloatmean_rvMean radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.meanfloatmedian_rvMedian radial velocitykm.s**-1spect.dopplerVeloc.opt;stat.medianfloatrange_rvDifference between the highest and lowest radial velocity transitskm.s**-1spect.dopplerVeloc.opt;arith.difffloatstd_dev_rvSquare root of the unweighted radial velocity variancekm.s**-1stat.stdev;spect.dopplerVeloc.optfloatskewness_rvStandardized unweighted radial velocity skewnessspect.dopplerVeloc.opt;stat.paramfloatkurtosis_rvStandardized unweighted radial velocity kurtosisspect.dopplerVeloc.opt;stat.paramfloatmad_rvMedian Absolute Deviation (MAD) for radial velocity transitskm.s**-1spect.dopplerVeloc.opt;stat.paramfloatabbe_rvAbbe value for radial velocity transitsspect.dopplerVeloc.opt;stat.paramfloatiqr_rvInterquartile range for radial velocity transitskm.s**-1spect.dopplerVeloc.opt;stat.paramfloatgaiadr3.vari_rotation_modulationThis table describes the solar-like stars with rotational modulation.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_segmentsNumber of segmentsmeta.numbershortsegments_start_timeTimes at which segments startdmeta.dataset;time.startcharsegments_end_timeTimes at which segments enddmeta.dataset;time.endcharsegments_colour_mag_interceptColour-Magnitude Intercept in segmentsstat.fit.paramcharsegments_colour_mag_intercept_errorColour-Magnitude Intercept uncertainty in segmentsstat.error;stat.fit.paramcharsegments_colour_mag_slopeColour-Magnitude Slope in segmentsstat.fit.paramcharsegments_colour_mag_slope_errorColour-Magnitude Slope uncertainty in segmentsstat.error;stat.fit.paramcharsegments_correlation_coefficientCorrelation coefficient in segmentsstat.correlationcharsegments_correlation_significanceCorrelation coefficient significance in segmentsstat.correlationcharnum_outliersNumber of outliersmeta.numbershortoutliers_timeTimes at which outliers occursdmeta.dataset;timecharsegments_rotation_periodRotation period in segmentdphys.veloc.rotat;time.periodcharsegments_rotation_period_errorRotation period uncertainty in segmentdstat.error;phys.veloc.rotat;time.periodcharsegments_rotation_period_fapFAP on rotation period in segmentstat.probabilitycharbest_rotation_periodBest rotation perioddphys.veloc.rotat;time.perioddoublebest_rotation_period_errorError on best rotation perioddstat.error;phys.veloc.rotat;time.periodfloatsegments_g_unspottedThe unspotted G mags in segmentmagphot.mag;em.optcharsegments_g_unspotted_errorThe unspotted G mag uncertainties in segmentmagstat.error;phot.mag;em.optcharsegments_bp_unspottedThe unspotted BP mag in segmentmagphot.mag;em.opt.Bcharsegments_bp_unspotted_errorThe unspotted BP mag uncertainties in segmentmagstat.error;phot.mag;em.opt.Bcharsegments_rp_unspottedThe unspotted RP mag in segmentmagphot.mag;em.opt.Rcharsegments_rp_unspotted_errorThe unspotted RP mag uncertainties in segmentmagstat.error;phot.mag;em.opt.Rcharg_unspottedUnspotted G magmagphot.mag;em.optfloatg_unspotted_errorUnspotted G mag uncertaintymagstat.error;em.opt;phot.magfloatbp_unspottedUnspotted BP magmagphot.mag;em.opt.Bfloatbp_unspotted_errorUnspotted BP mag uncertaintymagstat.error;phot.mag;em.opt.Bfloatrp_unspottedUnspotted RP magmagphot.mag;em.opt.Rfloatrp_unspotted_errorUnspotted RP mag uncertaintymagstat.error;phot.mag;em.opt.Rfloatsegments_g_cos_termCoefficient of cosine term of linear fit in segment in the G bandmagstat.fit.paramcharsegments_g_cos_term_errorErrors on cosine terms in the G bandmagstat.errorcharsegments_g_sin_termCoefficient of sine term of linear fit in segment in the G bandmagstat.fit.paramcharsegments_g_sin_term_errorErrors on sine terms in the G bandmagstat.errorcharsegments_g_a0_termConstant term (A0) of linear fit in segment in the G bandmagstat.fit.paramcharsegments_g_a0_term_errorErrors on constant terms in the G bandmagstat.errorcharsegments_bp_cos_termCoefficient of cosine term of linear fit in segment in the BP bandmagstat.fit.paramcharsegments_bp_cos_term_errorErrors on cosine terms in the BP bandmagstat.errorcharsegments_bp_sin_termCoefficient of sine term of linear fit in segment in the BP bandmagstat.fit.paramcharsegments_bp_sin_term_errorErrors on sine terms in the BP bandmagstat.errorcharsegments_bp_a0_termConstant term (A0) of linear fit in segment in the BP bandmagstat.fit.paramcharsegments_bp_a0_term_errorErrors on constant terms in the BP bandmagstat.errorcharsegments_rp_cos_termCoefficient of cosine term of linear fit in segment in the RP bandmagstat.fit.paramcharsegments_rp_cos_term_errorErrors on cosine terms in the RP bandmagstat.errorcharsegments_rp_sin_termCoefficient of sine term of linear fit in segment in the RP bandmagstat.fit.paramcharsegments_rp_sin_term_errorErrors on sine terms in the RP bandmagstat.errorcharsegments_rp_a0_termConstant term (A0) of linear fit in segment in the RP bandmagstat.fit.paramcharsegments_rp_a0_term_errorErrors on constant terms in the RP bandmagstat.errorcharsegments_g_activity_indexActivity Index in segment (computed in G band)magsrc.var.amplitudecharsegments_g_activity_index_errorerror on Activity index in segment (computed in G band)magstat.error;src.var.amplitudecharsegments_bp_activity_indexActivity Index in segment (computed in BP band)magsrc.var.amplitudecharsegments_bp_activity_index_errorerror on Activity index in segment (computed in BP band)magstat.error;src.var.amplitudecharsegments_rp_activity_indexActivity Index in segment (computed in RP band)magsrc.var.amplitudecharsegments_rp_activity_index_errorerror on Activity index in segment (computed in RP band)magstat.error;src.var.amplitudecharmax_activity_index_gThe maximum Activity Index in the G bandmagsrc.var.amplitudefloatmax_activity_index_g_errorError on maximum activity index in the G bandmagstat.error;src.var.amplitudefloatsegments_bp_rp_corr_coeffPearson coefficient between BP and RP in segmentstat.correlationcharsegments_bp_rp_corr_signifSignificance associated with Pearson coefficientstat.fit.paramcharsegments_bp_rp_interceptIntercept of regression fit of RP vs BP magnitudes in the segmentmagstat.fit.paramcharsegments_bp_rp_intercept_errorError on intercept of regression fit of RP vs BP magnitudes in the segmentmagstat.errorcharsegments_bp_rp_slopeSlope of regression fit of RP vs BP magnitudes in the segmentstat.fit.paramcharsegments_bp_rp_slope_errorError on slope of regression fit of RP vs BP magnitudes in the segmentstat.errorcharsegments_model_reference_timeTime used as reference time for the period search procedure in the segmentdtime.epochcharsegments_g_chi_squareArray of chisquares for linear models (G band)stat.fit.chi2charsegments_bp_chi_squareArray of chisquares for linear models (BP band)stat.fit.chi2charsegments_rp_chi_squareArray of chisquares for linear models (RP band)stat.fit.chi2chargaiadr3.vari_rrlyraeThis table describes the RR Lyrae stars.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongpfPeriod corresponding to the fundamental pulsation mode in the G band time seriesdsrc.var;time.perioddoublepf_errorUncertainty of the <tt>pf</tt> perioddstat.error;time.periodfloatp1_oPeriod corresponding to the first overtone pulsation mode in the G band time seriesdsrc.var;time.perioddoublep1_o_errorUncertainty of the <tt>p1O</tt> perioddstat.error;time.periodfloatepoch_gEpoch of the maximum of the light curve in the G banddtime.epoch;stat.maxdoubleepoch_g_errorUncertainty on the epoch parameter <tt>epochG</tt>dstat.error;time.epochfloatepoch_bpEpoch of the maximum of the light curve in the BP banddtime.epoch;stat.maxdoubleepoch_bp_errorUncertainty on the epoch parameter <tt>epochBp</tt>dstat.error;time.epochfloatepoch_rpEpoch of the maximum of the light curve in the RP banddtime.epoch;stat.maxdoubleepoch_rp_errorUncertainty on the epoch parameter <tt>epochRp</tt>dstat.error;time.epochfloatepoch_rvEpoch of the minimum of the radial velocity curvedtime.epoch;stat.maxdoubleepoch_rv_errorUncertainty on the epoch parameter <tt>epochRv</tt>dstat.error;time.epochfloatint_average_gIntensity-averaged magnitude in the G bandmagphot.mag;em.optfloatint_average_g_errorUncertainty on <tt>intAverageG</tt> parametermagstat.error;phot.mag;em.optfloatint_average_bpIntensity-averaged magnitude in the BP bandmagstat.error;phot.magfloatint_average_bp_errorUncertainty on <tt>intAverageBp</tt> parametermagstat.error;phot.magfloatint_average_rpIntensity-averaged magnitude in the RP bandmagstat.error;phot.magfloatint_average_rp_errorUncertainty on <tt>intAverageRp</tt> parametermagstat.error;phot.magfloataverage_rvMean radial velocitykm.s**-1spect.dopplerVeloc;stat.meanfloataverage_rv_errorUncertainty on <tt>averageRv</tt> parameterkm.s**-1stat.error;spect.dopplerVeloc;stat.meanfloatpeak_to_peak_gPeak-to-peak amplitude of the G band light curvemagsrc.var.amplitude;em.optfloatpeak_to_peak_g_errorUncertainty on the <tt>peakToPeakG</tt> parametermagstat.error;src.var.amplitude;em.optfloatpeak_to_peak_bpPeak-to-peak amplitude of the BP band light curvemagsrc.var.amplitudefloatpeak_to_peak_bp_errorUncertainty on the <tt>peakToPeakBp</tt> parametermagstat.error;src.var.amplitudefloatpeak_to_peak_rpPeak-to-peak amplitude of the RP band light curvemagsrc.var.amplitudefloatpeak_to_peak_rp_errorUncertainty on the <tt>peakToPeakRp</tt> parametermagstat.error;src.var.amplitudefloatpeak_to_peak_rvPeak-to-peak amplitude of the radial velocity curvekm.s**-1spect.dopplerVeloc;stat.paramdoublepeak_to_peak_rv_errorUncertainty on the <tt>peakToPeakRv</tt> parameterkm.s**-1stat.errordoublemetallicityMetallicity of the star from the Fourier parameters of the light curve"dex"phys.abund.Zfloatmetallicity_errorUncertainty of the <tt>metallicity</tt> parameter"dex"stat.error;phys.abund.Zfloatr21_gFourier decomposition parameter <tt>r21G</tt>: A2/A1 (for G band)stat.Fourierfloatr21_g_errorUncertainty on the <tt>r21G</tt> parameter: A2/A1 (for G band)stat.errorfloatr31_gFourier decomposition parameter <tt>r31G</tt>: A3/A1 (for G band)stat.Fourierfloatr31_g_errorUncertainty on the <tt>r31G</tt> parameter: A3/A1 (for G band)stat.errorfloatphi21_gFourier decomposition parameter <tt>phi21G</tt>: phi2 - 2*phi1 (for G band)radstat.Fourierfloatphi21_g_errorUncertainty on the <tt>phi21G</tt> parameter: phi2 - 2*phi1 (for G band)radstat.errorfloatphi31_gFourier decomposition parameter <tt>phi31G</tt>: phi3 - 3*phi1 (for G band)radstat.Fourierfloatphi31_g_errorUncertainty on the <tt>phi31G</tt> parameter: phi3 - 3*phi1 (for G band)radstat.errorfloatnum_clean_epochs_gNumber of G FoV epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_bpNumber of BP epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_rpNumber of RP epochs used in the fitting algorithmmeta.numbershortnum_clean_epochs_rvNumber of radial velocity epochs used in the fitting algorithmmeta.numbershortzp_mag_gZero point (mag) of the final model of the G band light curvemagphot.calib;em.optfloatzp_mag_bpZero point (mag) of the final model of the BP band light curvemagphot.calib;em.opt.Bfloatzp_mag_rpZero point (mag) of the final model of the RP band light curvemagphot.calib;em.opt.Rfloatnum_harmonics_for_p1_gNumber of harmonics used to model the first periodicity of the G-band light curvemeta.numbershortnum_harmonics_for_p1_bpNumber of harmonics used to model the first periodicity of the BP-band light curvemeta.numbershortnum_harmonics_for_p1_rpNumber of harmonics used to model the first periodicity of the RP-band light curvemeta.numbershortnum_harmonics_for_p1_rvNumber of harmonics used to model the first periodicity of the radial velocity curvemeta.numbershortreference_time_gReference time of the Fourier modelled G-band light curvedtime.epochdoublereference_time_bpReference time of the Fourier modelled BP-band light curvedtime.epochdoublereference_time_rpReference time of the Fourier modelled RP-band light curvedtime.epochdoublereference_time_rvReference time of the Fourier modelled radial velocity curvedtime.epochdoublefund_freq1First frequency of the non-linear Fourier modellingd**-1stat.Fourierdoublefund_freq1_errorError of the first frequency of the non-linear Fourier modellingd**-1stat.Fourierfloatfund_freq2Second frequency of the non-linear Fourier modelling in the G bandd**-1stat.Fourierdoublefund_freq2_errorError of the second frequency of the non-linear Fourier modelling in the G bandd**-1stat.Fourierfloatfund_freq1_harmonic_ampl_gAmplitudes of the Fourier model for the first frequency in the G bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_g_errorErrors of the amplitudes of the Fourier model for the first frequency in the G bandmagstat.errorcharfund_freq1_harmonic_phase_gPhases of the Fourier model for the first frequency in the G bandradstat.Fouriercharfund_freq1_harmonic_phase_g_errorErrors of the phases of the Fourier model for the first frequency in the G bandradstat.errorcharfund_freq1_harmonic_ampl_bpAmplitudes of the Fourier model for the first frequency in the BP bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_bp_errorErrors of the amplitudes of the Fourier model for the first frequency in the BP bandmagstat.errorcharfund_freq1_harmonic_phase_bpPhases of the Fourier model for the first frequency in the BP bandradstat.Fouriercharfund_freq1_harmonic_phase_bp_errorErrors of the phases of the Fourier model for the first frequency in the BP bandradstat.errorcharfund_freq1_harmonic_ampl_rpAmplitudes of the Fourier model for the first frequency in the RP bandmagsrc.var.amplitudecharfund_freq1_harmonic_ampl_rp_errorErrors of the amplitudes of the Fourier model for the first frequency in the RP bandmagstat.errorcharfund_freq1_harmonic_phase_rpPhases of the Fourier model for the first frequency in the RP bandradstat.Fouriercharfund_freq1_harmonic_phase_rp_errorErrors of the phases of the Fourier model for the first frequency in the RP bandradstat.errorcharfund_freq1_harmonic_ampl_rvAmplitudes of the Fourier model for the first frequency of the radial velocity curvekm.s**-1src.var.amplitudecharfund_freq1_harmonic_ampl_rv_errorErrors of the amplitudes of the Fourier model for the first frequency of the radial velocity curvekm.s**-1stat.errorcharfund_freq1_harmonic_phase_rvPhases of the Fourier model for the first frequency of the radial velocity curveradstat.Fouriercharfund_freq1_harmonic_phase_rv_errorErrors of the phases of the Fourier model for the first frequency of the radial velocity curveradstat.errorcharbest_classificationBest RR Lyrae classification estimate out of: {`RRc", `RRab", `RRd"}meta.code.class;src.classcharg_absorptionInterstellar absorption in the G-bandmagphys.absorption.galfloatg_absorption_errorError on the interstellar absorption in the G-bandmagstat.error;phys.absorption.galfloatgaiadr3.vari_short_timescaleThis table describes the short-timescale sources.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongamplitude_estimateAmplitude estimate of all per-CCD G-band photometry (95th quantile - 5th quantile)magsrc.var.amplitude;phot.mag;em.optfloatnumber_of_fov_transitsNumber of FoV transits with more than 7 CCD measurements after time series cleaningmeta.numbershortmean_of_fov_abbe_valuesMean of per-FoV Abbe values derived from per-CCD G-band photometrystat.valuefloatvariogram_num_pointsNumber of selected timescale(s) derived from the variogrammeta.numbershortvariogram_char_timescalesCharacteristic timescale(s) of variabilitydtimecharvariogram_valuesVariogram values associated with the <tt>variogramCharTimescales</tt>mag**2stat.valuecharfrequencyFrequency search result for either G CCD, G FoV, BP or RP photometryd**-1src.var;time.perioddoublegaiadr3.vari_summarySummary table that provides the information on where a <code>source_id</code> can be found in the different <code>variability</code> tables and statistical parameters of time series, using only transits not rejected.solution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_selected_g_fovTotal number of G FOV transits selected for variability analysismeta.numbershortmean_obs_time_g_fovMean observation time for G FoV transitsdtime.epoch;stat.meandoubletime_duration_g_fovTime duration of the time series for G FoV transitsdtime.durationfloatmin_mag_g_fovMinimum G FoV magnitudemagphot.mag;stat.minfloatmax_mag_g_fovMaximum G FoV magnitudemagphot.mag;stat.maxfloatmean_mag_g_fovMean G FoV magnitudemagphot.mag;stat.meanfloatmedian_mag_g_fovMedian G FoV magnitudemagphot.mag;stat.medianfloatrange_mag_g_fovDifference between the highest and lowest G FoV magnitudesmagphot.mag;em.opt;arith.difffloattrimmed_range_mag_g_fovTrimmed difference between the highest and lowest G FoV magnitudesmagphot.mag;em.opt;arith.difffloatstd_dev_mag_g_fovSquare root of the unweighted G FoV magnitude variancemagstat.stdev;phot.mag;em.optfloatskewness_mag_g_fovStandardized unweighted G FoV magnitude skewnessstat.value;phot.mag;em.optfloatkurtosis_mag_g_fovStandardized unweighted G FoV magnitude kurtosisstat.value;phot.mag;em.optfloatmad_mag_g_fovMedian Absolute Deviation (MAD) for G FoV transitsmagstat.value;phot.mag;em.optfloatabbe_mag_g_fovAbbe value for G FoV transitsstat.value;phot.mag;em.optfloatiqr_mag_g_fovInterquartile range for G FoV transitsmagstat.value;phot.mag;em.optfloatstetson_mag_g_fovStetson G FoV variability indexsrc.var.indexfloatstd_dev_over_rms_err_mag_g_fovSignal-to-Noise G FoV estimatestat.snrfloatoutlier_median_g_fovGreatest absolute deviation from the G FoV median normalized by the errorstat.fit.paramfloatnum_selected_bpTotal number of BP observations selected for variability analysismeta.numbershortmean_obs_time_bpMean observation time for BP observationsdtime.epoch;stat.meandoubletime_duration_bpTime duration of the BP time seriesdtime.durationfloatmin_mag_bpMinimum BP magnitudemagphot.mag;stat.minfloatmax_mag_bpMaximum BP magnitudemagphot.mag;stat.maxfloatmean_mag_bpMean BP magnitudemagphot.mag;stat.meanfloatmedian_mag_bpMedian BP magnitudemagphot.mag;stat.medianfloatrange_mag_bpDifference between the highest and lowest BP magnitudesmagphot.mag;em.opt.B;arith.difffloattrimmed_range_mag_bpTrimmed difference between the highest and lowest BP magnitudesmagphot.mag;em.opt.B;arith.difffloatstd_dev_mag_bpSquare root of the unweighted BP magnitude variancemagstat.stdev;phot.mag;em.opt.Bfloatskewness_mag_bpStandardized unweighted BP magnitude skewnessstat.value;phot.mag;em.opt.Bfloatkurtosis_mag_bpStandardized unweighted BP magnitude kurtosisstat.value;phot.mag;em.opt.Bfloatmad_mag_bpMedian Absolute Deviation (MAD) for BP observationsmagstat.value;phot.mag;em.opt.Bfloatabbe_mag_bpAbbe value for BP observationsstat.value;phot.mag;em.opt.Bfloatiqr_mag_bpInterquartile BP magnitude rangemagstat.value;phot.mag;em.opt.Bfloatstetson_mag_bpStetson BP variability indexsrc.var.indexfloatstd_dev_over_rms_err_mag_bpSignal-to-Noise BP estimatestat.snrfloatoutlier_median_bpGreatest absolute deviation from the BP median normalized by the errorstat.fit.paramfloatnum_selected_rpTotal number of RP observations selected for variability analysismeta.numbershortmean_obs_time_rpMean observation time for RP observationsdtime.epoch;stat.meandoubletime_duration_rpTime duration of the RP time seriesdtime.durationfloatmin_mag_rpMinimum RP magnitudemagphot.mag;stat.minfloatmax_mag_rpMaximum RP magnitudemagphot.mag;stat.maxfloatmean_mag_rpMean RP magnitudemagphot.mag;stat.meanfloatmedian_mag_rpMedian RP magnitudemagphot.mag;stat.medianfloatrange_mag_rpDifference between the highest and lowest RP magnitudesmagphot.mag;em.opt.R;arith.difffloattrimmed_range_mag_rpTrimmed difference between the highest and lowest RP magnitudesmagphot.mag;em.opt.R;arith.difffloatstd_dev_mag_rpSquare root of the unweighted RP magnitude variancemagstat.stdev;phot.mag;em.opt.Rfloatskewness_mag_rpStandardized unweighted RP magnitude skewnessstat.value;phot.mag;em.opt.Rfloatkurtosis_mag_rpStandardized unweighted RP magnitude kurtosisstat.value;phot.mag;em.opt.Rfloatmad_mag_rpMedian Absolute Deviation (MAD) for RP observationsmagstat.value;phot.mag;em.opt.Rfloatabbe_mag_rpAbbe value for RP observationsstat.value;phot.mag;em.opt.Rfloatiqr_mag_rpInterquartile RP magnitude rangemagstat.value;phot.mag;em.opt.Rfloatstetson_mag_rpStetson RP variability indexsrc.var.indexfloatstd_dev_over_rms_err_mag_rpSignal-to-Noise RP estimatestat.snrfloatoutlier_median_rpGreatest absolute deviation from the RP median normalized by the errorstat.fit.paramfloatin_vari_classification_resultSource is present in <tt>VariClassifierResult</tt>meta.recordbooleanin_vari_rrlyraeSource is present in <tt>VariRrlyrae</tt>meta.recordbooleanin_vari_cepheidSource is present in <tt>VariCepheid</tt>meta.recordbooleanin_vari_planetary_transitSource is present in <tt>VariPlanetaryTransit</tt>meta.recordbooleanin_vari_short_timescaleSource is present in <tt>VariShortTimescale</tt>meta.recordbooleanin_vari_long_period_variableSource is present in <tt>VariLongPeriodVariable</tt>meta.recordbooleanin_vari_eclipsing_binarySource is present in <tt>VariEclipsingBinary</tt>meta.recordbooleanin_vari_rotation_modulationSource is present in <tt>VariRotationModulation</tt>meta.recordbooleanin_vari_ms_oscillatorSource is present in <tt>VariMsOscillator</tt>meta.recordbooleanin_vari_agnSource is present in <tt>VariAgn</tt>meta.recordbooleanin_vari_microlensingSource is present in <tt>VariMicrolensing</tt>meta.recordbooleanin_vari_compact_companionSource is present in <tt>VariCompactCompanion</tt>meta.recordbooleangaiadr3.commanded_scan_lawThis table provides a representation of the Gaia scanning law over the 34 month time period covered by the Gaia Data Release 3 (from 2014-07-25 10:31:26 to 2017-05-28 08:46:29), including the Ecliptic Pole Scanning at the begin of the mission.jd_timeTime [Julian Date in TCB at Gaia - 2455197.5]dtime.epochdoublebjd_fov1Time [Julian Date in TCB at barycentre for FOV1 - 2455197.5]dtime.epochdoublebjd_fov2Time [Julian Date in TCB at barycentre for FOV2 - 2455197.5]dtime.epochdoubleobmt_timeTime at Gaia (OBMT)nstime.epochlongra_fov1Right Ascension of FOV1 centredegpos.eq.rafloatdec_fov1Declination of FOV1 centredegpos.eq.decfloatheal_pix_fov1FOV1 HEALPix level 12pos.healpixcharscan_angle_fov1Scan position angle of FOV1degpos.angDistancefloatra_fov2Right ascension of FOV2 centredegpos.eq.rafloatdec_fov2Declination of FOV2 centredegpos.eq.decfloatheal_pix_fov2FOV2 HEALPix level 12pos.healpixcharscan_angle_fov2Scan position angle of FOV2degpos.angDistancefloatsolution_idSolution Identifiermeta.versionlonggaiadr3.frame_rotator_sourceSources used to compute the Gaia reference frame.source_idGaia source identifiermeta.id;meta.main;meta.reflongconsidered_for_reference_frame_orientationConsidered for the reference frame orientationmeta.codebooleanused_for_reference_frame_orientationUsed for the reference frame orientationmeta.codebooleanconsidered_for_reference_frame_spinConsidered for the reference frame spinmeta.codebooleanused_for_reference_frame_spinUsed for the reference frame spinmeta.codebooleangaiadr3.alerts_mixedin_sourceidsSome photometric science alerts mix transits from their primary source and other sources in the catalogue.solution_idSolution Identifiermeta.versionlongalert_source_idPrimary sourceId associated to the alertmeta.id;meta.mainlongmixed_in_source_idAdditional sourceId, if any, associated to the alertmeta.id.assoclonggaiadr3.gaia_crf3_xmThis table contains the full cross-match information for the Gaia-CRF3 sources.solution_idSolution Identifiermeta.versionlongsource_idGaia source identifiermeta.id;meta.main;meta.reflongicrf3sxThe flag describing if the Gaia-CRF3 source was found in ICRF3 S/Xmeta.code.statusbooleanicrf3kThe flag describing if the Gaia-CRF3 source was found in ICRF3 Kmeta.code.statusbooleanicrf3xkaThe flag describing if the Gaia-CRF3 source was found in ICRF3 X/Kameta.code.statusbooleanicrf_nameThe ICRF name of the sourcemeta.id.crosschariers_nameThe IERS name of the sourcemeta.id.crosscharocarsThe flag describing if the Gaia-CRF3 source was found in OCARSmeta.code.statusbooleanocars_nameThe name for this source in OCARSmeta.id.crosscharaw15The flag describing if the Gaia-CRF3 source was found in allWISEmeta.code.statusbooleanaw15_nameThe name for this source in allWISEmeta.id.crosscharr90The flag describing if the Gaia-CRF3 source was found in the catalogue R90meta.code.statusbooleanr90_nameThe name for this source in R90meta.id.crosscharm65The flag describing if the Gaia-CRF3 source was found in Milliquas v6.5meta.code.statusbooleanm65_nameThe name for this source in Milliquas v6.5meta.id.crosscharc75The flag describing if the Gaia-CRF3 source was found in the catalogue C75meta.code.statusbooleanc75_nameThe name for this source in C75meta.id.crosschardr14qThe flag describing if the Gaia-CRF3 source was found in the catalogue SDSS DR14Qmeta.code.statusbooleandr14q_nameThe name for this source in SDSS DR14Qmeta.id.crosscharlqac5The flag describing if the Gaia-CRF3 source was found in LQAC-5meta.code.statusbooleanlqac5_nameThe name for this source in LQAC-5meta.id.crosscharlamost5The flag describing if the Gaia-CRF3 source was found in the LAMOST QSO cataloguemeta.code.statusbooleanlamost5_nameThe name for this source in the LAMOST QSO cataloguemeta.id.crosscharlqrfThe flag describing if the Gaia-CRF3 source was found in LQRFmeta.code.statusbooleanlqrf_nameThe name for this source in LQRFmeta.id.crosscharcat2qzThe flag describing if the Gaia-CRF3 source was found in 2QZmeta.code.statusbooleancat2qz_nameThe name for this source in 2QZmeta.id.crosscharbzcat5The flag describing if the Gaia-CRF3 source was found in Roma-BZCAT, v5meta.code.statusbooleanbzcat5_nameThe name for this source in Roma-BZCAT, v5meta.id.crosscharcat2whspjThe flag describing if the Gaia-CRF3 source was found in 2WHSPJmeta.code.statusbooleancat2whspj_nameThe name for this source in 2WHSPJmeta.id.crosscharalma19The flag describing if the Gaia-CRF3 source was found in the ALMA calibrator cataloguemeta.code.statusbooleanalma19_nameThe name for this source in the ALMA calibrator cataloguemeta.id.crosscharguwThe flag describing if the Gaia-CRF3 source was found in Gaia-unWISEmeta.code.statusbooleanguw_nameThe name for this source in Gaia-unWISEmeta.id.crosscharb19The flag describing if the Gaia-CRF3 source was found in the Gaia DR2 quasar and galaxy classification cataloguemeta.code.statusbooleanb19_nameThe name for this source in the Gaia DR2 quasar and galaxy classification cataloguemeta.id.crosschargaiadr3.science_alertsTable containing all Gaia Photometric Science Alerts triggered in the period 25-07-2014 to 28-05-2017.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongtransit_idAlerting transit identifiermeta.idlongnameName of alertmeta.idcharsolution_idSolution Identifiermeta.versionlonggaiadr3.agn_cross_idTable <code>agn_cross_id</code> lists sources whose positions and proper motions define the celestial reference frame of Gaia catalogue.source_name_in_catalogueIdentifier in the external cataloguemeta.id.cross;meta.maincharsource_idGaia source identifiermeta.id;meta.main;meta.reflongcatalogue_nameName of the external cataloguemeta.datasetchargaiadr3.tycho2tdsc_mergeTycho-2 merged with the TDSC catalog and TDSC supplement. The Tycho Double Star Catalogue, (TDSC, ) contains 98482 components of double and multiple systems processed in the Tycho-2 context.idTycho-2 identifiermeta.id;meta.maincharhipHipparcos numbermeta.id.crosschartyc1TYC1 component from TYC or GSCmeta.id.part;meta.mainchartyc2TYC2 component from TYC or GSCmeta.id.part;meta.mainchartyc3TYC3 component from TYC or TDSCmeta.id.part;meta.maincharid_tychoNumeric Tycho-2 identifiermeta.id;meta.datasetlongtycTycho-1 starmeta.codecharraObserved Tycho-2 Right Ascension, ICRSdegpos.eq.radoubledecObserved Tycho-2 Declination, ICRSdegpos.eq.decdoublera_degObserved Tycho-2 Right Ascension, ICRSdegpos.eq.radoublede_degObserved Tycho-2 Declination, ICRSdegpos.eq.decdoublera_mdegMean Right Ascension, ICRS, epoch=J2000degpos.eq.radoublede_mdegMean Declination, ICRS, at epoch=J2000degpos.eq.decdoublepm_raProper motion in RA*cos(dec)mas.yr**-1pos.eq.ra;pos.pmfloatpm_deProper motion in Decmas.yr**-1pos.eq.dec;pos.pmfloatep_ra1990Epoch--1990 of raDegyrtime.epochfloatep_de1990Epoch--1990 of deDegyrtime.epochfloatep_ra_mMean epoch of RA.yrtime.epochfloatep_de_mMean epoch of Dec.yrtime.epochfloatnumNumber of positions used for forming mean datameta.numbershorte_ra_degUncertainty RA*cos(dec), of observed Tycho-2 RA.masstat.errordoublee_de_degUncertainty of observed Tycho-2 Dec.masstat.errordoublecorrCorrelation (RAdeg,DEdeg)stat.correlation;pos.eq.ra;pos.eq.decdoublee_ra_mdegUncertainty RA*cos(dec),at mean epoch.masstat.errordoublee_de_mdegUncertainty of Dec at mean epoch.masstat.errordoublee_pm_raUncertainty proper motion in RA*cos(dec).mas.yr**-1stat.errorfloate_pm_deUncertainty of proper motion in Dec.mas.yr**-1stat.errorfloatq_ra_mdegGoodness of fit for mean RAmeta.code.qualfloatq_de_mdegGoodness of fit for mean Decmeta.code.qualfloatq_pm_deGoodness of fit for pmDemeta.code.qualfloatq_pm_raGoodness of fit for pmRameta.code.qualfloatpflagMean position flagmeta.codecharposflgType of Tycho-2 solutionmeta.id;stat.fitcharccdmCCDM component identifier for HIP starsmeta.code.multipcharproxProximity indicator100masmeta.codeshortbt_magTycho-2 BT magnitudemagphot.mag;em.opt.Bfloatvt_magTycho-2 VT magnitudemagphot.mag;em.opt.Vfloate_bt_magUncertainty of BTmagstat.errorfloate_vt_magUncertainty of VTmagstat.errorfloatsys_noTDSC identifier for the systemmeta.idcharcmpComponent designationmeta.id.partcharn_mainNumber of components in TDSC main cataloguemeta.numbershortn_supNumber of components in the TDSC supplementmeta.numbershortmagflgTDSC photometry flagmeta.codecharwdsWDS identifier for the systemmeta.id.crosscharnoteTDSC notesmeta.notecharhdHD identifier for TDSC entriesmeta.id.crosscharrcmpReference component for position angle and separationmeta.id.assoccharpaPosition angledegpos.posAngfloatsepSeparationarcsecpos.angDistancefloate_paUncertainty of the position angledegstat.errorfloate_pa_sepUncertainty of the position angle * separationstat.errorshorte_sepUncertainty of the separationmasstat.errorshortgaiadr3.hipparcos2_best_neighbourTable <code>hipparcos2_best_neighbour</code> lists each matched external catalogue object with its best neighbour in Gaia.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.hipparcos2_neighbourhoodTable <code>hipparcos2_neighbourhood</code> includes all good neighbours for each matched Hipparcos2 object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.tycho2tdsc_merge_best_neighbourTable <code>tycho2tdsc_merge_best_neighbour</code> lists each matched external catalogue object with its best neighbour in Gaia.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshorttycho2tdsc_merge_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortgaiadr3.tycho2tdsc_merge_neighbourhoodTable <code>tycho2tdsc_merge_neighbourhood</code> includes all good neighbours for each matched Tycho2tdscMerge object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshorttycho2tdsc_merge_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.panstarrs1_best_neighbourTable <code>panstarrs1_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.panstarrs1_neighbourhoodTable <code>panstarrs1_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.panstarrs1_joinConvenience table to be used to join Pan-STARRS1 DR1.1 catalogue with the cross-match results. The table links the external catalogue original <code>source_id</code> (<code>original_ext_source_id</code>) to the corresponding additional numerical identifier (<code>clean_panstarrs1_oid</code>).original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslonggaiadr3.sdssdr13_best_neighbourTable <code>sdssdr13_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crosscharoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.sdssdr13_neighbourhoodTable <code>sdssdr13_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crosscharoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.sdssdr13_joinConvenience table to be used to join SDSS DR13 catalogue with the cross-match results. The table links the external catalogue original <code>source_id</code> (<code>original_ext_source_id</code>) to the corresponding additional numerical identifier (<code>clean_sdssdr13_oid</code>).original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.skymapperdr2_best_neighbourTable <code>skymapperdr2_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.skymapperdr2_neighbourhoodTable <code>skymapperdr2_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiadr3.skymapperdr2_joinConvenience table to be used to join the SkyMapper DR2 catalogue with the cross-match results. It lists all the SkyMapper DR2 sources which were used in the cross-match. See Chapter [chap:crossmatch] for more details on the catalogue.original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslonggaiadr3.urat1_best_neighbourTable <code>urat1_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshorturat1_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiadr3.urat1_neighbourhoodTable <code>urat1_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshorturat1_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.allwise_best_neighbourTable <code>allwise_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortallwise_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiadr3.allwise_neighbourhoodTable <code>allwise_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortallwise_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.apassdr9_best_neighbourTable <code>apassdr9_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancedoublenumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbercharnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statuschargaiadr3.apassdr9_neighbourhoodTable <code>apassdr9_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancedoublescoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statuschargaiadr3.apassdr9_joinConvenience table to be used to join the APASS DR9 catalogue with the cross-match results. The table links the external catalogue original <code>source_id</code> (<code>original_ex_source_id</code>) to the corresponding additional numerical identifier (<code>clean_apassdr9_oid</code>).original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.gsc23_best_neighbourTable <code>gsc23_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_gsc23_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiadr3.gsc23_neighbourhoodTable <code>gsc23_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_gsc23_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.gsc23_joinConvenience table to be used to join the GSC 2.3 catalogue with cross-match results. The table links the external catalogue original sourceId (originalExtSourceId) to the corresponding additional numerical identifier (cleanGsc23Oid).original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharclean_gsc23_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.ravedr5_best_neighbourTable <code>ravedr5_best_neighbour</code> lists each matched external catalogue object with its best neighbour in Gaia.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortgaiadr3.ravedr5_neighbourhoodTable <code>ravedr5_neighbourhood</code> includes all good neighbours for each matched RAVE DR5 object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.ravedr5_joinConvenience table to be used to join RAVE DR5 catalogue with the cross-match results. The table links the external catalogue original sourceId (originalExtSourceId) to the corresponding additional numerical identifier (cleanRavedr5Oid).original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.tmass_psc_xsc_best_neighbourTable <code>tmass_psc_xsc_best_neighbour</code> lists each matched Gaia object with its best neighbour in the external catalogue.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crosscharnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiadr3.tmass_psc_xsc_neighbourhoodTable <code>tmass_psc_xsc_neighbourhood</code> includes all good neighbours for each matched Gaia object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.tmass_psc_xsc_joinConvenience table to be used to join 2MASS PSC+XSC catalogue with the cross-match results. The table links the external catalogue original sourceId (originalExtSourceId) to the corresponding additional numerical identifier (cleanTmassPscXscOid).original_psc_source_idOriginal 2MASS PSC source identifiermeta.id.crosscharoriginal_xsc_source_idOriginal 2MASS XSC source identifiermeta.id.crosscharclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crosschargaiadr3.ravedr6_best_neighbourTable <tt>Ravedr6BestNeighbour</tt> lists each matched external catalogue object with its best neighbour in Gaia.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortravedr6_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortgaiadr3.ravedr6_neighbourhoodTable <tt>Ravedr6Neighbourhood</tt> includes all good neighbours for each matched RAVE DR6 object.source_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortravedr6_oidExternal Catalogue source identifiermeta.id.crossintgaiadr3.ravedr6_joinConvenience table to be used to join RAVE DR6 catalogue with the cross-match results.original_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharravedr6_oidExternal Catalogue source identifiermeta.id.crossintgaiadr3.gaia_source_simulationTable of sources realised according to the Gaia Object Generator (GOG) simulation.solution_idSolution Identifiermeta.versionlongsource_idLong Identifiermeta.id;meta.main;meta.reflongraRight Ascensiondegpos.eq.radoublera_errorRight Ascension errormasstat.errorfloatdecDeclinationdegpos.eq.dec;pos.eq.radoubledec_errorDeclination errormasstat.errorfloatparallaxParallaxmaspos.parallaxfloatparallax_errorParallax errormasstat.errorfloatpmraProper motion in RAmas.yr**-1pos.pm;pos.eq.rafloatpmra_errorError in RA proper motionmas.yr**-1stat.errorfloatpmdecProper motion in decmas.yr**-1pos.pm;pos.eq.decfloatpmdec_errorError in dec. proper motionmas.yr**-1stat.errorfloatn_obs_alNumber of AL observationsmeta.numbercharn_outliers_alNumber of outliers AL observationsmeta.numbercharphot_g_mean_fluxMean G flux"electron".s**-1phot.flux;em.optfloatphot_g_mean_flux_errorMean G flux error"electron".s**-1stat.error;phot.flux;em.optfloatphot_g_mean_magMean G magnitudemagphot.mag;em.optfloatphot_bp_mean_fluxMean BP flux"electron".s**-1phot.flux;em.opt.Bfloatphot_bp_mean_flux_errorMean BP flux error"electron".s**-1stat.error;phot.flux;em.opt.Bfloatphot_bp_mean_magMean BP magnitudemagphot.mag;em.opt.Bfloatphot_rp_mean_fluxMean RP flux"electron".s**-1phot.flux;em.opt.Rfloatphot_rp_mean_flux_errorMean RP flux error"electron".s**-1stat.error;phot.flux;em.opt.Rfloatphot_rp_mean_magMean RP magnitudemagphot.mag;em.opt.Rfloatphot_rvs_mean_fluxMean RVS flux"electron".s**-1phot.flux;em.opt.Ifloatphot_rvs_mean_flux_errorMean RVS flux error"electron".s**-1stat.error;phot.flux;em.opt.Ifloatphot_rvs_mean_magMean RVS magnitudemagphot.mag;em.opt.Ifloatradial_velocityRadial velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatradial_velocity_errorRadial velocity errorkm.s**-1stat.errorfloatteffEffective temperatureKphys.temperature.effectivefloatteff_errorEffective temperature errorKstat.error;phys.temperature.effectivefloatvsiniv sin ikm.s**-1phys.veloc.rotatfloatvsini_errorv sin i errorkm.s**-1stat.error;phys.veloc.rotatfloata0Extinction at 550 nmmagphys.absorption;em.opt.Vfloata0_errorExtinction at 550 nm errormagstat.error;phys.absorption;em.opt.VfloatfehIron abundance"dex"phys.abund.Fefloatfeh_errorIron abundance error"dex"stat.error;phys.abund.FefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogg_errorSurface gravity Errorlog(cm.s**-2)stat.error;phys.gravityfloatgaiadr3.gaia_universe_modelTable of simulated galactic stars according to the Gaia Universal Model Simulation (GUMS).source_extended_idExtended source identifiermeta.numbercharsource_idLong Identifiermeta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongraRight Ascensiondegpos.eq.radoubledecDeclinationdegpos.eq.decdoublebarycentric_distanceBarycentric distance to the simulated sourcepcpos.distancefloatpmraProper motion along right ascensionmas.yr**-1pos.pm;pos.eq.rafloatpmdecProper motion along declinationmas.yr**-1pos.pm;pos.eq.decfloatradial_velocityRadial Velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatmag_gMean Apparent G magnitudemagphot.mag;em.optfloatmag_bpMean Apparent BP magnitudemagphot.mag;em.opt.Bfloatmag_rpMean Apparent RP magnitudemagphot.mag;em.opt.Rfloatmag_rvsMean Apparent RVS magnitudemagphot.mag;em.opt.Ifloatv_i(V-I) colormagphot.color;em.opt.V;em.opt.Ifloatmean_absolute_vMean Absolute V magnitudemagphot.mag;em.opt.VfloatagAbsorption in Gmagphys.absorption;em.optfloatavAbsorption in Vmagphys.absorption;em.opt.VfloatteffEffective temperatureKphys.temperature.effectivefloatspectral_typespectral class + luminosity classsrc.spTypecharloggSurface gravitylog(cm.s**-2)phys.gravityfloatfehMetallicity"dex"phys.abund.FefloatalphafeAlpha elements"dex"phys.abundfloatmbolAbsolute bolometric magnitudemagphot.mag.bolfloatageAgeGyrtime.agefloatmassMasssolMassphys.massfloatradiusRadiussolRadphys.size.radiusfloatvsiniRotational velocitykm.s**-1phys.veloc.rotatfloatpopulationPopulationmeta.code.membercharhas_photocenter_motionBoolean describing if the photocenter has or not motionmeta.code.statusbooleanncNumber of componentsmeta.numbercharntTotal number of objectmeta.numbercharsemimajor_axisSemi major axisAUsrc.orbitalfloateccentricityEccentricitysrc.orbital.eccentricityfloatinclinationInclinationdegsrc.orbital.inclinationfloatlongitude_ascending_nodeLongitude of ascending nodedegpos.bodyrc.lonfloatorbit_periodPeriod of the orbitdsrc.orbitalfloatperiastron_dateDate of periastrondsrc.orbital.periastronfloatperiastron_argumentPeriastron argumentdegsrc.orbital.periastronfloatvariability_typeVariability typesrc.varcharvariability_amplitudeAmplitude of variabilitymagsrc.var;src.var.amplitude;em.optfloatvariability_periodPeriod of variabilitydsrc.var;time.periodfloatvariability_phasePhase of variabilitysrc.var;time.phasefloatr_env_r_starEnvelope characterisic for Be starsmetafloatgaiadr3_contribContributions using Gaia DR3 catalog tablesgaiadr3_contrib.estimates_gdr3_rvBayesian Estimates for Gaia DR3 Radial Velocitiessource_idUnique source identifier (unique within a particular Data Release)meta.idlongsample_meanMean of radial velocity posteriorkm.s**-1stat.mean;spect.dopplerVelocfloatsample_stdStandard deviation of radial velocity posteriorkm.s**-1stat.stdev;spect.dopplerVelocfloatq0505th percentile of radial velocity posteriorkm.s**-1stat.value;spect.dopplerVelocfloatq15915.9th percentile velocities for each starkm.s**-1stat.value;spect.dopplerVelocfloatq50050th percentile velocities for each starkm.s**-1stat.value;spect.dopplerVelocfloatq84184.1th percentile velocities for each starkm.s**-1stat.value;spect.dopplerVelocfloatq95095.5th percentile velocities for each starkm.s**-1stat.value;spect.dopplerVelocfloatw_0Weight of Gaussian component 0. (w0+w1+w2+w3) = 1.0stat.weightfloatw_1Weight of Gaussian component 1. (w0+w1+w2+w3) = 1.0stat.weightfloatw_2Weight of Gaussian component 2. (w0+w1+w2+w3) = 1.0stat.weightfloatw_3Weight of Gaussian component 2. (w0+w1+w2+w3) = 1.0stat.weightfloatmu_0Mean of Gaussian component 0.km.s**-1stat.mean;spect.dopplerVelocfloatmu_1Mean of Gaussian component 1.km.s**-1stat.mean;spect.dopplerVelocfloatmu_2Mean of Gaussian component 2.km.s**-1stat.mean;spect.dopplerVelocfloatmu_3Mean of Gaussian component 3.km**2.s**-2stat.mean;spect.dopplerVelocfloatvar_0Variance of Gaussian component 0.km**2.s**-2stat.variancefloatvar_1Variance of Gaussian component 1.km**2.s**-2stat.variancefloatvar_2Variance of Gaussian component 2.km**2.s**-2stat.variancefloatvar_3Variance of Gaussian component 3.km**2.s**-2stat.variancefloatgaiadr3_contrib.cnn_gaia_rvs_catalogThe table contains atmospheric parameters (Teff, log(g), [M/H]), chemical abundances ([Fe/H], [alpha/M]), and their associated uncertainties for 886080 stars. We also provide a boundary_flag that should be used to filter the stars outside of the training sample limits. We recommend using flag_boundary = '00000000' for science applications.source_idGaia Source IDmeta.id;meta.main;meta.reflongteffEffective temperatureKphys.temperature.effectivedoubleeteffModel-to-model despersion of <tt>teff</tt>Kstat.value;phys.temperature.effectivedoublesigma_teffOverall dispersion of <tt>teff</tt>Kstat.value;phys.temperature.effectivedoubleloggSurface gravitylog(cm.s**-2)phys.gravitydoubleeloggModel-to-model dispersion of <tt>logg</tt>log(cm.s**-2)stat.value;phys.gravitydoublesigma_loggOverall dispersion of <tt>logg</tt>log(cm.s**-2)stat.value;phys.gravitydoublemhOverall metallicity"dex"phys.abunddoubleemhModel-to-model despersion of [M/H]"dex"stat.value;phys.abunddoublesigma_mhOverall dispersion of [M/H]"dex"stat.phys;phys.abunddoublefeh[Fe/H] ratio"dex"phys.abund.FedoubleefehModel-to-model dispersion of [Fe/H]"dex"stat.value;phys.abund.Fedoublesigma_fehOverall dispersion of [Fe/H]"dex"stat.value;phys.abund.Fedoublealpham[alpha/M] ratio"dex"phys.abunddoubleealphamModel-to-model dispersion of [alpha/M]"dex"stat.value;phys.abunddoublesigma_alphamOverall dispersion of [alpha/M]"dex"stat.value;phys.abunddoubleflag_boundaryBoundary flag composed of 8 digitschargaiadr3_contrib.shboost2024SHBoost, catalogue of stellar properties derived from Gaia DR3 XP spectra, astrometry, and multi-wavelength photometry.source_idGaia DR3 unique source identifiermeta.id;meta.main;meta.reflongrandom_indexRandom index for use when selecting subsetsmeta.codelongxgb_avline-of-sight extinction at λ = 5420 Å, AV, xgboost point estimatemagphys.absorption.galfloatxgbdist_av_meanline-of-sight extinction at λ = 5420 Å, AV, xgboost-distribution mean valuemagphys.absorption.gal;stat.meanfloatxgbdist_av_stdline-of-sight extinction at λ = 5420 Å, AV, xgboost-distribution standard deviationmagphys.absorption.gal;stat.stdevfloatxgb_logteffeffective temperature, xgboost point estimateKphys.temperature.effectivefloatxgbdist_logteff_meaneffective temperature, xgboost-distribution mean valueKphys.temperature.effective;stat.meanfloatxgbdist_logteff_stdeffective temperature, xgboost-distribution standard deviationKphys.temperature.effective;stat.stdevfloatxgb_loggsurface gravity, xgboost point estimatecgsphys.gravityfloatxgbdist_logg_meansurface gravity, xgboost-distribution mean valuecgsphys.gravity;stat.meanfloatxgbdist_logg_stdsurface gravity, xgboost-distribution standard deviationcgsphys.gravity;stat.stdevfloatxgb_metmetallicity, xgboost point estimatephys.abund.Zfloatxgbdist_met_meanmetallicity, xgboost-distribution mean valuephys.abund.Z;stat.meanfloatxgbdist_met_stdmetallicity, xgboost-distribution standard deviationphys.abund.Z;stat.stdevfloatxgb_massstellar mass, xgboost point estimatesolMassphys.massfloatxgbdist_mass_meanstellar mass, xgboost-distribution mean valuesolMassphys.mass;stat.meanfloatxgbdist_mass_stdstellar mass, xgboost-distribution standard deviationsolMassphys.mass;stat.stdevfloatdistDistance estimate from the literaturekpcpos.distancefloatdist_lower16th distance percentile from the literaturekpcpos.distancefloatdist_upper84th distance percentile from the literaturekpcpos.distancefloatdist_flagDistance flag (0=StarHorse EDR3, 1=Bailer-Jones et al. 2021 photogeo, =2 BJ2021 geo)meta.codeintbprp0dereddened colour, derived with gaia_edr3_photutilsmagphot.color.reddFreefloatmg0absolute magnitude, derived with gaia_edr3_photutilsmagphys.magAbsfloatxgGalactocentric Cartesian X coordinate, derived from dist and assuming X0 = −8.2 kpckpcpos.cartesian.xfloatygGalactocentric Cartesian Y coordinate, derived from dist and assuming X0 = −8.2 kpckpcpos.cartesian.yfloatzgGalactocentric Cartesian Z coordinate, derived from dist and assuming Z0 = 0kpcpos.cartesian.zfloatrgGalactocentric planar distance, derived from XGal and YGalkpcpos.distancefloatvxgGalactic Cartesian velocity in X directionkm/sphys.velocfloatvygGalactic Cartesian velocity in Y directionkm/sphys.velocfloatvzgGalactic Cartesian velocity in Z directionkm/sphys.velocfloatvrgGalactic radial velocitykm/sphys.velocfloatvphigGalactic angular velocitykm/sphys.velocfloatxgb_inputflagSHBoost input flagmeta.codecharxgb_av_outputflagAV output quality flag (=0 if xgbdist_av_std < 0.3)meta.codecharxgb_logteff_outputflaglog Teff output quality flag (=0 if xgbdist_logteff_std < 0.1)meta.codecharxgb_logg_outputflaglog g output quality flag (=0 if xgbdist_logg_std < 0.3)meta.codecharxgb_met_outputflag[M/H] output quality flag (=0 if xgbdist_met_std < 0.3)meta.codecharxgb_mass_outputflagMass output quality flag (=0 if xgbdist_mass_std / xgbdist_mass_mean < 0.3)meta.codechargaiaedr3Gaia Early Data Release 3gaiaedr3.gaia_sourcesolution_idSolution Identifiermeta.versionlongdesignationUnique source designation (unique across all Data Releases)meta.id;meta.maincharsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongrandom_indexRandom index used to select subsetsmeta.codelongref_epochReference epochyrmeta.ref;time.epochdoubleraRight ascensiondegpos.eq.ra;meta.maindoublera_errorStandard error of right ascensionmasstat.error;pos.eq.rafloatdecDeclinationdegpos.eq.dec;meta.maindoubledec_errorStandard error of declinationmasstat.error;pos.eq.decfloatparallaxParallaxmaspos.parallax.trigdoubleparallax_errorStandard error of parallaxmasstat.error;pos.parallax.trigfloatparallax_over_errorParallax divided by its standard errorstat.snr;pos.parallax.trigfloatpmTotal proper motionmas.yr**-1pos.pm;pos.eqfloatpmraProper motion in right ascension directionmas.yr**-1pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionmas.yr**-1stat.error;pos.pm;pos.eq.rafloatpmdecProper motion in declination directionmas.yr**-1pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionmas.yr**-1stat.error;pos.pm;pos.eq.decfloatra_dec_corrCorrelation between right ascension and declinationstat.correlationfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatastrometric_n_obs_alTotal number of observations ALmeta.numbershortastrometric_n_obs_acTotal number of observations ACmeta.numbershortastrometric_n_good_obs_alNumber of good observations ALmeta.numbershortastrometric_n_bad_obs_alNumber of bad observations ALmeta.numbershortastrometric_gof_alGoodness of fit statistic of model wrt along-scan observationsstat.fit.goodnessfloatastrometric_chi2_alAL chi-square valuestat.fit.chi2floatastrometric_excess_noiseExcess noise of the sourcemasstat.valuefloatastrometric_excess_noise_sigSignificance of excess noisestat.valuefloatastrometric_params_solvedWhich parameters have been solved for?meta.numbershortastrometric_primary_flagPrimary or secondaymeta.codebooleannu_eff_used_in_astrometryEffective wavenumber of the source used in the astrometric solutionum**-1em.wavenumberfloatpseudocolourAstrometrically estimated pseudocolour of the sourceum**-1em.wavenumberfloatpseudocolour_errorStandard error of the pseudocolour of the sourceum**-1stat.error;em.wavenumberfloatra_pseudocolour_corrCorrelation between right ascension and pseudocolourstat.correlation;em.wavenumber;pos.eq.rafloatdec_pseudocolour_corrCorrelation between declination and pseudocolourstat.correlation;em.wavenumber;pos.eq.decfloatparallax_pseudocolour_corrCorrelation between parallax and pseudocolourstat.correlation;em.wavenumber;pos.parallaxfloatpmra_pseudocolour_corrCorrelation between proper motion in right asension and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.rafloatpmdec_pseudocolour_corrCorrelation between proper motion in declination and pseudocolourstat.correlation;em.wavenumber;pos.pm;pos.eq.decfloatastrometric_matched_transitsMatched FOV transits used in the AGIS solutionmeta.numbershortvisibility_periods_usedNumber of visibility periods used in Astrometric solutionmeta.numbershortastrometric_sigma5d_maxThe longest semi-major axis of the 5-d error ellipsoidmasstat;pos.errorEllipsefloatmatched_transitsThe number of transits matched to this sourcemeta.numbershortnew_matched_transitsThe number of transits newly incorporated into an existing source in the current cyclemeta.numbershortmatched_transits_removedThe number of transits removed from an existing source in the current cyclemeta.numbershortipd_gof_harmonic_amplitudeAmplitude of the IPD GoF versus position angle of scanstat.valuefloatipd_gof_harmonic_phasePhase of the IPD GoF versus position angle of scandegpos.posAng;stat.valuefloatipd_frac_multi_peakPercent of successful-IPD windows with more than one peakstat.valueshortipd_frac_odd_winPercent of transits with truncated windows or multiple gatestat.valueshortruweRenormalised unit weight errorstat.errorfloatscan_direction_strength_k1Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k2Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k3Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_strength_k4Degree of concentration of scan directions across the sourcestat.valuefloatscan_direction_mean_k1Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k2Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k3Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatscan_direction_mean_k4Mean position angle of scan directions across the sourcedegpos.posAng;stat.meanfloatduplicated_sourceSource with multiple source identifiersmeta.code.statusbooleanphot_g_n_obsNumber of observations contributing to G photometrymeta.numbershortphot_g_mean_fluxG-band mean flux"electron".s**-1phot.flux;em.optdoublephot_g_mean_flux_errorError on G-band mean flux"electron".s**-1stat.error;phot.flux;em.optfloatphot_g_mean_flux_over_errorG-band mean flux divided by its errorstat.snr;phot.flux;em.optfloatphot_g_mean_magG-band mean magnitudemagphot.mag;em.optfloatphot_bp_n_obsNumber of observations contributing to BP photometrymeta.numbershortphot_bp_mean_fluxIntegrated BP mean flux"electron".s**-1phot.flux;em.opt.Bdoublephot_bp_mean_flux_errorError on the integrated BP mean flux"electron".s**-1stat.error;phot.flux;em.opt.Bfloatphot_bp_mean_flux_over_errorIntegrated BP mean flux divided by its errorstat.snr;phot.flux;em.opt.Bfloatphot_bp_mean_magIntegrated BP mean magnitudemagphot.mag;em.opt.Bfloatphot_rp_n_obsNumber of observations contributing to RP photometrymeta.numbershortphot_rp_mean_fluxIntegrated RP mean flux"electron".s**-1phot.flux;em.opt.Rdoublephot_rp_mean_flux_errorError on the integrated RP mean flux"electron".s**-1stat.error;phot.flux;em.opt.Rfloatphot_rp_mean_flux_over_errorIntegrated RP mean flux divided by its errorstat.snr;phot.flux;em.opt.Rfloatphot_rp_mean_magIntegrated RP mean magnitudemagphot.mag;em.opt.Rfloatphot_bp_n_contaminated_transitsNumber of BP contaminated transitsmeta.numbershortphot_bp_n_blended_transitsNumber of BP blended transitsmeta.numbershortphot_rp_n_contaminated_transitsNumber of RP contaminated transitsmeta.numbershortphot_rp_n_blended_transitsNumber of RP blended transitsmeta.numbershortphot_proc_modePhotometry processing modemeta.codeshortphot_bp_rp_excess_factorBP/RP excess factorarith.factor;phot.flux;em.optfloatbp_rpBP - RP colourmagphot.color;em.opt.B;em.opt.Rfloatbp_gBP - G colourmagphot.color;em.opt.B;em.optfloatg_rpG - RP colourmagphot.color;em.opt;em.opt.Rfloatdr2_radial_velocityRadial velocity from Gaia DR2km.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatdr2_radial_velocity_errorRadial velocity error from Gaia DR2km.s**-1stat.error;spect.dopplerVeloc.opt;em.opt.Ifloatdr2_rv_nb_transitsNumber of transits used to compute radial velocity in Gaia DR2meta.numbershortdr2_rv_template_teffTeff of the template used to compute radial velocity in Gaia DR2Kstat.fit.paramfloatdr2_rv_template_logglogg of the template used to compute radial velocity in Gaia DR2log(cm.s**-2)stat.fit.paramfloatdr2_rv_template_fe_hFe/H of the template used to compute radial velocity in Gaia DR2"dex"stat.fit.paramfloatlGalactic longitudedegpos.galactic.londoublebGalactic latitudedegpos.galactic.latdoubleecl_lonEcliptic longitudedegpos.ecliptic.londoubleecl_latEcliptic latitudedegpos.ecliptic.latdoubleposchargaiaedr3.gaia_source_simulationsolution_idSolution Identifiermeta.versionlongsource_idLong Identifiermeta.id;meta.main;meta.reflongraRight Ascensiondegpos.eq.radoublera_errorRight Ascension errormasstat.errorfloatdecDeclinationdegpos.eq.dec;pos.eq.radoubledec_errorDeclination errormasstat.errorfloatparallaxParallaxmaspos.parallaxfloatparallax_errorParallax errormasstat.errorfloatpmraProper motion in RAmas.yr**-1pos.pm;pos.eq.rafloatpmra_errorError in RA proper motionmas.yr**-1stat.errorfloatpmdecProper motion in decmas.yr**-1pos.pm;pos.eq.decfloatpmdec_errorError in dec. proper motionmas.yr**-1stat.errorfloatn_obs_alNumber of AL observationsmeta.numberintn_outliers_alNumber of outliers AL observationsmeta.numberintphot_g_mean_fluxMean G flux"electron".s**-1phot.flux;em.optfloatphot_g_mean_flux_errorMean G flux error"electron".s**-1stat.error;phot.flux;em.optfloatphot_g_mean_magMean G magnitudemagphot.mag;em.optfloatphot_bp_mean_fluxMean BP flux"electron".s**-1phot.flux;em.opt.Bfloatphot_bp_mean_flux_errorMean BP flux error"electron".s**-1stat.error;phot.flux;em.opt.Bfloatphot_bp_mean_magMean BP magnitudemagphot.mag;em.opt.Bfloatphot_rp_mean_fluxMean RP flux"electron".s**-1phot.flux;em.opt.Rfloatphot_rp_mean_flux_errorMean RP flux error"electron".s**-1stat.error;phot.flux;em.opt.Rfloatphot_rp_mean_magMean RP magnitudemagphot.mag;em.opt.Rfloatphot_rvs_mean_fluxMean RVS flux"electron".s**-1phot.flux;em.opt.Ifloatphot_rvs_mean_flux_errorMean RVS flux error"electron".s**-1stat.error;phot.flux;em.opt.Ifloatphot_rvs_mean_magMean RVS magnitudemagphot.mag;em.opt.Ifloatradial_velocityRadial velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatradial_velocity_errorRadial velocity errorkm.s**-1stat.errorfloatteffEffective temperatureKphys.temperature.effectivefloatteff_errorEffective temperature errorKstat.error;phys.temperature.effectivefloatvsiniv sin ikm.s**-1phys.veloc.rotatfloatvsini_errorv sin i errorkm.s**-1stat.error;phys.veloc.rotatfloata0Extinction at 550 nmmagphys.absorption;em.opt.Vfloata0_errorExtinction at 550 nm errormagstat.error;phys.absorption;em.opt.VfloatfehIron abundance"dex"phys.abund.Fefloatfeh_errorIron abundance error"dex"stat.error;phys.abund.FefloatloggSurface gravitylog(cm.s**-2)phys.gravityfloatlogg_errorSurface gravity Errorlog(cm.s**-2)stat.error;phys.gravityfloatgaiaedr3.gaia_universe_modelsource_extended_idExtended source identifiermeta.numbercharsource_idLong Identifiermeta.id;meta.main;meta.reflongsolution_idSolution Identifiermeta.versionlongraRight Ascensiondegpos.eq.radoubledecDeclinationdegpos.eq.decdoublebarycentric_distanceBarycentric distance to the simulated sourcepcpos.distancefloatpmraProper motion along right ascensionmas.yr**-1pos.pm;pos.eq.rafloatpmdecProper motion along declinationmas.yr**-1pos.pm;pos.eq.decfloatradial_velocityRadial Velocitykm.s**-1spect.dopplerVeloc.opt;em.opt.Ifloatmag_gMean Apparent G magnitudemagphot.mag;em.optfloatmag_bpMean Apparent BP magnitudemagphot.mag;em.opt.Bfloatmag_rpMean Apparent RP magnitudemagphot.mag;em.opt.Rfloatmag_rvsMean Apparent RVS magnitudemagphot.mag;em.opt.Ifloatv_i(V-I) colormagphot.color;em.opt.V;em.opt.Ifloatmean_absolute_vMean Absolute V magnitudemagphot.mag;em.opt.VfloatagAbsorption in Gmagphys.absorption;em.optfloatavAbsorption in Vmagphys.absorption;em.opt.VfloatteffEffective temperatureKphys.temperature.effectivefloatspectral_typespectral class + luminosity classsrc.spTypecharloggSurface gravitylog(cm.s**-2)phys.gravityfloatfehMetallicity"dex"phys.abund.FefloatalphafeAlpha elements"dex"phys.abundfloatmbolAbsolute bolometric magnitudemagphot.mag.bolfloatageAgeGyrtime.agefloatmassMasssolMassphys.massfloatradiusRadiussolRadphys.size.radiusfloatvsiniRotational velocitykm.s**-1phys.veloc.rotatfloatpopulationPopulationmeta.code.memberinthas_photocenter_motionBoolean describing if the photocenter has or not motionmeta.code.statusbooleanncNumber of componentsmeta.numberintntTotal number of objectmeta.numberintsemimajor_axisSemi major axisAUsrc.orbitalfloateccentricityEccentricitysrc.orbital.eccentricityfloatinclinationInclinationdegsrc.orbital.inclinationfloatlongitude_ascending_nodeLongitude of ascending nodedegpos.bodyrc.lonfloatorbit_periodPeriod of the orbitdsrc.orbitalfloatperiastron_dateDate of periastrondsrc.orbital.periastronfloatperiastron_argumentPeriastron argumentdegsrc.orbital.periastronfloatvariability_typeVariability typesrc.varcharvariability_amplitudeAmplitude of variabilitymagsrc.var;src.var.amplitude;em.optfloatvariability_periodPeriod of variabilitydsrc.var;time.periodfloatvariability_phasePhase of variabilitysrc.var;time.phasefloatr_env_r_starEnvelope characterisic for Be starsmetafloatgaiaedr3.dr2_neighbourhooddr2_source_idSource identifier in Gaia DR2meta.id.crosslongdr3_source_idSource identifier in Gaia E/DR3meta.id.cross;meta.mainlongangular_distanceAngular distance between the two sourcesmaspos.angDistancefloatmagnitude_differenceG band magnitude difference between the sourcesmagphot.mag;arith.difffloatproper_motion_propagationFlag indicating whether E/DR3 coordinates were proper motion correctedmeta.code.statusbooleangaiaedr3.agn_cross_idsource_name_in_catalogueIdentifier in the external cataloguemeta.id.cross;meta.maincharsource_idGaia source identifiermeta.id;meta.main;meta.reflongcatalogue_nameName of the external cataloguemeta.datasetchargaiaedr3.tycho2tdsc_mergeidTycho-2 identifiermeta.id;meta.maincharhipHipparcos numbermeta.id.crossinttyc1TYC1 component from TYC or GSCmeta.id.part;meta.mainchartyc2TYC2 component from TYC or GSCmeta.id.part;meta.mainchartyc3TYC3 component from TYC or TDSCmeta.id.part;meta.maincharid_tychoNumeric Tycho-2 identifiermeta.id;meta.datasetlongtycTycho-1 starmeta.codecharraObserved Tycho-2 Right Ascension, ICRSdegpos.eq.radoubledecObserved Tycho-2 Declination, ICRSdegpos.eq.decdoublera_degObserved Tycho-2 Right Ascension, ICRSdegpos.eq.radoublede_degObserved Tycho-2 Declination, ICRSdegpos.eq.decdoublera_mdegMean Right Ascension, ICRS, epoch=J2000degpos.eq.radoublede_mdegMean Declination, ICRS, at epoch=J2000degpos.eq.decdoublepm_raProper motion in RA*cos(dec)mas.yr**-1pos.eq.ra;pos.pmfloatpm_deProper motion in Decmas.yr**-1pos.eq.dec;pos.pmfloatep_ra1990Epoch--1990 of raDegyrtime.epochfloatep_de1990Epoch--1990 of deDegyrtime.epochfloatep_ra_mMean epoch of RA.yrtime.epochfloatep_de_mMean epoch of Dec.yrtime.epochfloatnumNumber of positions used for forming mean datameta.numbershorte_ra_degUncertainty RA*cos(dec), of observed Tycho-2 RA.masstat.errordoublee_de_degUncertainty of observed Tycho-2 Dec.masstat.errordoublecorrCorrelation (RAdeg,DEdeg)stat.correlation;pos.eq.ra;pos.eq.decdoublee_ra_mdegUncertainty RA*cos(dec),at mean epoch.masstat.errordoublee_de_mdegUncertainty of Dec at mean epoch.masstat.errordoublee_pm_raUncertainty proper motion in RA*cos(dec).mas.yr**-1stat.errorfloate_pm_deUncertainty of proper motion in Dec.mas.yr**-1stat.errorfloatq_ra_mdegGoodness of fit for mean RAmeta.code.qualfloatq_de_mdegGoodness of fit for mean Decmeta.code.qualfloatq_pm_deGoodness of fit for pmDemeta.code.qualfloatq_pm_raGoodness of fit for pmRameta.code.qualfloatpflagMean position flagmeta.codecharposflgType of Tycho-2 solutionmeta.id;stat.fitcharccdmCCDM component identifier for HIP starsmeta.code.multipcharproxProximity indicator100masmeta.codeshortbt_magTycho-2 BT magnitudemagphot.mag;em.opt.Bfloatvt_magTycho-2 VT magnitudemagphot.mag;em.opt.Vfloate_bt_magUncertainty of BTmagstat.errorfloate_vt_magUncertainty of VTmagstat.errorfloatsys_noTDSC identifier for the systemmeta.idintcmpComponent designationmeta.id.partcharn_mainNumber of components in TDSC main cataloguemeta.numbershortn_supNumber of components in the TDSC supplementmeta.numbershortmagflgTDSC photometry flagmeta.codecharwdsWDS identifier for the systemmeta.id.crosscharnoteTDSC notesmeta.notecharhdHD identifier for TDSC entriesmeta.id.crossintrcmpReference component for position angle and separationmeta.id.assoccharpaPosition angledegpos.posAngfloatsepSeparationarcsecpos.angDistancefloate_paUncertainty of the position angledegstat.errorfloate_pa_sepUncertainty of the position angle * separationstat.errorshorte_sepUncertainty of the separationmasstat.errorshortgaiaedr3.commanded_scan_lawjd_timeTime [Julian Date in TCB at Gaia - 2455197.5]dtime.epochdoublebjd_fov1Time [Julian Date in TCB at barycentre for FOV1 - 2455197.5]dtime.epochdoublebjd_fov2Time [Julian Date in TCB at barycentre for FOV2 - 2455197.5]dtime.epochdoubleobmt_timeTime at Gaia (OBMT)nstime.epochlongra_fov1Right Ascension of FOV1 centredegpos.eq.rafloatdec_fov1Declination of FOV1 centredegpos.eq.decfloatheal_pix_fov1FOV1 HEALPix level 12pos.healpixintscan_angle_fov1Scan position angle of FOV1degpos.angDistancefloatra_fov2Right ascension of FOV2 centredegpos.eq.rafloatdec_fov2Declination of FOV2 centredegpos.eq.decfloatheal_pix_fov2FOV2 HEALPix level 12pos.healpixintscan_angle_fov2Scan position angle of FOV2degpos.angDistancefloatsolution_idSolution Identifiermeta.versionlonggaiaedr3.frame_rotator_sourcesource_idGaia source identifiermeta.id;meta.main;meta.reflongconsidered_for_reference_frame_orientationConsidered for the reference frame orientationmeta.codebooleanused_for_reference_frame_orientationUsed for the reference frame orientationmeta.codebooleanconsidered_for_reference_frame_spinConsidered for the reference frame spinmeta.codebooleanused_for_reference_frame_spinUsed for the reference frame spinmeta.codebooleangaiaedr3.hipparcos2_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crossintangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.hipparcos2_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crossintangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.tycho2tdsc_merge_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshorttycho2tdsc_merge_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortgaiaedr3.tycho2tdsc_merge_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshorttycho2tdsc_merge_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.panstarrs1_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.panstarrs1_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.panstarrs1_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_panstarrs1_oidExternal Catalogue source identifiermeta.id.crosslonggaiaedr3.sdssdr13_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crossintoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.sdssdr13_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crossintoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.sdssdr13_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_sdssdr13_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.skymapperdr2_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.skymapperdr2_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortgaiaedr3.skymapperdr2_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslonggaiaedr3.urat1_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshorturat1_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiaedr3.urat1_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshorturat1_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.allwise_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortallwise_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiaedr3.allwise_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortallwise_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.apassdr9_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancedoublenumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortxm_flagCross-match algorithm flagmeta.code.statusintgaiaedr3.apassdr9_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crosslongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancedoublescoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusintgaiaedr3.apassdr9_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongclean_apassdr9_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.gsc23_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_gsc23_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiaedr3.gsc23_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_gsc23_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.gsc23_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharclean_gsc23_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.ravedr5_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numbershortgaiaedr3.ravedr5_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.ravedr5_joinoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharclean_ravedr5_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.tmass_psc_xsc_best_neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatxm_flagCross-match algorithm flagmeta.code.statusshortclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crossintnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numbershortnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortgaiaedr3.tmass_psc_xsc_neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosscharangular_distanceAngular Distance between the two sourcesarcsecpos.angDistancefloatscoreScore of neighboursmeta.codedoublexm_flagCross-match algorithm flagmeta.code.statusshortclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3.tmass_psc_xsc_joinoriginal_psc_source_idOriginal 2MASS PSC source identifiermeta.id.crosscharoriginal_xsc_source_idOriginal 2MASS XSC source identifiermeta.id.crosscharclean_tmass_psc_xsc_oidExternal Catalogue source identifiermeta.id.crossintgaiaedr3_contribNon-official contributions to the Gaia Early Data Release 3gaiaedr3_contrib.starhorseEstimating Distance from Parallaxes. StarHorse Catalog v.12source_idGaia EDR3 unique source identifiermeta.id;meta.main;meta.reflongdist05StarHorse distance, 5th percentilekpcpos.distancefloatdist16StarHorse distance, 16th percentilekpcpos.distancefloatdist50StarHorse distance, 50th percentilekpcpos.distancefloatdist84StarHorse distance, 84th percentilekpcpos.distancefloatdist95Starhorse distance, 95th percentilekpcpos.distancefloatav05StarHorse line-of-sight extinction at ? = 5420 Å, AV, 5th percentilemagphys.absorption.galfloatav16StarHorse line-of-sight extinction at ? = 5420 Å, AV, 16th percentilemagphys.absorption.galfloatav50StarHorse line-of-sight extinction at ? = 5420 Å, AV, 50th percentilemagphys.absorption.galfloatav84StarHorse line-of-sight extinction at ? = 5420 Å, AV, 84th percentilemagphys.absorption.galfloatav95StarHorse line-of-sight extinction at ? = 5420 Å, AV, 95th percentilemagphys.absorption.galfloatteff16StarHorse effective temperature, 16th percentileKphys.temperature.effectivefloatteff50StarHorse effective temperature, 50th percentileKphys.temperature.effectivefloatteff84StarHorse effective temperature, 84th percentileKphys.temperature.effectivefloatlogg16StarHorse surface gravity, 16th percentilelog("g")phys.gravityfloatlogg50StarHorse surface gravity, 50th percentilelog("g")phys.gravityfloatlogg84StarHorse surface gravity, 84th percentilelog("g")phys.gravityfloatmet16StarHorse metallicity, 16th percentile"dex"phys.abund.Zfloatmet50StarHorse metallicity, 50th percentile"dex"phys.abund.Zfloatmet84StarHorse metallicity, 84th percentile"dex"phys.abund.Zfloatmass16StarHorse stellar mass, 16th percentilesolMassphys.massfloatmass50StarHorse stellar mass, 50th percentilesolMassphys.massfloatmass84StarHorse stellar mass, 84th percentilesolMassphys.massfloatag50StarHorse line-of-sight extinction in the G band, AG, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatabp50StarHorse line-of-sight extinction in the GBP band, ABP, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatarp50StarHorse line-of-sight extinction in the GRP band, ARP, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatbprp0StarHorse dereddened colour, (GBP - GRP)0, derived from phot_bp_mean_mag, phot_rp_mean_mag, ABP50, and ARP50magphot.mag,stat.meanfloatmg0StarHorse absolute magnitude, derived from phot_g_mean_mag (recalibrated), dist50, and AG50magphot.mag,stat.meanfloatxgalStarHorse Galactocentric Cartesian X coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatygalStarHorse Galactocentric Cartesian Y coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatzgalStarHorse Galactocentric Cartesian Z coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatrgalStarHorse Galactocentric planar distance, derived from XGal and YGalkpcpos.distancefloatfidelityGaia EDR3 astrometric fidelity flag (Rybizki et al. 2021)meta.codefloatbp_rp_excess_corr"Gaia EDR3 photometric BP/RP flux excess factor (corrected following Riello et al. (2021))"meta.codefloatsh_photoflagStarHorse photometry input flagmeta.codecharsh_outflagStarHorse output flagmeta.codechargaiaedr3_contrib.starhorse_1_1Estimating Distance from Parallaxes. StarHorse Catalog v.11source_idGaia EDR3 unique source identifiermeta.id;meta.main;meta.reflongdist05StarHorse distance, 5th percentilekpcpos.distancefloatdist16StarHorse distance, 16th percentilekpcpos.distancefloatdist50StarHorse distance, 50th percentilekpcpos.distancefloatdist84StarHorse distance, 84th percentilekpcpos.distancefloatdist95Starhorse distance, 95th percentilekpcpos.distancefloatav05StarHorse line-of-sight extinction at ? = 5420 Å, AV, 5th percentilemagphys.absorption.galfloatav16StarHorse line-of-sight extinction at ? = 5420 Å, AV, 16th percentilemagphys.absorption.galfloatav50StarHorse line-of-sight extinction at ? = 5420 Å, AV, 50th percentilemagphys.absorption.galfloatav84StarHorse line-of-sight extinction at ? = 5420 Å, AV, 84th percentilemagphys.absorption.galfloatav95StarHorse line-of-sight extinction at ? = 5420 Å, AV, 95th percentilemagphys.absorption.galfloatteff16StarHorse effective temperature, 16th percentileKphys.temperature.effectivefloatteff50StarHorse effective temperature, 50th percentileKphys.temperature.effectivefloatteff84StarHorse effective temperature, 84th percentileKphys.temperature.effectivefloatlogg16StarHorse surface gravity, 16th percentilelog("g")phys.gravityfloatlogg50StarHorse surface gravity, 50th percentilelog("g")phys.gravityfloatlogg84StarHorse surface gravity, 84th percentilelog("g")phys.gravityfloatmet16StarHorse metallicity, 16th percentile"dex"phys.abund.Zfloatmet50StarHorse metallicity, 50th percentile"dex"phys.abund.Zfloatmet84StarHorse metallicity, 84th percentile"dex"phys.abund.Zfloatmass16StarHorse stellar mass, 16th percentilesolMassphys.massfloatmass50StarHorse stellar mass, 50th percentilesolMassphys.massfloatmass84StarHorse stellar mass, 84th percentilesolMassphys.massfloatag50StarHorse line-of-sight extinction in the G band, AG, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatabp50StarHorse line-of-sight extinction in the GBP band, ABP, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatarp50StarHorse line-of-sight extinction in the GRP band, ARP, 50th percentile, derived from AV50 and teff50magphys.absorption.galfloatbprp0StarHorse dereddened colour, (GBP - GRP)0, derived from phot_bp_mean_mag, phot_rp_mean_mag, ABP50, and ARP50magphot.mag,stat.meanfloatmg0StarHorse absolute magnitude, derived from phot_g_mean_mag (recalibrated), dist50, and AG50magphot.mag,stat.meanfloatxgalStarHorse Galactocentric Cartesian X coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatygalStarHorse Galactocentric Cartesian Y coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatzgalStarHorse Galactocentric Cartesian Z coordinate, derived from dist50 and assuming R0 = 8.2 kpckpcpos.distancefloatrgalStarHorse Galactocentric planar distance, derived from XGal and YGalkpcpos.distancefloatfidelityGaia EDR3 astrometric fidelity flag (Rybizki et al. 2021)meta.codefloatbp_rp_excess_corr"Gaia EDR3 photometric BP/RP flux excess factor (corrected following Riello et al. (2021))"meta.codefloatsh_photoflagStarHorse photometry input flagmeta.codecharsh_outflagStarHorse output flagmeta.codechargaiaedr3_contrib.source_id2splitThis table is linking between data splits and sourceid. Table used for the acceleration for PDF data and plots.source_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongsplitstring to identify the PDF files paths, for more detail see https://data.aip.de/starhorse21meta.idchargaiaedr3_contrib.gaia_source_j2000Source positions at reference J2000 for Gaia early data release 3source_idSource IdentifierDimensionlessmeta.id;meta.main;meta.reflongraRight AscensionAngle[deg]pos.eq.radoubledecDeclinationAngle[deg]pos.eq.decdoubleposThe point position of a source (ra, dec) in radianAngle[rad], Angle[rad]pos.eq.ra;pos.eq.decchargaiadr2Gaia second data release.gaiadr2.gaia_sourceMain cataloguesolution_idSolution Identifiermeta.versionlongdesignationUnique source designation (unique across all Data Releases)meta.id;meta.maincharsource_idUnique source identifier (unique within a particular Data Release)meta.id;meta.main;meta.reflongrandom_indexRandom index used to select subsetsmeta.codelongref_epochReference epochTime[Julian Years]meta.ref;time.epochdoubleraRight ascensionAngle[deg]pos.eq.ra;meta.maindoublera_errorStandard error of right ascensionAngle[mas]stat.error;pos.eq.radoubledecDeclinationAngle[deg]pos.eq.dec;meta.maindoubledec_errorStandard error of declinationAngle[mas]stat.error;pos.eq.decdoubleparallaxParallaxAngle[mas]pos.parallaxdoubleparallax_errorStandard error of parallaxAngle[mas]stat.error;pos.parallaxdoubleparallax_over_errorParallax divided by its errorarith.ratiofloatpmraProper motion in right ascension directionAngular Velocity[mas/year]pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.radoublepmdecProper motion in declination directionAngular Velocity[mas/year]pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.decdoublera_dec_corrCorrelation between right ascension and declinationstat.correlation;pos.eq.ra;pos.eq.decfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlation;pos.eq.ra;pos.parallaxfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlation;pos.eq.ra;pos.pm;pos.eq.rafloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlation;pos.eq.ra;pos.pm;pos.eq.decfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlation;pos.eq.dec;pos.parallaxfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlation;pos.eq.dec;pos.pm;pos.eq.rafloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlation;pos.eq.dec;pos.pm;pos.eq.decfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlation;pos.parallax;pos.pm;pos.eq.rafloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlation;pos.parallax;pos.pm;pos.eq.decfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlation;pos.pm;pos.eq.ra;pos.pm;pos.eq.decfloatastrometric_n_obs_alTotal number of observations ALmeta.numberintastrometric_n_obs_acTotal number of observations ACmeta.numberintastrometric_n_good_obs_alNumber of good observations ALmeta.numberintastrometric_n_bad_obs_alNumber of bad observations ALmeta.numberintastrometric_gof_alGoodness of fit statistic of model wrt along-scan observationsstat.fit.goodnessfloatastrometric_chi2_alAL chi-square valuestat.fit.chi2floatastrometric_excess_noiseExcess noise of the sourceAngle[mas]stat.valuedoubleastrometric_excess_noise_sigSignificance of excess noisestat.valuedoubleastrometric_params_solvedWhich parameters have been solved for?meta.numbershortastrometric_primary_flagPrimary or secondaymeta.codebooleanastrometric_weight_alMean astrometric weight of the sourceAngle[mas^-2]stat.weight;stat.meanfloatastrometric_pseudo_colourAstrometrically determined pseudocolour of the sourceMisc[um^-1]em.wavenumberdoubleastrometric_pseudo_colour_errorStandard error of the pseudocolour of the sourceMisc[um^-1]em.wavenumber;stat.errordoublemean_varpi_factor_alMean Parallax factor ALarith.factor;pos.parallaxfloatastrometric_matched_observationsMatched FOV transits used in the AGIS solutionmeta.numbershortvisibility_periods_usedNumber of visibility periods used in Astrometric solutionmeta.numbershortastrometric_sigma5d_maxThe longest semi-major axis of the 5-d error ellipsoidAngle[mas]pos.errorEllipse;stat.maxfloatframe_rotator_object_typeThe type of the source mainly used for frame rotationmeta.codeintmatched_observationsAmount of observations matched to this sourcemeta.numbershortduplicated_sourceSource with duplicate sourcesmeta.code.statusbooleanphot_g_n_obsNumber of observations contributing to G photometrymeta.numberintphot_g_mean_fluxG-band mean fluxFlux[e-/s]phot.flux;stat.mean;em.optdoublephot_g_mean_flux_errorError on G-band mean fluxFlux[e-/s]stat.error;phot.flux;stat.mean;em.optdoublephot_g_mean_flux_over_errorG-band mean flux divided by its errorarith.ratiofloatphot_g_mean_magG-band mean magnitudeMagnitude[mag]phot.mag;stat.mean;em.optfloatphot_bp_n_obsNumber of observations contributing to BP photometrymeta.numberintphot_bp_mean_fluxIntegrated BP mean fluxFlux[e-/s]phot.flux;stat.meandoublephot_bp_mean_flux_errorError on the integrated BP mean fluxFlux[e-/s]stat.error;phot.flux;stat.meandoublephot_bp_mean_flux_over_errorIntegrated BP mean flux divided by its errorarith.ratiofloatphot_bp_mean_magIntegrated BP mean magnitudeMagnitude[mag]phot.mag;stat.meanfloatphot_rp_n_obsNumber of observations contributing to RP photometrymeta.numberintphot_rp_mean_fluxIntegrated RP mean fluxFlux[e-/s]phot.flux;stat.meandoublephot_rp_mean_flux_errorError on the integrated RP mean fluxFlux[e-/s]stat.error;phot.fluxdoublephot_rp_mean_flux_over_errorIntegrated RP mean flux divided by its errorarith.ratiofloatphot_rp_mean_magIntegrated RP mean magnitudeMagnitude[mag]phot.mag;stat.meanfloatphot_bp_rp_excess_factorBP/RP excess factorfloatphot_proc_modePhotometry processing modeshortbp_rpBP - RP colourMagnitude[mag]phot.colorfloatbp_gBP - G colourMagnitude[mag]phot.colorfloatg_rpG - RP colourMagnitude[mag]phot.colorfloatradial_velocityRadial velocityVelocity[km/s]spect.dopplerVeloc.optdoubleradial_velocity_errorRadial velocity errorVelocity[km/s]stat.error;spect.dopplerVeloc.optdoublerv_nb_transitsNumber of transits used to compute radial velocitymeta.numberintrv_template_teffTeff of the template used to compute radial velocityTemperature[K]stat.fit.paramfloatrv_template_logglogg of the template used to compute radial velocityGravitySurface[log cgs]stat.fit.paramfloatrv_template_fe_hFe/H of the template used to compute radial velocityAbundances[dex]stat.fit.paramfloatphot_variable_flagPhotometric variability flagmeta.code;src.varcharlGalactic longitudeAngle[deg]pos.galactic.londoublebGalactic latitudeAngle[deg]pos.galactic.latdoubleecl_lonEcliptic longitudeAngle[deg]pos.ecliptic.londoubleecl_latEcliptic latitudeAngle[deg]pos.ecliptic.latdoublepriam_flagsflags for the Apsis-Priam resultsmeta.codelongteff_valstellar effective temperatureTemperature[K]phys.temperature.effectivefloatteff_percentile_lowerteffVal lower uncertaintyTemperature[K]phys.temperature.effective;stat.minfloatteff_percentile_upperteffVal upper uncertaintyTemperature[K]phys.temperature.effective;stat.maxfloata_g_valline-of-sight extinction in the G band, A_G)Magnitude[mag]phys.absorption.galfloata_g_percentile_loweraGVal lower uncertaintyMagnitude[mag]phys.absorption.gal;stat.minfloata_g_percentile_upperaGVal upper uncertaintyMagnitude[mag]phys.absorption.gal;stat.maxfloate_bp_min_rp_valline-of-sight reddening E(BP-RP)Magnitude[mag]floate_bp_min_rp_percentile_lowereBPminRPVal lower uncertaintyMagnitude[mag]floate_bp_min_rp_percentile_uppereBPminRPVal upper uncertaintyMagnitude[mag]floatflame_flagsFlags for the Apsis-FLAME resultsmeta.codelongradius_valstellar radiusLength & Distance[Solar Radius]phys.size.radiusfloatradius_percentile_lowerradiusVal lower uncertaintyLength & Distance[Solar Radius]phys.size.radius;stat.errorfloatradius_percentile_upperradiusVal upper uncertaintyLength & Distance[Solar Radius]phys.size.radius;stat.errorfloatlum_valstellar luminosityLuminosity[Solar Luminosity]phys.luminosityfloatlum_percentile_lowerlumVal lower uncertaintyLuminosity[Solar Luminosity]phys.luminosity;stat.errorfloatlum_percentile_upperlumVal upper uncertaintyLuminosity[Solar Luminosity]phys.luminosity;stat.errorfloatposThe point position of a source (ra, dec) in radian.Angle[rad], Angle[rad]pos.eq.ra, pos.eq.decchargaiadr2.sso_observationSolar System object observationssolution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongobservation_idObservation Identifiermeta.idlongnumber_mpminor planet number attributed by MPCmeta.id.crosslongepochGaia-centric epoch TCB(Gaia)Time[Barycentric JD in TCB - 2455197.5 (day)]time.epochdoubleepoch_errError in Gaiacentric epochTime[day]stat.error;time.epochdoubleepoch_utcGaiacentric epoch UTCTime[Julian Date (day)]time.epochdoubleraRight ascension of the sourceAngle[deg]pos.eq.radoubledecDeclination of the sourceAngle[deg]pos.eq.decdoublera_error_systematicStandard error of right ascension - systematicAngle[mas]pos.eq.ra;stat.errordoubledec_error_systematicStandard error of declination - systematicAngle[mas]pos.eq.dec;stat.errordoublera_dec_correlation_systematicCorrelation of ra and dec errors - systematicpos.eq;stat.correlationdoublera_error_randomStandard error of right ascension - randomAngle[mas]pos.eq.ra;stat.errordoubledec_error_randomStandard error of declination - randomAngle[mas]pos.eq.dec;stat.errordoublera_dec_correlation_randomCorrelation of ra and dec errors - randompos.eq;stat.correlationdoubleg_magCalibrated G magMagnitude[mag]em.opt;phot.magdoubleg_fluxAverage calibrated G flux for the transitFlux[e-/s]em.opt;phot.flux;stat.meandoubleg_flux_errorError on the G fluxFlux[e-/s]em.opt;phot.flux;stat.errordoublex_gaiaBarycentric x position of GaiaLength & Distance[AU]pos.barycenter;pos.cartesian.xdoubley_gaiaBarycentric y position of GaiaLength & Distance[AU]pos.barycenter;pos.cartesian.ydoublez_gaiaBarycentric z position of GaiaLength & Distance[AU]pos.barycenter;pos.cartesian.zdoublevx_gaiaBarycentric x velocity of GaiaVelocity[au/d]phys.veloc;pos.barycenter;pos.cartesian.xdoublevy_gaiaBarycentric y velocity of GaiaVelocity[au/d]phys.veloc;pos.barycenter;pos.cartesian.ydoublevz_gaiaBarycentric z velocity of GaiaVelocity[au/d]phys.veloc;pos.barycenter;pos.cartesian.zdoubleposition_angle_scanPosition angle of the scanning directionAngle[deg]pos.posAngdoublelevel_of_confidenceLevel of confidence of the identificationDimensionless[percentage/100]meta.id.cross;stat.likelihoodshortposchargaiadr2.sso_sourceSolar System objects related datasolution_idSolution Identifiermeta.versionlongsource_idSource identifiermeta.id;meta.main;meta.reflongnum_of_obsnumber of observationsmeta.numberintnumber_mpMinor Planet numbermeta.id.crosslongdenominationstandard MPC denomination of the asteroidmeta.id.crosschargaiadr2.vari_cepheidCepheid starstype_best_classificationBest type classification estimate out of: {"DCEP", "T2CEP", "ACEP"}meta.code.class;src.classchartype2_best_sub_classificationBest subclassification estimate for typeBestClassification="T2CEP" out of: {"BL_HER", "W_VIR","RV_TAU"}meta.code.class;src.classcharmode_best_classificationBest mode classification estimate out of: { "FUNDAMENTAL", "FIRST_OVERTONE","SECOND_OVERTONE","MULTI","UNDEFINED","NOT_APPLICABLE"}meta.code.class;src.classcharmulti_mode_best_classificationBest multi mode DCEP classification out of: { "F/1O", "F/2O","1O/2O","1O/3O","2O/3O","F/1O/2O","1O/2O/3O"}meta.code.class;src.classcharsolution_idlongsource_idmeta.id;meta.main;meta.reflongpfdoublepf_errordoublep1_odoublep1_o_errordoublep2_odoublep2_o_errordoublep3_odoublep3_o_errordoubleepoch_gdoubleepoch_g_errordoubleepoch_bpdoubleepoch_bp_errordoubleepoch_rpdoubleepoch_rp_errordoubleint_average_gdoubleint_average_g_errordoubleint_average_bpdoubleint_average_bp_errordoubleint_average_rpdoubleint_average_rp_errordoublepeak_to_peak_gdoublepeak_to_peak_g_errordoublepeak_to_peak_bpdoublepeak_to_peak_bp_errordoublepeak_to_peak_rpdoublepeak_to_peak_rp_errordoublemetallicitydoublemetallicity_errordoubler21_gdoubler21_g_errordoubler31_gdoubler31_g_errordoublephi21_gdoublephi21_g_errordoublephi31_gdoublephi31_g_errordoublenum_clean_epochs_gintnum_clean_epochs_bpintnum_clean_epochs_rpintg_absorptiondoubleg_absorption_errordoublegaiadr2.vari_classifier_class_definitionDetailed description of variable classessolution_idSolution Identifiermeta.versionlongclassifier_nameName of the classifier that is detailed in this entrymeta.softwarecharclass_nameName of the published class from this classifiermeta.titlecharclass_descriptionDescription of the published class from this classifiermeta.notechargaiadr2.vari_classifier_definitionDescription of all classifierssolution_idSolution Identifiermeta.versionlongclassifier_nameName of the classifier that is detailed in this entrymeta.softwarecharclassifier_descriptionDescription of this classifiermeta.softwarechargaiadr2.vari_classifier_resultVariability classification resultssolution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongclassifier_nameClassifier name used to produce this result, use for lookup in VariClassifierDefinition tablemeta.softwarecharbest_class_nameName of best class, see table VariClassifierDefinition for details of the classmeta.titlecharbest_class_scoreScore of the best classmeta.code.qualdoublegaiadr2.vari_long_period_variableLong period variablessolution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongabs_mag_bolAbsolute bolometric magnitude of the starMagnitude[mag]phot.mag.boldoubleabs_mag_bol_errorError of absolute bolometric magnitudeMagnitude[mag]phot.mag.bol;stat.errordoublersg_flagRed supergiant flagmeta.code.statusbooleanbolometric_corrBolometric correction for LPVsMagnitude[mag]phot.mag.bcdoublebolometric_corr_errorError of the bolometric correctionMagnitude[mag]phot.mag.bc;stat.errordoublefrequencyFrequency of the LPVFrequency[day^-1]doublefrequency_errorError on the frequencyFrequency[day^-1]doublegaiadr2.vari_rotation_modulationRotation Modulationsegments_rotation_periodRotation period in segmentTime[day]phys.veloc.rotat;time.periodcharsegments_rotation_period_errorRotation period uncertainty in segmentTime[day]phys.veloc.rotat;time.period;stat.errorcharsegments_rotation_period_fapFAP on rotation period in segmentDimensionless[percentage/100]stat.probabilitycharsegments_cos_termCoefficient of cosine term of linear fit in segmentMagnitude[mag]stat.fit.paramcharsegments_cos_term_errorErrors on cosin termsMagnitude[mag]stat.error;stat.fit.paramcharsegments_sin_termCoefficient of sin term of linear fit in segmentMagnitude[mag]stat.fit.paramcharsegments_sin_term_errorErrors on sine termsMagnitude[mag]stat.error;stat.fit.paramcharsegments_a0_termConstant term (A0) of linear fit in segmentMagnitude[mag]stat.fit.paramcharsegments_a0_term_errorErrors on constant termsMagnitude[mag]stat.error;stat.fit.paramcharbest_rotation_periodBest rotation periodTime[day]phys.veloc.rotat;time.perioddoublebest_rotation_period_errorError on best rotation periodTime[day]phys.veloc.rotat;time.period;stat.errordoublesegments_activity_indexActivity Index in segmentMagnitude[mag]phot.mag;src.var.amplitudecharsegments_activity_index_errorerror on Activity index in segmentMagnitude[mag]phot.mag;src.var.amplitude;stat.errorcharmax_activity_indexThe maximum Activity IndexMagnitude[mag]phot.mag;src.var.amplitude;stat.maxdoublemax_activity_index_errorError on maximum activity indexMagnitude[mag]phot.mag;src.var.amplitude;stat.max;stat.errordoublesegments_g_unspottedThe unspotted G mags in segmentMagnitude[mag]em.opt;phot.mag;stat.mincharsegments_g_unspotted_errorThe unspotted G mag uncertainties in segmentMagnitude[mag]em.opt;phot.mag;stat.error;stat.mincharsegments_bp_unspottedThe unspotted BP mag in segmentMagnitude[mag]em.opt.B;phot.mag;stat.mincharsegments_bp_unspotted_errorThe unspotted BP mag uncertainties in segmentMagnitude[mag]em.opt.B;phot.mag;stat.min;stat.errorcharsegments_rp_unspottedThe unspotted RP mag in segmentMagnitude[mag]em.opt.R;phot.mag;stat.mincharsegments_rp_unspotted_errorThe unspotted RP mag uncertainties in segmentMagnitude[mag]em.opt.R;phot.mag;stat.min;stat.errorcharg_unspottedUnspotted G magMagnitude[mag]em.opt;phot.mag;stat.mindoubleg_unspotted_errorUnspotted G mag uncertaintyMagnitude[mag]em.opt;phot.mag;stat.min;stat.errordoublebp_unspottedUnspotted BP magMagnitude[mag]em.opt.B;phot.mag;stat.mindoublebp_unspotted_errorUnspotted BP mag uncertaintyMagnitude[mag]em.opt.B;phot.mag;stat.min;stat.errordoublerp_unspottedUnspotted RP magMagnitude[mag]em.opt.R;phot.mag;stat.mindoublerp_unspotted_errordoublesolution_idlongsource_idmeta.id;meta.main;meta.reflongnum_segmentsintsegments_start_timecharsegments_end_timecharsegments_colour_mag_interceptcharsegments_colour_mag_intercept_errorcharsegments_colour_mag_slopecharsegments_colour_mag_slope_errorcharsegments_correlation_coefficientcharsegments_correlation_significancecharnum_outliersintoutliers_timechargaiadr2.vari_rrlyraeRR Lyrae starsbest_classificationBest RR Lyrae classification estimate out of: {"RRC", "RRAB", "RRD"}meta.code.class;src.classcharsolution_idlongsource_idmeta.id;meta.main;meta.reflongpfdoublepf_errordoublep1_odoublep1_o_errordoublep2_odoublep2_o_errordoublep3_odoublep3_o_errordoubleepoch_gdoubleepoch_g_errordoubleepoch_bpdoubleepoch_bp_errordoubleepoch_rpdoubleepoch_rp_errordoubleint_average_gdoubleint_average_g_errordoubleint_average_bpdoubleint_average_bp_errordoubleint_average_rpdoubleint_average_rp_errordoublepeak_to_peak_gdoublepeak_to_peak_g_errordoublepeak_to_peak_bpdoublepeak_to_peak_bp_errordoublepeak_to_peak_rpdoublepeak_to_peak_rp_errordoublemetallicitydoublemetallicity_errordoubler21_gdoubler21_g_errordoubler31_gdoubler31_g_errordoublephi21_gdoublephi21_g_errordoublephi31_gdoublephi31_g_errordoublenum_clean_epochs_gintnum_clean_epochs_bpintnum_clean_epochs_rpintg_absorptiondoubleg_absorption_errordoublegaiadr2.vari_short_timescaleShort timescale sourcessolution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongamplitude_estimateAmplitude estimate of all per CCD G-band photometry (quantile(95%)-quantile(5%))Magnitude[mag]src.var.amplitude;phot.mag;em.optdoublenumber_of_fov_transitsNumber of FoV transits with more than 7 CCD measurements after time series cleaningmeta.numberintmean_of_fov_abbe_valuesMean of per-FOV Abbe values derived from CCD G-band photometrystat.valuedoublevariogram_num_pointsNumber of points in the variogrammeta.numberintvariogram_char_timescalesCharacteristic time scales of variabilityTime[day]timecharvariogram_valuesVariogram values associated with the variogramCharTimescalesMisc[mag**2]stat.valuecharfrequencyFrequency search result for either G CCD, G FoV, BP or RP photometry (Null if no periodicity detected)Frequency[day^-1]src.var;time.perioddoublegaiadr2.vari_time_series_statisticsStatistical parameters of time seriessolution_idSolution Identifiermeta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_selected_g_fovTotal number of G FOV transits selected for variability analysismeta.numberintmean_obs_time_g_fovMean observation time for G FoV transitsTime[Barycentric JD in TCB - 2455197.5 (day)]stat.mean;timedoubletime_duration_g_fovTime duration of the time series for G FoV transitsTime[day]time.durationdoublemin_mag_g_fovMinimum G FoV magnitudeMagnitude[mag]em.opt;phot.mag;stat.mindoublemax_mag_g_fovMaximum G FoV magnitudeMagnitude[mag]em.opt;phot.mag;stat.maxdoublemean_mag_g_fovMean G FoV magnitudeMagnitude[mag]em.opt;phot.mag;stat.meandoublemedian_mag_g_fovMedian G FoV magnitudeMagnitude[mag]em.opt;phot.mag;stat.mediandoublerange_mag_g_fovDifference between the highest and lowest G FoV magnitudesMagnitude[mag]em.opt;phot.mag;arith.diffdoublestd_dev_mag_g_fovSquare root of the unweighted G FoV magnitude varianceMagnitude[mag]em.opt;phot.mag;stat.stdevdoubleskewness_mag_g_fovStandardized unweighted G FoV magnitude skewnessem.opt;phot.mag;stat.valuedoublekurtosis_mag_g_fovStandardized unweighted G FoV magnitude kurtosisem.opt;phot.mag;stat.valuedoublemad_mag_g_fovMedian Absolute Deviation (MAD) for G FoV transitsMagnitude[mag]em.opt;phot.mag;stat.valuedoubleabbe_mag_g_fovAbbe value for G FoV transitsem.opt;phot.mag;stat.valuedoubleiqr_mag_g_fovInterquartile range for G FoV transitsMagnitude[mag]em.opt;phot.mag;stat.valuedoublenum_selected_bpTotal number of BP observations selected for variability analysismeta.numberintmean_obs_time_bpMean observation time for BP observationsTime[Barycentric JD in TCB - 2455197.5 (day)]stat.mean;timedoubletime_duration_bpTime duration of the BP time seriesTime[day]time.durationdoublemin_mag_bpMinimum BP magnitudeMagnitude[mag]em.opt.B;phot.mag;stat.mindoublemax_mag_bpMaximum BP magnitudeMagnitude[mag]em.opt.B;phot.mag;stat.maxdoublemean_mag_bpMean BP magnitudeMagnitude[mag]em.opt.B;phot.mag;stat.meandoublemedian_mag_bpMedian BP magnitudeMagnitude[mag]em.opt.B;phot.mag;stat.mediandoublerange_mag_bpDifference between the highest and lowest BP magnitudesMagnitude[mag]em.opt.B;phot.mag;arith.diffdoublestd_dev_mag_bpSquare root of the unweighted BP magnitude varianceMagnitude[mag]em.opt.B;phot.mag;stat.stdevdoubleskewness_mag_bpStandardized unweighted BP magnitude skewnessem.opt.B;phot.mag;stat.valuedoublekurtosis_mag_bpStandardized unweighted BP magnitude kurtosisem.opt.B;phot.mag;stat.valuedoublemad_mag_bpMedian Absolute Deviation (MAD) for BP observationsMagnitude[mag]em.opt.B;phot.mag;stat.valuedoubleabbe_mag_bpAbbe value for BP observationsem.opt.B;phot.mag;stat.valuedoubleiqr_mag_bpInterquartile BP magnitude rangeMagnitude[mag]em.opt.B;phot.mag;stat.valuedoublenum_selected_rpTotal number of RP observations selected for variability analysismeta.numberintmean_obs_time_rpMean observation time for RP observationsTime[Barycentric JD in TCB - 2455197.5 (day)]stat.mean;timedoubletime_duration_rpTime duration of the RP time seriesTime[day]time.durationdoublemin_mag_rpMinimum RP magnitudeMagnitude[mag]em.opt.R;phot.mag;stat.mindoublemax_mag_rpMaximum RP magnitudeMagnitude[mag]em.opt.R;phot.mag;stat.maxdoublemean_mag_rpMean RP magnitudeMagnitude[mag]em.opt.R;phot.mag;stat.meandoublemedian_mag_rpMedian RP magnitudeMagnitude[mag]em.opt.R;phot.mag;stat.mediandoublerange_mag_rpDifference between the highest and lowest RP magnitudesMagnitude[mag]em.opt.R;phot.mag;arith.diffdoublestd_dev_mag_rpSquare root of the unweighted RP magnitude varianceMagnitude[mag]em.opt.R;phot.mag;stat.stdevdoubleskewness_mag_rpStandardized unweighted RP magnitude skewnessem.opt.R;phot.mag;stat.valuedoublekurtosis_mag_rpStandardized unweighted RP magnitude kurtosisem.opt.R;phot.mag;stat.valuedoublemad_mag_rpMedian Absolute Deviation (MAD) for RP observationsMagnitude[mag]em.opt.R;phot.mag;stat.valuedoubleabbe_mag_rpAbbe value for RP observationsem.opt.R;phot.mag;stat.valuedoubleiqr_mag_rpInterquartile RP magnitude rangeMagnitude[mag]em.opt.R;phot.mag;stat.valuedoublegaiadr2.epoch_photometryCalibrated FoV transit photometrysolution_idSolution Identifiermeta.versionlongsource_idSource Identifiermeta.id;meta.main;meta.reflongn_transitsNumber of Gaia transitsmeta.numbershorttransit_idTransit Identifiermeta.idcharg_transit_timetransit averaged G band observation timeTime[Barycentric JD in TCB - 2455197.5 (day)]time.epochcharg_transit_fluxtransit averaged G band fluxFlux[e-/s]em.opt;phot.flux;stat.meancharg_transit_flux_errorError on the transit averaged G band fluxFlux[e-/s]em.opt;phot.flux;stat.errorcharg_transit_flux_over_errortransit averaged G band flux divided by its errorarith.ratiocharg_transit_magtransit averaged G band magnitude (converted from transit averaged G band flux)Magnitude[mag]phot.mag;em.optcharbp_obs_timeBP CCD transit observation timeTime[Barycentric JD in TCB - 2455197.5 (day)]time.epochcharbp_fluxBP band fluxFlux[e-/s]em.opt.B;phot.flux;stat.meancharbp_flux_errorError on the BP band fluxFlux[e-/s]em.opt.B;phot.flux;stat.errorcharbp_flux_over_errorBP band flux divided by its errorarith.ratiocharbp_magBP band magnitude (converted from BP band flux)Magnitude[mag]em.opt.B;phot.magcharrp_obs_timeRP CCD transit observation timeTime[Barycentric JD in TCB - 2455197.5 (day)]time.epochcharrp_fluxRP band fluxFlux[e-/s]em.opt.R;phot.flux;stat.meancharrp_flux_errorError on the RP band fluxFlux[e-/s]em.opt.R;phot.flux;stat.errorcharrp_flux_over_errorRP band flux divided by its errorarith.ratiocharrp_magRP band magnitude (converted from RP band flux)Magnitude[mag]phot.mag;em.opt.Rcharphotometry_flag_noisy_dataG band flux scatter larger than expected by photometry processing (all CCDs considered)meta.code.statuscharphotometry_flag_sm_unavailableSM transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af1_unavailableAF1 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af2_unavailableAF2 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af3_unavailableAF3 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af4_unavailableAF4 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af5_unavailableAF5 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af6_unavailableAF6 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af7_unavailableAF7 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af8_unavailableAF8 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_af9_unavailableAF9 transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_bp_unavailableBP transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_rp_unavailableRP transit unavailable by photometry processingmeta.code.statuscharphotometry_flag_sm_rejectSM transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af1_rejectAF1 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af2_rejectAF2 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af3_rejectAF3 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af4_rejectAF4 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af5_rejectAF5 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af6_rejectAF6 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af7_rejectAF7 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af8_rejectAF8 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_af9_rejectAF9 transit rejected by photometry processingmeta.code.statuscharphotometry_flag_bp_rejectBP transit rejected by photometry processingmeta.code.statuscharphotometry_flag_rp_rejectRP transit rejected by photometry processingmeta.code.statuscharvariability_flag_g_rejectAverage G transit photometry rejected by variability processingmeta.code.statuscharvariability_flag_bp_rejectBP transit photometry rejected by variability processingmeta.code.statuscharvariability_flag_rp_rejectRP transit photometry rejected by variability processingmeta.code.statuschargaiadr2.allwise_best_neighbourAllwise best neighbourallwise_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.allwise_neighbourhoodAllwise neighbourhoodallwise_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.apassdr9_best_neighbourAPASS DR9 best neighbourapassdr9_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.apassdr9_neighbourhoodAPASS DR9 neighbourhoodapassdr9_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.gsc23_best_neighbourGSC2.3 best neighbourgsc23_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.gsc23_neighbourhoodGSC2.3 neighbourhoodgsc23_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.hipparcos2_best_neighbourHipparcos-2 best neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesAngle[arcsec]pos.angDistancedoublenumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numberintgaia_astrometric_paramsNumber of Gaia astrometric params usedmeta.code.statusshortgaiadr2.hipparcos2_neighbourhoodHipparcos-2 neighbourhoodsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesAngle[arcsec]pos.angDistancedoublescoreScore of neighboursmeta.codedoublegaia_astrometric_paramsNumber of Gaia astrometric params usedmeta.code.statusshortgaiadr2.panstarrs1_best_neighbourPan-STARRS1 best neighboursource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesAngle[arcsec]pos.angDistancedoublenumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortgaia_astrometric_paramsNumber of Gaia astrometric params usedmeta.code.statusshortgaiadr2.panstarrs1_neighbourhoodPan-STARRS1 neighbourhoodsource_idUnique Gaia source identifiermeta.id;meta.main;meta.reflongoriginal_ext_source_idOriginal External Catalogue source identifiermeta.id.crosslongangular_distanceAngular Distance between the two sourcesAngle[arcsec]pos.angDistancedoublescoreScore of neighboursmeta.codedoublegaia_astrometric_paramsNumber of Gaia astrometric params usedmeta.code.statusshortgaiadr2.ppmxl_best_neighbourPPMXL best neighbourppmxl_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.ppmxl_neighbourhoodPPMXL neighbourhoodppmxl_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.ravedr5_best_neighbourRAVE DR5 best neighbourravedr5_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numberintsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.ravedr5_neighbourhoodRAVE DR5 neighbourhoodravedr5_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.sdssdr9_best_neighbourSDSS DR9 best neighboursdssdr9_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.sdssdr9_neighbourhoodSDSS DR9 neighbourhoodsdssdr9_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.tmass_best_neighbour2MASS best neighbourtmass_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.tmass_neighbourhood2MASS neighbourhoodtmass_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.tycho2_best_neighbourTycho-2 best neighbourtycho2_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in Gaia Cataloguemeta.numberintsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.tycho2_neighbourhoodTycho-2 neighbourhoodtycho2_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.urat1_best_neighbourURAT-1 best neighboururat1_oidExternal Catalogue source identifiermeta.id.crosslongnumber_of_neighboursNumber of neighbours in External Cataloguemeta.numberintnumber_of_matesNumber of mates in Gaia Cataloguemeta.numbershortbest_neighbour_multiplicityNumber of neighbours with same probability as best neighbourmeta.numbershortsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublegaia_astrometric_paramsshortgaiadr2.urat1_neighbourhoodURAT-1 neighbourhoodurat1_oidExternal Catalogue source identifiermeta.id.crosslongsource_idmeta.id;meta.main;meta.reflongoriginal_ext_source_idcharangular_distancedoublescoredoublegaia_astrometric_paramsshortgaiadr2.aux_allwise_agn_gdr2_cross_idGaia DR2 celestial reference frame sourcesallwise_nameIdentifier in the ALLWISE AGN cataloguemeta.id.cross;meta.maincharsource_idGaia source identifiermeta.id;meta.main;meta.reflonggaiadr2.aux_iers_gdr2_cross_idGaia DR2 celestial reference frame sourcesiers_nameIERS namemeta.id.cross;meta.maincharsource_idGaia source identifiermeta.id;meta.main;meta.reflonggaiadr2.aux_sso_orbit_residualsOrbital fit residualssource_idSource identifiermeta.id;meta.main;meta.reflongtransit_idTransit Identifiermeta.idlongobservation_idObservation Identifiermeta.id.crosslongnumber_mpminor planet number attributed by MPCmeta.id.crosslongepochGaiacentric epoch TCB(Gaia)Time[Barycentric JD in TCB - 2455197.5 (day)]time.epochdoubleresidual_rapost-orbital fit residual in RA*cos(Dec)Angle[mas]arith.diff;pos.angDistancedoubleresidual_decpost-orbital fit residual in DecAngle[mas]arith.diff;pos.angDistancedoubleresidual_alpost-orbital fit residual ALAngle[mas]arith.diff;pos.angDistancedoubleresidual_acpost-orbital fit residual ACAngle[mas]arith.diff;pos.angDistancedoubleselectedobservation not rejected by orbital fitmeta.code.statusbooleangaiadr2.aux_sso_orbitsOrbit auxiliary informationsolution_idSolution Identifiermeta.versionlongnumber_mpAsteroid MPC numbermeta.idlongdesignationMPC namemeta.id;meta.maincharmag_habsolute magnitudeMagnitude[mag]phot.magdoubleslope_gslope parameterstat.fit.paramdoublecodeobject specific flagsmeta.code.statusintobs_arcarc spanned by the observationsTime[day]time.intervallongobs_numnumber of observations usedmeta.numberlongosc_epochepoch of osculationTime[yyyymmdd]time.epochcharorb_mmean anomalyAngle[deg]src.orbital.meanAnomalydoubleomegaargument of perihelionAngle[deg]src.orbital.periastrondoublenode_omegalongitude of ascending nodeAngle[deg]src.orbital.nodedoubleinclinationorbit inclinationAngle[deg]src.orbital.inclinationdoubleeccentricityorbit eccentricitysrc.orbital.eccentricitydoubleasemimajor axisLength & Distance[AU]src.orbital;phys.size.smajAxisdoubleorb_datedate of orbit computationTime[yyyymmdd]time.processingcharceucurrent orbit uncertaintyAngle[arcsec]src.orbital;stat.errordoubleceu_raterate of change of the orbit uncertaintyAngular Velocity[mas/s]arith.rate;src.orbital;stat.errordoubleceu_epochdate of the CEUTime[yyyymmdd]timechargaiadr2_contribTables derived from GDR2 data.gaiadr2_contrib.geometric_distanceEstimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2. For the vast majority of stars in the second Gaia data release, reliable distances cannot be obtained by inverting the parallax. A correct inference procedure must instead be used to account for the nonlinearity of the transformation and the asymmetry of the resulting probability distribution. Here, we infer distances to essentially all 1.33 billion stars with parallaxes published in the second Gaia data release. This is done using a weak distance prior that varies smoothly as a function of Galactic longitude and latitude according to a Galaxy model. The irreducible uncertainty in the distance estimate is characterized by the lower and upper bounds of an asymmetric confidence interval. Although more precise distances can be estimated for a subset of the stars using additional data (such as photometry), our goal is to provide purely geometric distance estimates, independent of assumptions about the physical properties of, or interstellar extinction toward, individual stars. We analyze the characteristics of the catalog and validate it using clusters.source_idSource identifier, identical to the Gaia-DR2 source_idmeta.id;meta.main;meta.reflongr_estEstimated distancepcpos.distancedoubler_loLower bound on the confidence interval of the estimated distancepcstat.error;pos.distancedoubler_hiUpper bound on the confidence interval of the estimated distancepcstat.error;pos.distancedoubler_lenLength scale used in the prior for the distance estimationpcpos.distancedoubleresult_flag=0 failed estimate (none of r_est, r_lo, r_hi are defined) =1 r_est is the mode (highest if the posterior is bimodal); r_lo/r_hi define the lower/upper limits of the highest density interval (HDI) containing 68% of the posterior probability =2 r_est is the median; r_lo/r_hi define the lower/upper limits of the equal-tailed interval (ETI), containing 68% of the posterior probabilityshortmodality_flagno. of modes in the posterior (1 or 2)shortgaiadr2_contrib.ruweThis table includes re-normalised unit weight error (RUWE) for sources from the Gaia DR2 gaia_source table. Values of RUWE less than or equal to 1.4 are considered to be indicating a good astrometric solution. More information on how these values are derived can be found in this [document](http://www.rssd.esa.int/doc_fetch.php?id=3757412).source_idUnique source identifierDimensionlessmeta.id;meta.main;meta.reflongruweRe-normalised unit weight errorDimensionlessstat.errordoublegaiadr2_contrib.starhorse_v05Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2.sh_photoflagStarHorse photometry input flagDimensionlessmeta.codecharsource_idUnique source identifier (unique within a particular Data Release) of Gaia DR2Dimensionlessmeta.id;meta.main;meta.reflongsh_parallaxflagStarHorse parallax input flagDimensionlessmeta.codecharsh_gaiaflagStarHorse GDR2 quality flagDimensionlessmeta.codecharsh_outflagStarHorse output quality flagDimensionlessmeta.codechardist05StarHorse distance, 5th percentileDistance[kpc]pos.distancedoubledist16StarHorse distance, 16th percentileDistance[kpc]pos.distancedoubledist50StarHorse distance, 50th percentileDistance[kpc]pos.distancedoubledist84StarHorse distance, 84th percentileDistance[kpc]pos.distancedoubledist95StarHorse distance, 95th percentileDistance[kpc]pos.distancedoubleav05StarHorse line-of-sight extinction at 5420 nm, A_V, 5th percentileMagnitude[mag]phys.absorption.galdoubleav16StarHorse line-of-sight extinction at 5420 nm, A_V, 16th percentileMagnitude[mag]phys.absorption.galdoubleav50StarHorse line-of-sight extinction at 5420 nm, A_V, 50th percentileMagnitude[mag]phys.absorption.galdoubleav84StarHorse line-of-sight extinction at 5420 nm, A_V, 84th percentileMagnitude[mag]phys.absorption.galdoubleav95StarHorse line-of-sight extinction at 5420 nm, A_V, 95th percentileMagnitude[mag]phys.absorption.galdoubleag50StarHorse line-of-sight extinction in the Gaia DR2 G band (Maiz-Apellaniz & Weiler 2018), A_G, 50th percentileMagnitude[mag]phys.absorption.galdoubleteff16StarHorse effective temperature, 16th percentileTemperature[K]phys.temperature.effectivedoubleteff50StarHorse effective temperature, 50th percentileTemperature[K]phys.temperature.effectivedoubleteff84StarHorse effective temperature, 84th percentileTemperature[K]phys.temperature.effectivedoublelogg16StarHorse surface gravity, 16th percentileGravitySurface[log cgs]phys.gravitydoublelogg50StarHorse surface gravity, 50th percentileGravitySurface[log cgs]phys.gravitydoublelogg84StarHorse surface gravity, 84th percentileGravitySurface[log cgs]phys.gravitydoublemet16StarHorse metallicity, 16th percentileAbundances[dex]phys.abund.Zdoublemet50StarHorse metallicity, 50th percentileAbundances[dex]phys.abund.Zdoublemet84StarHorse metallicity, 84th percentileAbundances[dex]phys.abund.Zdoublemass16StarHorse stellar mass, 16th percentileMass[solar]phys.massdoublemass50StarHorse stellar mass, 50th percentileMass[solar]phys.massdoublemass84StarHorse stellar mass, 84th percentileMass[solar]phys.massdoubleabp50StarHorse line-of-sight extinction in the G_BP band (Maiz-Apellaniz & Weiler 2018), A_BP, 50th percentileMagnitude[mag]phys.absorption.galdoublearp50StarHorse line-of-sight extinction in the G_RP band (Maiz-Apellaniz & Weiler 2018), A_RP, 50th percentileMagnitude[mag]phys.absorption.galdoublebprp0StarHorse dereddened G_BP - G_RP colour, derived from phot_bp_mean_mag, phot_rp_mean_mag, Teff50 and AV50Magnitude[mag]phot.mag;stat.meandoublemg0StarHorse absolute magnitude, derived from phot_g_mean_mag_oct2018, dist50, and AG50Magnitude[mag]phot.mag;stat.meandoublexgalStarHorse Galactocentric Cartesian X coordinate, derived from dist50Distance[kpc]pos.distancedoubleygalStarHorse Galactocentric Cartesian Y coordinate, derived from dist50Distance[kpc]pos.distancedoublezgalStarHorse Galactocentric Cartesian Z coordinate, derived from dist50Distance[kpc]pos.distancedoublergalStarHorse Galactocentric distance, derived from dist50 and assuming R_0 = 8.2 kpcDistance[kpc]pos.distancedoubleruweGaia DR2 renormalised unit weight error (RUWE; Lindegren 2018)Dimensionlessstat.errordoublegaiadr2_contrib.starhorseEstimating Distance from Parallaxes. StarHorse Catalog v.06, with dr2_source_id (source_id). From Gaia Early DR3 are added dr3_source_id (source_id of gaiaedr3), angular_distance, magnitude_difference, proper_motion_propagation, dup_max_number.dr3_source_idUnique source identifier (unique within a particular Data Release) of Gaia EDR3Dimensionlessmeta.idlongsource_idUnique source identifier (unique within a particular Data Release) of Gaia DR2Dimensionlessmeta.id;meta.main;meta.reflongsh_photoflagStarHorse photometry input flagDimensionlessmeta.codecharsh_parallaxflagStarHorse parallax input flagDimensionlessmeta.codecharsh_gaiaflagStarHorse GDR2 quality flagDimensionlessmeta.codecharsh_outflagStarHorse output quality flagDimensionlessmeta.codechardist05StarHorse distance, 5th percentileDistance[kpc]pos.distancedoubledist16StarHorse distance, 16th percentileDistance[kpc]pos.distancedoubledist50StarHorse distance, 50th percentileDistance[kpc]pos.distancedoubledist84StarHorse distance, 84th percentileDistance[kpc]pos.distancedoubledist95StarHorse distance, 95th percentileDistance[kpc]pos.distancedoubleav05StarHorse line-of-sight extinction at 5420 nm, A_V, 5th percentileMagnitude[mag]phys.absorption.galdoubleav16StarHorse line-of-sight extinction at 5420 nm, A_V, 16th percentileMagnitude[mag]phys.absorption.galdoubleav50StarHorse line-of-sight extinction at 5420 nm, A_V, 50th percentileMagnitude[mag]phys.absorption.galdoubleav84StarHorse line-of-sight extinction at 5420 nm, A_V, 84th percentileMagnitude[mag]phys.absorption.galdoubleav95StarHorse line-of-sight extinction at 5420 nm, A_V, 95th percentileMagnitude[mag]phys.absorption.galdoubleag50StarHorse line-of-sight extinction in the Gaia DR2 G band (Maiz-Apellaniz & Weiler 2018), A_G, 50th percentileMagnitude[mag]phys.absorption.galdoubleteff16StarHorse effective temperature, 16th percentileTemperature[K]phys.temperature.effectivedoubleteff50StarHorse effective temperature, 50th percentileTemperature[K]phys.temperature.effectivedoubleteff84StarHorse effective temperature, 84th percentileTemperature[K]phys.temperature.effectivedoublelogg16StarHorse surface gravity, 16th percentileGravitySurface[log cgs]phys.gravitydoublelogg50StarHorse surface gravity, 50th percentileGravitySurface[log cgs]phys.gravitydoublelogg84StarHorse surface gravity, 84th percentileGravitySurface[log cgs]phys.gravitydoublemet16StarHorse metallicity, 16th percentileAbundances[dex]phys.abund.Zdoublemet50StarHorse metallicity, 50th percentileAbundances[dex]phys.abund.Zdoublemet84StarHorse metallicity, 84th percentileAbundances[dex]phys.abund.Zdoublemass16StarHorse stellar mass, 16th percentileMass[solar]phys.massdoublemass50StarHorse stellar mass, 50th percentileMass[solar]phys.massdoublemass84StarHorse stellar mass, 84th percentileMass[solar]phys.massdoubleabp50StarHorse line-of-sight extinction in the G_BP band (Maiz-Apellaniz & Weiler 2018), A_BP, 50th percentileMagnitude[mag]phys.absorption.galdoublearp50StarHorse line-of-sight extinction in the G_RP band (Maiz-Apellaniz & Weiler 2018), A_RP, 50th percentileMagnitude[mag]phys.absorption.galdoublebprp0StarHorse dereddened G_BP - G_RP colour, derived from phot_bp_mean_mag, phot_rp_mean_mag, Teff50 and AV50Magnitude[mag]phot.mag;stat.meandoublemg0StarHorse absolute magnitude, derived from phot_g_mean_mag_oct2018, dist50, and AG50Magnitude[mag]phot.mag;stat.meandoublexgalStarHorse Galactocentric Cartesian X coordinate, derived from dist50Distance[kpc]pos.distancedoubleygalStarHorse Galactocentric Cartesian Y coordinate, derived from dist50Distance[kpc]pos.distancedoublezgalStarHorse Galactocentric Cartesian Z coordinate, derived from dist50Distance[kpc]pos.distancedoublergalStarHorse Galactocentric distance, derived from dist50 and assuming R_0 = 8.2 kpcDistance[kpc]pos.distancedoubleruweGaia DR2 renormalised unit weight error (RUWE; Lindegren 2018)Dimensionlessstat.errordoubleangular_distanceAngular distance between the two sourcesAngle[mas]pos.angDistancedoublemagnitude_differenceG band magnitude difference between the sourcesMagnitude[mag]phot.mag;arith.diffdoubleproper_motion_propagationFlag indicating whether E/DR3 coordinates were proper motion correctedDimensionlessmeta.code.statusbooleandup_max_number4m stars have more than one counterpart, provides number of duplicatesDimensionlessmeta.numbershortgaiadr2_contrib.gaia_source_j2000Source positions at reference J2000 for Gaia data release 2source_idSource IdentifierDimensionlessmeta.id;meta.main;meta.reflongraRight AscensionAngle[deg]pos.eq.radoubledecDeclinationAngle[deg]pos.eq.decdoubleposThe point position of a source (ra, dec) in radiansAngle[rad], Angle[rad]pos.eq.ra;pos.eq.decchargaiadr1Gaia first data release.gaiadr1.gaia_sourceThis table has an entry for every Gaia observed source as listed in the Main Database accumulating catalogue version from which the catalogue release has been generated. It contains the basic source parameters, that is only final data (no epoch data) and no spectra (neither final nor epoch).solution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongrandom_indexRandom index used to select subsetsmeta.codelongref_epochReference epochTime[Julian Years]meta.ref;time.epochdoubleraRight ascensionAngle[deg]pos.eq.ra;meta.maindoublera_errorStandard error of right ascensionAngle[mas]stat.error;pos.eq.radoubledecDeclinationAngle[deg]pos.eq.dec;meta.maindoubledec_errorStandard error of declinationAngle[mas]stat.error;pos.eq.decdoubleparallaxParallaxAngle[mas]pos.parallaxdoubleparallax_errorStandard error of parallaxAngle[mas]stat.error;pos.parallaxdoublepmraProper motion in right ascension directionAngular Velocity[mas/year]pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.radoublepmdecProper motion in declination directionAngular Velocity[mas/year]pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.decdoublera_dec_corrCorrelation between right ascension and declinationstat.correlationfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatastrometric_n_obs_alTotal number of observations ALmeta.numberintastrometric_n_obs_acTotal number of observations ACmeta.numberintastrometric_n_good_obs_alNumber of good observations ALmeta.numberintastrometric_n_good_obs_acNumber of good observations ACmeta.numberintastrometric_n_bad_obs_acNumber of bad observations ACmeta.numberintastrometric_n_bad_obs_alNumber of bad observations ALmeta.numberintastrometric_delta_qHipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)stat.valuefloatastrometric_excess_noiseExcess noise of the sourceAngle[mas]stat.valuedoubleastrometric_excess_noise_sigSignificance of excess noisestat.valuedoubleastrometric_primary_flagPrimary or secondaymeta.codebooleanastrometric_relegation_factorRelegation factorarith.factorfloatastrometric_weight_alMean astrometric weight of the sourceAngle[mas^-2]stat.weight;stat.meanfloatastrometric_weight_acMean astrometric weight of the sourceAngle[mas^-2]stat.weight;stat.meanfloatastrometric_priors_usedType of prior used in the astrometric solutionintmatched_observationsAmount of observations matched to this sourcemeta.numbershortduplicated_sourceSource with duplicate sourcesbooleanscan_direction_strength_k1Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k2Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k3Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k4Degree of concentration of scan directions across the sourcefloatscan_direction_mean_k1Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k2Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k3Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k4Mean position angle of scan directions across the sourceAngle[deg]floatphot_g_n_obsNumber of observations contributing to G photometrymeta.numberintphot_g_mean_fluxG-band mean fluxFlux[e-/s]phot.flux;stat.mean;em.optdoublephot_g_mean_flux_errorError on G-band mean fluxFlux[e-/s]stat.error;phot.flux;stat.mean;em.optdoublephot_g_mean_magG-band mean magnitudeMagnitude[mag]phot.mag;stat.mean;em.optdoublephot_variable_flagPhotometric variability flagmeta.code;src.varcharlGalactic longitudeAngle[deg]pos.galactic.londoublebGalactic latitudeAngle[deg]pos.galactic.latdoubleecl_lonEcliptic longitudeAngle[deg]pos.ecliptic.londoubleecl_latEcliptic latitudeAngle[deg]pos.ecliptic.latdoubleposSpherical point computed from right ascension and declinationchargaiadr1.tgas_sourceThis table is a subset of GaiaSource comprising those stars in the Hipparcos and Tycho-2 Catalogues for which a full 5-parameter astrometric solution has been possible in Gaia Data Release 1. This is possible because the early Hipparcos epoch positions break some degeneracies due to the limited Gaia time coverage. The table contains a substantial fraction of the around 2.5 million stars in the Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to several reasons, such as saturation, cross-match errors or bad astrometric solution.hipHipparcos identifiermeta.id.crossinttycho2_idTycho 2 identifiermeta.id.crosscharsolution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongrandom_indexRandom index used to select subsetsmeta.codelongref_epochReference epochTime[Julian Years]meta.ref;time.epochdoubleraRight ascensionAngle[deg]pos.eq.ra;meta.maindoublera_errorStandard error of right ascensionAngle[mas]stat.error;pos.eq.radoubledecDeclinationAngle[deg]pos.eq.dec;meta.maindoubledec_errorStandard error of declinationAngle[mas]stat.error;pos.eq.decdoubleparallaxParallaxAngle[mas]pos.parallaxdoubleparallax_errorStandard error of parallaxAngle[mas]stat.error;pos.parallaxdoublepmraProper motion in right ascension directionAngular Velocity[mas/year]pos.pm;pos.eq.radoublepmra_errorStandard error of proper motion in right ascension directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.radoublepmdecProper motion in declination directionAngular Velocity[mas/year]pos.pm;pos.eq.decdoublepmdec_errorStandard error of proper motion in declination directionAngular Velocity[mas/year]stat.error;pos.pm;pos.eq.decdoublera_dec_corrCorrelation between right ascension and declinationstat.correlationfloatra_parallax_corrCorrelation between right ascension and parallaxstat.correlationfloatra_pmra_corrCorrelation between right ascension and proper motion in right ascensionstat.correlationfloatra_pmdec_corrCorrelation between right ascension and proper motion in declinationstat.correlationfloatdec_parallax_corrCorrelation between declination and parallaxstat.correlationfloatdec_pmra_corrCorrelation between declination and proper motion in right ascensionstat.correlationfloatdec_pmdec_corrCorrelation between declination and proper motion in declinationstat.correlationfloatparallax_pmra_corrCorrelation between parallax and proper motion in right ascensionstat.correlationfloatparallax_pmdec_corrCorrelation between parallax and proper motion in declinationstat.correlationfloatpmra_pmdec_corrCorrelation between proper motion in right ascension and proper motion in declinationstat.correlationfloatastrometric_n_obs_alTotal number of observations ALmeta.numberintastrometric_n_obs_acTotal number of observations ACmeta.numberintastrometric_n_good_obs_alNumber of good observations ALmeta.numberintastrometric_n_good_obs_acNumber of good observations ACmeta.numberintastrometric_n_bad_obs_acNumber of bad observations ACmeta.numberintastrometric_n_bad_obs_alNumber of bad observations ALmeta.numberintastrometric_delta_qHipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only)stat.valuefloatastrometric_excess_noiseExcess noise of the sourceAngle[mas]stat.valuedoubleastrometric_excess_noise_sigSignificance of excess noisestat.valuedoubleastrometric_primary_flagPrimary or secondaymeta.codebooleanastrometric_relegation_factorRelegation factorarith.factorfloatastrometric_weight_alMean astrometric weight of the sourceAngle[mas^-2]stat.weight;stat.meanfloatastrometric_weight_acMean astrometric weight of the sourceAngle[mas^-2]stat.weight;stat.meanfloatastrometric_priors_usedType of prior used in the astrometric solutionintmatched_observationsAmount of observations matched to this sourcemeta.numbershortduplicated_sourceSource with duplicate sourcesbooleanscan_direction_strength_k1Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k2Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k3Degree of concentration of scan directions across the sourcefloatscan_direction_strength_k4Degree of concentration of scan directions across the sourcefloatscan_direction_mean_k1Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k2Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k3Mean position angle of scan directions across the sourceAngle[deg]floatscan_direction_mean_k4Mean position angle of scan directions across the sourceAngle[deg]floatphot_g_n_obsNumber of observations contributing to G photometrymeta.numberintphot_g_mean_fluxG-band mean fluxFlux[e-/s]phot.flux;stat.mean;em.optdoublephot_g_mean_flux_errorError on G-band mean fluxFlux[e-/s]stat.error;phot.flux;stat.mean;em.optdoublephot_g_mean_magG-band mean magnitudeMagnitude[mag]phot.mag;stat.mean;em.optdoublephot_variable_flagPhotometric variability flagmeta.code;src.varcharlGalactic longitudeAngle[deg]pos.galactic.londoublebdoubleecl_londoubleecl_latdoubleposSpherical point computed from right ascension and declinationchargaiadr1.cepheidThis table describes the Cepheid stars identified in the table variable_summary as "CEP".type_best_classificationBest type classification estimate out of: {"DCEP", "T2CEP", "ACEP"}meta.code.class;src.classchartype2_best_sub_classificationBest subclassification estimate for typeBestClassification="T2CEP" out of: {"BL_HER", "W_VIR","RV_TAU"}meta.code.class;src.classcharmode_best_classificationBest mode classification estimate out of: {"FUNDAMENTAL", "FIRST_OVERTONE", "SECOND_OVERTONE", "UNDEFINED", "NOT_APPLICABLE"}meta.code.class;src.classcharsolution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflonggaiadr1.rrlyraeThis table describes the Cepheid stars identified in the table variable_summary as "RRLYR".best_classificationBest RR Lyrae classification estimate out of: {"RRC", "RRAB"}meta.code.class;src.classcharsolution_idlongsource_idmeta.id;meta.main;meta.reflonggaiadr1.phot_variable_time_series_gfovFOV time series of variable sources.solution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongobservation_timeBarycentric light-travel time corrected timestamp for each FOV observationTime[Barycentric JD in TCB - 2455197.5 (day)]time.epochdoubleg_fluxG-band flux for each FOV observationFlux[e-/s]phot.flux;em.optdoubleg_flux_errorEstimated G-band flux uncertainty for each FOV observationFlux[e-/s]stat.error;phot.flux;em.optdoubleg_magnitudeG-band magnitude for each FOV observationMagnitude[mag]phot.mag;em.optdoublerejected_by_variability_processingTrue when this FOV observation was excluded from variability analysesmeta.codebooleangaiadr1.phot_variable_time_series_gfov_statistical_parametersStatistical parameters of field-of-view time series, incl. only variable sources.solution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongnum_observations_processedNumber of processed G-band observations for variability analysesmeta.numberintmean_obs_timeMean observation time (with respect to T0) of G-band time seriesTime[day]time.epoch;stat.meandoubleminimumMinimum magnitude of the G-band time seriesMagnitude[mag]phot.mag;stat.mindoublemaximumMaximum magnitude of the G-band time seriesMagnitude[mag]phot.mag;stat.maxdoublemeanMean magnitude of the G-band time seriesMagnitude[mag]phot.mag;stat.meandoublemedianMedian magnitude of the G-band time seriesMagnitude[mag]phot.mag;stat.mediandoublerangeDifference between the highest and lowest magnitude of the G-band time seriesMagnitude[mag]phot.mag;arith.diffdoublestd_devSquare root of the unweighted variance of the G-band time series valuesMagnitude[mag]phot.mag;stat.stdevdoubleskewnessStandardized unweighted skewness of the G-band time series valuesstat.valuedoublekurtosisStandardized unweighted kurtosis of the G-band time series valuesstat.valuedoubletime_durationTime duration of the G-band time seriesTime[day]time.durationdoublemedian_absolute_deviationMedian Absolute Deviation (MAD) of the G-band time series valuesMagnitude[mag]phot.mag;stat.valuedoubleabbeAbbe value of the G-band time series valuesstat.valuedoubleiqrInterquartile range of the time series valuesMagnitude[mag]phot.mag;stat.valuedoublegaiadr1.variable_summaryVariability summary of variable sources.solution_idSolution Identifiermeta.id;meta.versionlongsource_idUnique source identifiermeta.id;meta.main;meta.reflongphot_variable_fundam_freq1Fundamental frequency 1Frequency[day^-1]src.var.pulsedoubleclassificationPhotometric variability classification "RRLYR" (RR Lyrae) or "CEP" (Cepheid)meta.code.class;src.varchar