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<ri:Resource created="2022-06-20T07:37:42Z" status="active" updated="2025-12-04T00:00:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Gaia DR3 Part 1. Main source</title><shortName>I/355</shortName><identifier>ivo://CDS.VizieR/I/355</identifier><altIdentifier>doi:10.26093/cds/vizier.1355</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gaia collaboration</name></creator><date role="Updated">2024-12-12T11:51:59Z</date><date role="Created">2022-06-20T07:37:42Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>surveys</subject><subject>standard-stars</subject><subject>astrometry</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>photographic-photometry</subject><subject>astronomical-object-identification</subject><subject>radial-velocity</subject><subject>variable-stars</subject><subject>asteroids</subject><subject>trigonometric-parallax</subject><description>Gaia Data Release 3 (Gaia DR3) will be released on 13 June 2022. The Gaia DR3 catalogue builds upon the Early Data Release 3 (released on 3 December 2020) and combines, for the same stretch of time and the same set of observations, these already-published data products with numerous new data products such as extended objects and non-single stars.</description><source format="bibcode">2023A&amp;A...674A...1G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/I/355</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1: Main sources</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/356">I/356 : Gaia DR3 Part 2: Extra-galactic</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/357">I/357 : Gaia DR3 Part 3: Non-single stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/358">I/358 : Gaia DR3 Part 4: Variability</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/359">I/359 : Gaia DR3 Part 5: Solar System</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/360">I/360 : Gaia DR3 Part 6: Performance verification</relatedResource></relationship><relationship><relationshipType>Cites</relationshipType><relatedResource altIdentifier="doi:10.5270/esa-qa4lep3">Gaia DR3 at ESA: https://doi.org/10.5270/esa-qa4lep3</relatedResource></relationship><relationship><relationshipType>IsVariantFormOf</relationshipType><relatedResource altIdentifier="doi:10.5270/esa-qa4lep3">Gaia DR3 at ESA: 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Correlation between proper motion in right ascension and proper motion in declination (pmra_pmdec_corr)</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NAL</name><description>Total number of observations in the along-scan (AL) direction (astrometric_n_obs_al)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>DR3Name</name><description>Unique source designation (unique across all Data Releases) (designation)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RandomI</name><description>Random index for use when selecting subsets (random_index)</description><ucd>meta.code</ucd><flag>indexed</flag></column><column><name>e_RA_ICRS</name><description>Standard error of right ascension (ra_error)</description><unit>mas</unit><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DE_ICRS</name><description>Standard error of declination (dec_error)</description><unit>mas</unit><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Plx</name><description>? 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Proper motion in right ascension direction, pmRA*cosDE (pmra)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_pmRA</name><description>? Standard error of proper motion in right ascension direction (pmra_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmDE</name><description>? Proper motion in declination direction (pmdec)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_pmDE</name><description>? Standard error of proper motion in declination direction (pmdec_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RADEcor</name><description>[-1/1] Correlation between right ascension and declination (ra_dec_corr)</description><ucd>stat.correlation</ucd></column><column><name>RAPlxcor</name><description>[-1/1]? Correlation between right ascension and parallax (ra_parallax_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>RApmRAcor</name><description>[-1/1]? Correlation between right ascension and proper motion in right ascension (ra_pmra_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>RApmDEcor</name><description>[-1/1]? Correlation between right ascension and proper motion in declination (ra_pmdec_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>DEPlxcor</name><description>[-1/1]? Correlation between declination and parallax (dec_parallax_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>DEpmRAcor</name><description>[-1/1]? Correlation between declination and proper motion in right ascension (dec_pmra_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>DEpmDEcor</name><description>[-1/1]? Correlation between declination and proper motion in declination (dec_pmdec_corr)</description><ucd>stat.correlation</ucd><flag>nullable</flag></column><column><name>PlxpmRAcor</name><description>[-1/1]? Correlation between parallax and proper motion in right ascension (parallax_pmra_corr)</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PlxpmDEcor</name><description>[-1/1]? Correlation between parallax and proper motion in declination (parallax_pmdec_corr)</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NAC</name><description>Total number of observations in the across-scan (AC) direction (astrometric_n_obs_ac)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NgAL</name><description>Number of good observations in the along-scan (AL) direction (astrometric_n_good_obs_al)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NbAL</name><description>Number of bad observations in the along-scan (AL) direction (astrometric_n_bad_obs_al)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>gofAL</name><description>Goodness of fit statistic of model wrt along-scan observations (astrometric_gof_al)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>chi2AL</name><description>AL chi-square value (astrometric_chi2_al)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>epsi</name><description>Excess noise of the source (astrometric_excess_noise)</description><unit>mas</unit><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>sepsi</name><description>Significance of excess noise (astrometric_excess_noise_sig)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Solved</name><description>[3/95] Which parameters have been solved for? (astrometric_params_solved) (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>APF</name><description>[0/1] Primary or secondary (astrometric_primary_flag)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nueff</name><description>? Effective wavenumber of the source used in the astrometric solution (nu_eff_used_in_astrometry)</description><unit>um**-1</unit><ucd>em.wavenumber</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pscol</name><description>? Astrometrically estimated pseudocolour of the source (pseudocolour)</description><unit>um**-1</unit><ucd>em.wavenumber</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pscol</name><description>? Standard error of the pseudocolour of the source (pseudocolour_error)</description><unit>um**-1</unit><ucd>stat.error;em.wavenumber</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RApscolCorr</name><description>[-1/1]? Correlation between right ascension and pseudocolour (ra_pseudocolour_corr)</description><ucd>stat.correlation;em.wavenumber;pos.eq.ra</ucd><flag>nullable</flag></column><column><name>DEpscolCorr</name><description>[-1/1]? Correlation between declination and pseudocolour (dec_pseudocolour_corr)</description><ucd>stat.correlation;em.wavenumber;pos.eq.dec</ucd><flag>nullable</flag></column><column><name>PlxpscolCorr</name><description>[-1/1]? Correlation between parallax and pseudocolour (parallax_pseudocolour_corr)</description><ucd>stat.correlation;em.wavenumber;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmRApscolCorr</name><description>[-1/1]? Correlation between proper motion in right ascension and pseudocolour (pmra_pseudocolour_corr)</description><ucd>stat.correlation;em.wavenumber;pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pmDEpscolCorr</name><description>[-1/1]? Correlation between proper motion in declination and pseudocolour (pmdec_pseudocolour_corr)</description><ucd>stat.correlation;em.wavenumber;pos.pm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MatchObsA</name><description>Matched FOV transits used in the AGIS solution (astrometric_matched_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nper</name><description>[1/33] Number of visibility periods used in Astrometric solution (visibility_periods_used)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>amax</name><description>The longest semi-major axis of the -2- -7 error ellipsoid (astrometric_sigma5d_max)</description><unit>mas</unit><ucd>stat;pos.errorEllipse</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MatchObs</name><description>The number of transits matched to this source (matched_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NewMatchObs</name><description>The number of transits newly incorporated into an existing source in the current cycle (new_matched_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MatchObsrm</name><description>The number of transits removed from an existing source in the current cycle (matched_transits_removed)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IPDgofha</name><description>Amplitude of the IPD GoF versus position angle of scan (ipd_gof_harmonic_amplitude)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IPDgofhp</name><description>Phase of the IPD GoF versus position angle of scan (ipd_gof_harmonic_phase)</description><unit>deg</unit><ucd>pos.posAng;stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>IPDfmp</name><description>[0/100] Percent of successful-IPD windows with more than one peak (ipd_frac_multi_peak)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>IPDfow</name><description>[0/100] Percent of transits with truncated windows or multiple gate (ipd_frac_odd_win)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RUWE</name><description>? Renormalised unit weight error (ruwe)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SDSk1</name><description>? Degree of concentration of scan directions across the source (scan_direction_strength_k1)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SDSk2</name><description>? Degree of concentration of scan directions across the source (scan_direction_strength_k2)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SDSk3</name><description>? Degree of concentration of scan directions across the source (scan_direction_strength_k3)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SDSk4</name><description>? Degree of concentration of scan directions across the source (scan_direction_strength_k4)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SDMk1</name><description>? Mean position angle of scan directions across the source (scan_direction_mean_k1)</description><ucd>pos.posAng;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SDMk2</name><description>? Mean position angle of scan directions across the source (scan_direction_mean_k2)</description><ucd>pos.posAng;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SDMk3</name><description>? Mean position angle of scan directions across the source (scan_direction_mean_k3)</description><ucd>pos.posAng;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SDMk4</name><description>? Mean position angle of scan directions across the source (scan_direction_mean_k4)</description><unit>deg</unit><ucd>pos.posAng;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dup</name><description>[0/1] Source with multiple source identifiers (duplicated_source)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>o_Gmag</name><description>Number of observations contributing to G photometry (phot_g_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FG</name><description>? G-band mean flux (phot_g_mean_flux)</description><ucd>phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FG</name><description>? Error on G-band mean flux (phot_g_mean_flux_error)</description><ucd>stat.error;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFG</name><description>? G-band mean flux divided by its error (phot_g_mean_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>? G-band mean magnitude (phot_g_mean_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_FBP</name><description>? Error on the integrated BP mean flux (phot_bp_mean_flux_error)</description><ucd>stat.error;phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFBP</name><description>? Integrated BP mean flux divided by its error (phot_bp_mean_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPmag</name><description>? Integrated BP mean magnitude (phot_bp_mean_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_BPmag</name><description>? Error on integrated BP mean magnitude (added by CDS) (phot_bp_mean_mag_error)</description><unit>mag</unit><ucd>stat.error;phot.mag;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>o_RPmag</name><description>Number of observations contributing to RP photometry (phot_rp_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FRP</name><description>? Integrated RP mean flux (phot_rp_mean_flux)</description><ucd>phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FRP</name><description>? Error on the integrated RP mean flux (phot_rp_mean_flux_error)</description><ucd>stat.error;phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFRP</name><description>? Integrated RP mean flux divided by its error (phot_rp_mean_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPmag</name><description>? Integrated RP mean magnitude (phot_rp_mean_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_RPmag</name><description>? Error on integrated RP mean magnitude (added by CDS) (phot_rp_mean_mag_error)</description><unit>mag</unit><ucd>stat.error;phot.mag;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E(BP/RP)</name><description>? BP/RP excess factor (phot_bp_rp_excess_factor)</description><unit>mag</unit><ucd>arith.factor;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NBPcont</name><description>? Number of BP contaminated transits (phot_bp_n_contaminated_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NBPblend</name><description>? Number of BP blended transits (phot_bp_n_blended_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NRPcont</name><description>? Number of RP contaminated transits (phot_rp_n_contaminated_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NRPblend</name><description>? Number of RP contaminated transits (phot_rp_n_blended_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mode</name><description>[0/2]? Photometry processing mode (phot_proc_mode)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BP-RP</name><description>? BP-RP colour (bp_rp)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>BP-G</name><description>? BP-G colour (bp_g)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>G-RP</name><description>? G-RP colour (g_rp)</description><unit>mag</unit><ucd>phot.color;em.opt;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>RV</name><description>? Radial velocity (radial_velocity)</description><unit>km/s</unit><ucd>spect.dopplerVeloc.opt;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>e_RV</name><description>? Radial velocity error (radial_velocity_error)</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc.opt;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_RV</name><description>[0/2]? Method used to obtain the radial velocity (rv_method_used)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_RV</name><description>? Number of transits used to compute the radial velocity (rv_nb_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>o_RVd</name><description>? Number of valid transits that have undergone deblending (rv_nb_deblended_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RVNper</name><description>[0/33]? Number of visibility periods used to estimate the radial velocity (rv_visibility_periods_used)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RVS/N</name><description>? Expected signal to noise ratio in the combination of the spectra used to obtain the radial velocity (rv_expected_sig_to_noise)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RVgof</name><description>? Radial velocity renormalised goodness of fit (rv_renormalised_gof)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RVchi2</name><description>? P-value for constancy based on a chi-squared criterion (rv_chisq_pvalue)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RVTdur</name><description>? Time coverage of the radial velocity time series (rv_time_duration)</description><unit>d</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RVamp</name><description>? Total amplitude in the radial velocity time series after outlier removal (rv_amplitude_robust)</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc.opt;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RVtempTeff</name><description>? Teff of the template used to compute the radial velocity (rv_template_teff)</description><unit>K</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RVtemplogg</name><description>? Logg of the template used to compute the radial velocity (rv_template_logg)</description><unit>log(cm.s**-2)</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RVtemp[Fe/H]</name><description>? [Fe/H] of the template used to compute the radial velocity (rv_template_fe_h)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vatmparam</name><description>? Origin of the atmospheric parameters associated to the template (rv_atm_param_origin)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vbroad</name><description>? Spectral line broadening parameter (vbroad)</description><unit>km/s</unit><ucd>spect.dopplerVeloc.opt;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Vbroad</name><description>? Uncertainty on the spectral line broadening (vbroad_error)</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc.opt;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>o_Vbroad</name><description>? Number of transits used to compute vbroad (vbroad_nb_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GRVSmag</name><description>? Integrated Grvs magnitude (grvs_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GRVSmag</name><description>? Grvs magnitude uncertainty (grvs_mag_error)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>o_GRVSmag</name><description>? Number of transits used to compute Grvs (grvs_mag_nb_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RVSS/N</name><description>? Signal to noise ratio in the mean RVS spectrum (rvs_spec_sig_to_noise)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VarFlag</name><description>Photometric variability flag (phot_variable_flag)</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>GLON</name><description>Galactic longitude (l)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><flag>indexed</flag></column><column><name>GLAT</name><description>Galactic latitude (b)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>indexed</flag></column><column><name>ELON</name><description>Ecliptic longitude (ecl_lon)</description><unit>deg</unit><ucd>pos.ecliptic.lon</ucd></column><column><name>ELAT</name><description>Ecliptic latitude (ecl_lat)</description><unit>deg</unit><ucd>pos.ecliptic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>QSO</name><description>[0/1] Flag indicating the availability of additional information in the QSO candidates table (in_qso_candidates)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Gal</name><description>[0/1] Flag indicating the availability of additional information in the galaxy candidates table (in_galaxy_candidates)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NSS</name><description>[0/7] Flag indicating the availability of additional information in the various Non-Single Star tables (non_single_star)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>XPcont</name><description>[0/1] Flag indicating the availability of mean BP/RP spectrum in continuous representation for this source (has_xp_continuous)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>XPsamp</name><description>[0/1] Flag indicating the availability of mean BP/RP spectrum in sampled form for this source (has_xp_sampled)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RVS</name><description>[0/1] Flag indicating the availability of mean RVS spectrum for this source (has_rvs)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EpochPh</name><description>[0/1] Flag indicating the availability of epoch photometry for this source (has_epoch_photometry)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>URAT1</name><description>URAT1 name, Zacharias et al., Cat. I/329 (urat1_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType><flag>indexed</flag></column><column><name>EpochRV</name><description>[0/1] Flag indicating the availability of epoch radial velocity for this source (has_epoch_rv)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MCMCGSP</name><description>[0/1] Flag indicating the availability of GSP-Phot MCMC samples for this source (has_mcmc_gspphot)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MCMCMSC</name><description>[0/1] Flag indicating the availability of MSC MCMC samples for this source (has_mcmc_msc)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>And</name><description>[0/1] Flag indicating that the source is present in the Gaia Andromeda Photometric Survey (GAPS) (in_andromeda_survey)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PQSO</name><description>? Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_combmod_quasar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PGal</name><description>? Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PSS</name><description>? Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_combmod_star)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff</name><description>? Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Teff</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Teff</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg</name><description>? Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>? Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Fe/H]</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Fe/H]</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)</description><unit>pc</unit><ucd>pos.distance;pos.eq</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower)</description><unit>pc</unit><ucd>pos.distance;pos.eq</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper)</description><unit>pc</unit><ucd>pos.distance;pos.eq</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0</name><description>? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0</name><description>? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0</name><description>? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG</name><description>? Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)</name><description>? Reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)</name><description>? Lower confidence level (16%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower)</description><unit>mag</unit><ucd>phot.color.excess;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)</name><description>? Upper confidence level (84%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper)</description><unit>mag</unit><ucd>phot.color.excess;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lib</name><description>Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table (libname_gspphot)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>mGSC23</name><description>? Number of mates in Gaia Catalog (gsc23_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>HIP</name><description>? HIP cross-id number, van Leeuwen, Cat. I/311 (hip_original_ext_source_id)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>dHIP</name><description>? Angular distance between the two sources (hip_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>nHIP</name><description>[0/3]? Number of neighbours in HIP (hip_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_HIP</name><description>[0/72]? Cross-match algorithm flag (hip_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PS1coid</name><description>? PS1 cross-id original name (clean_panstarrs1_oid)</description><ucd>meta.id.cross</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>PS1</name><description>? PS1 cross-id name, Chambers et al., Cat. II/349 (ps1_original_ext_source_id)</description><ucd>meta.id.cross</ucd><flag>nullable</flag></column><column><name>dPS1</name><description>? Angular Distance between the two sources (ps1_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>nPS1</name><description>[0/76]? Number of neighbours in PS1 (ps1_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mPS1</name><description>? Number of mates in Gaia Catalog (ps1_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_PS1</name><description>[0/76]? Cross-match algorithm flag (ps1_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SDSS13coid</name><description>? SDSS cross-id original name (clean_sdssdr13_oid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>SDSS13</name><description>? SDSS name, Albareti et al., 2017ApJS..233...25A (sdss13_ext_source_id)</description><ucd>meta.id.cross</ucd><flag>nullable</flag></column><column><name>dSDSS13</name><description>? Angular Distance between the two sources (sdss13_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>nSDSS13</name><description>[0/6]? Number of neighbours in SDSS13 (sdss13_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mSDSS13</name><description>[0/6]? Number of mates in Gaia Catalog (sdss13_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_SDSS13</name><description>[0/76]? Cross-match algorithm flag (sdss13_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SKYM2</name><description>? SkyMapperDR2 cross-id name, Onken et al., 2019PASA...36...33O (skym2_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>dSKYM2</name><description>? Angular Distance between the two sources (skym2_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>nSKYM2</name><description>[0/4]? Number of neighbours in SKYM2 (skym2_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mSKYM2</name><description>? Number of mates in Gaia Catalog (skym2_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_SKYM2</name><description>[0/72]? Cross-match algorithm flag (skym2_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TYC2</name><description>Tycho-2 cross-id name, Hog et al., Cat. I/259 (tyc2_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>indexed</flag></column><column><name>dTYC2</name><description>? Angular Distance between the two source (tyc2_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_TYC2</name><description>[0/72]? Cross-match algorithm flag (tyc2_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TYC2moid</name><description>? Tycho-2 cross-id original name (tycho2tdsc_merge_oid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nTYC2</name><description>[0/4]? Number of neighbours in TYC2 (tyc2_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>dURAT1</name><description>? Angular Distance between the two sources (urat1_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_URAT1</name><description>[0/72]? Cross-match algorithm flag (urat1_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>nURAT1</name><description>[0/4]? Number of neighbours in URAT1 (urat1_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mURAT1</name><description>[0/4]? Number of mates in Gaia Catalog (urat1_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AllWISE</name><description>ALLWISE cross-id name, Cutri et al., Cat. II/328 (allwise_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType><flag>indexed</flag></column><column><name>dAllWISE</name><description>? Angular Distance between the two sources (allwise_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_AllWISE</name><description>[0/72]? Cross-match algorithm flag (allwise_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>AllWISEoid</name><description>? ALLWISE identification number (allwise_oid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>nAllWISE</name><description>[0/3]? Number of neighbours in ALLWISE catalog (allwise_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mAllWISE</name><description>? Number of mates in Gaia Catalog (allwise_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>APASS9coid</name><description>? APASS9 cross-id original identification number (clean_apassdr9_oid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>APASS9</name><description>? APASS9 identification, Henden et al., Cat. II/336 (apass9_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag><flag>indexed</flag></column><column><name>dAPASS9</name><description>? Angular Distance between the two sources (apass9_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>nAPASS9</name><description>? Number of neighbours in APASS9 (apass9_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>mAPASS9</name><description>? Number of mates in Gaia Catalog (apass9_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_APASS9</name><description>[0/74]? Cross-match algorithm flag (apass9_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GSC23</name><description>GSC2.3 cross-id name, Lasker et al., Cat. I/305 (gsc23_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>indexed</flag></column><column><name>dGSC23</name><description>? Angular Distance between the two sources (gsc23_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_GSC23</name><description>? Cross-match algorithm flag (gsc23_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>GSC23coid</name><description>? GSC2.3 cross-id original name (clean_gsc23_oid)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">long</dataType><flag>nullable</flag></column><column><name>nGSC23</name><description>[0/16]? Number of neighbours in GSC23 (gsc23_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAVE5</name><description>RAVE DR5 cross-id name, Kunder et al., Cat. III/279 (rave5_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType><flag>indexed</flag></column><column><name>dRAVE5</name><description>? Angular Distance between the two sources (rave5_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_RAVE5</name><description>[0/72]? Cross-match algorithm flag (rave5_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAVE5coid</name><description>? RAVE DR5 cross-id original name (clean_ravedr5_oid)</description><ucd>meta.id.cross</ucd><flag>nullable</flag></column><column><name>nRAVE5</name><description>[0/3]? Number of neighbours in RAVE5 (rave5_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>2MASS</name><description>2MASS cross-id name, Cutri et al., Cat. II/246 (twomass_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType><flag>indexed</flag></column><column><name>m2MASS</name><description>[0/13]? Number of mates in Gaia Catalog (twomass_number_of_mates)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAVE6</name><description>RAVE DR6 cross-id name, Steinmetz et al., Cat. III/283 (rave6_original_ext_source_id)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType><flag>indexed</flag></column><column><name>dRAVE6</name><description>? Angular Distance between the two sources (rave6_angular_distance)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_RAVE6</name><description>[0/72]? Cross-match algorithm flag (rave6_xm_flag)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAVE6oid</name><description>? RAVE DR6 original name (ravedr6_oid)</description><ucd>meta.id.cross</ucd><flag>nullable</flag></column><column><name>nRAVE6</name><description>[0/3]? Number of neighbours in RAVE6 (rave6_number_of_neighbours)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Barycentric right ascension (ICRS) at Ep=2000.0 (added by CDS) (ra2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Barycentric declination (ICRS) at Ep=2000.0 (added by CDS) (dec2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>e_RAJ2000</name><description>Standard error of right ascension (e_RA*cosDE) (added by CDS) (ra2000_error)</description><unit>mas</unit><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DEJ2000</name><description>Standard error of declination (added by CDS) (dec2000_error)</description><unit>mas</unit><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RADEcorJ2000</name><description>[-1/1] Correlation between right ascension and declination at epoch 2000 (added by CDS) (ra2000_de2000_corr)</description><ucd>stat.correlation;pos.eq.ra;pos.eq.dec</ucd></column></table><table><name>I/355/paramp</name><description>1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8 (1590932717 sources) (astrophysical_parameters)</description><column><name>Source</name><description>Source Identifier (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>PQSO</name><description>? Probability from DSC-Combmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_combmod_quasar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PGal</name><description>? Probability from DSC-Combmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_combmod_galaxy)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pstar</name><description>? Probability from DSC-Combmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_combmod_star)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PWD</name><description>? Probability from DSC-Combmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_combmod_whitedwarf)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pbin</name><description>? Probability from DSC-Combmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_combmod_binarystar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PQSO-S</name><description>? Probability from DSC-Specmod of being a quasar (data used: BP/RP spectrum) (classprob_dsc_specmod_quasar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pgal-S</name><description>? Probability from DSC-Specmod of being a galaxy (data used: BP/RP spectrum) (classprob_dsc_specmod_galaxy)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAG</name><description>? Absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pstar-S</name><description>? Probability from DSC-Specmod of being a single star (but not a white dwarf) (data used: BP/RP spectrum) (classprob_dsc_specmod_star)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PWD-S</name><description>? Probability from DSC-Specmod of being a white dwarf (data used: BP/RP spectrum) (classprob_dsc_specmod_whitedwarf)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pbin-S</name><description>? Probability from DSC-Specmod of being a binary star (data used: BP/RP spectrum) (classprob_dsc_specmod_binarystar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PQSO-A</name><description>? Probability from DSC-Allosmod of being a quasar (data used: photometry) (classprob_dsc_allosmod_quasar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PGal-A</name><description>? Probability from DSC-Allosmod of being a galaxy (data used: photometry) (classprob_dsc_allosmod_galaxy)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pstar-A</name><description>? Probability from DSC-Allosmod of being a star (data used: photometry) (classprob_dsc_allosmod_star)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff</name><description>? Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower)</description><unit>K</unit><ucd>stat.value;phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper)</description><unit>K</unit><ucd>stat.value;phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg</name><description>? Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (logg_gspphot_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>? Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Fe/H]</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Fe/H]</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra (mh_gspphot_upper)</description><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0</name><description>? Monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0</name><description>? Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0</name><description>? Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from GSP-Phot Aeneas best library using BP/RP spectra (azero_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG</name><description>? Extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ABP</name><description>? Extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ABP</name><description>? Lower confidence level (16%) of extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ABP</name><description>? Upper confidence level (84%) of extinction in G_BP_ band from GSP-Phot Aeneas best library using BP/RP spectra (abp_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ARP</name><description>? Extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ARP</name><description>? Lower confidence level (16%) of extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ARP</name><description>? Upper confidence level (84%) of extinction in G_RP_ band from GSP-Phot Aeneas best library using BP/RP spectra (arp_gspphot_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)</name><description>? Reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)</description><unit>mag</unit><ucd>stat.value;phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)</name><description>? Lower confidence level (16%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)</name><description>? Upper confidence level (84%) of reddening E(G_BP_-G_RP_) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_GMAG</name><description>? Lower confidence level (16%) of absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_lower)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_GMAG</name><description>? Upper confidence level (84%) of absolute magnitude M_G_ from GSP-Phot Aeneas best library using BP/RP spectra (mg_gspphot_upper)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad</name><description>? Radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad</name><description>? Lower confidence level (16%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad</name><description>? Upper confidence level (84%) of radius from GSP-Phot Aeneas best library using BP/RP spectra (radius_gspphot_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logpost</name><description>? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC best library (logposterior_gspphot)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp</name><description>? MCMC acceptance rate of GSP-Phot Aeneas MCMC best library (mcmcaccept_gspphot)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lib</name><description>Name of library that achieves the highest mean log-posterior in MCMC samples and was used to derive GSP-Phot parameters in this table (libname_gspphot)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Teff-S</name><description>? Effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec)</description><unit>K</unit><ucd>phys.temperature.effective;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Teff-S</name><description>? 16th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Teff-S</name><description>? 84th percentile of effective temperature from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (teff_gspspec_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg-S</name><description>? Logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg-S</name><description>? 16th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg-S</name><description>? 84th percentile of the logarithm of the stellar surface gravity from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (logg_gspspec_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]-S</name><description>? Global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec)</description><ucd>phys.abund.Fe;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]-S</name><description>? 16th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]-S</name><description>? 84th percentile of global metallicity [M/H] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mh_gspspec_upper)</description><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[alpha/Fe]-S</name><description>? Abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec)</description><ucd>phys.abund;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>s_[Ti/Fe]-S</name><description>? Uncertainty estimation of [Ti/Fe] abundance using N lines of the element (tife_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[alpha/Fe]-S</name><description>? 16th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_lower)</description><ucd>phys.abund;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[alpha/Fe]-S</name><description>? 84th percentile of the abundance of alpha-elements [alpha/Fe] with respect to iron from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (alphafe_gspspec_upper)</description><ucd>phys.abund;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]-S</name><description>? Abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec)</description><ucd>phys.abund.Fe;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Fe/H]-S</name><description>? 16th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Fe/H]-S</name><description>? 84th percentile of the abundance of neutral iron [Fe/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (fem_gspspec_upper)</description><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[Fe/H]-S</name><description>[0/8]? Number of lines used for [Fe/M] abundance estimation (fem_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[Fe/H]-S</name><description>? Uncertainty estimation of [Fe/M] abundance using N lines of the element (fem_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/Fe]-S</name><description>? Abundance of Silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Si/Fe]-S</name><description>? 16th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Si/Fe]-S</name><description>? 84th percentile of the abundance of silicon [Si/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sife_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[Si/Fe]-S</name><description>[0/3]? Number of lines used for [Si/Fe] abundance estimation (sife_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[Si/Fe]-S</name><description>? Uncertainty estimation of [Si/Fe] abundance using N lines of the element (sife_gspspec_linescatter)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ca/Fe]-S</name><description>? Abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Ca/Fe]-S</name><description>? 16th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Ca/Fe]-S</name><description>? 84th percentile of the abundance of Calcium [Ca/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cafe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[Ca/Fe]-S</name><description>[0/7]? Number of lines used for [Ca/Fe] abundance estimation (cafe_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[Ca/Fe]-S</name><description>? Uncertainty estimation of [Ca/Fe] abundance using N lines of the element (cafe_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ti/Fe]-S</name><description>? Abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Ti/Fe]-S</name><description>? 16th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Ti/Fe]-S</name><description>? 84th percentile of the abundance of Titanium [Ti/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (tife_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[Ti/Fe]-S</name><description>[0/3]? Number of lines used for [Ti/Fe] abundance estimation (tife_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Flags</name><description>? Catalogue flags for GSP-Spec MatisseGauguin (flags_gspspec) (1)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType" arraysize="41*">char</dataType></column><column><name>[Mg/Fe]-S</name><description>? Abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Mg/Fe]-S</name><description>? 16th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Mg/Fe]-S</name><description>? 84th percentile of the abundance of Magnesium [Mg/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (mgfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Nd/Fe]-S</name><description>? Abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Nd/Fe]-S</name><description>? 16th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Nd/Fe]-S</name><description>? 84th percentile of the abundance of neodymium [Nd/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (ndfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[FeII/M]-S</name><description>? Abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec)</description><ucd>phys.abund.Fe;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[FeII/M]-S</name><description>? 16th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[FeII/M]-S</name><description>? 84th percentile of the abundance of ionised iron [FeII/M] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (feiim_gspspec_upper)</description><ucd>phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[S/Fe]-S</name><description>? Abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[S/Fe]-S</name><description>? 16th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[S/Fe]-S</name><description>? 84th percentile of the abundance of Sulphur [S/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (sfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[S/Fe]-S</name><description>[0/2]? Number of lines used for [S/Fe] abundance estimation (sfe_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[S/Fe]-S</name><description>? Uncertainty estimation of [S/Fe] abundance using N lines of the element (sfe_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Zr/Fe]-S</name><description>? Abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Zr/Fe]-S</name><description>? 16th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Zr/Fe]-S</name><description>? 84th percentile of the abundance of Zirconium [Zr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (zrfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[N/Fe]-S</name><description>? Abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[N/Fe]-S</name><description>? 16th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[N/Fe]-S</name><description>? 84th percentile of the abundance of Nitrogen [N/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[N/Fe]-S</name><description>[0/2]? Number of lines used for [N/Fe] abundance estimation (nfe_gspspec_nlines)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[N/Fe]-S</name><description>? Uncertainty estimation of [N/Fe] abundance using N lines of the element (nfe_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Cr/Fe]-S</name><description>? Abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Cr/Fe]-S</name><description>? 16th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Cr/Fe]-S</name><description>? 84th percentile of the abundance of Chromium [Cr/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (crfe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_[Cr/Fe]-S</name><description>[0/2]? Number of lines used for [Cr/Fe] abundance estimation (crfe_gspspec_nlines)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>s_[Cr/Fe]-S</name><description>? Uncertainty estimation of [Cr/Fe] abundance using N lines of the element (crfe_gspspec_linescatter)</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ce/Fe]-S</name><description>? Abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Ce/Fe]-S</name><description>? 16th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Ce/Fe]-S</name><description>? 84th percentile of the abundance of Cerium [Ce/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (cefe_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Ni/Fe]-S</name><description>? Abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec)</description><ucd>phys.abund.Z;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[Ni/Fe]-S</name><description>? 16th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_lower)</description><ucd>phys.abund.Z;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[Ni/Fe]-S</name><description>? 84th percentile of the abundance of Nickel [Ni/Fe] from GSP-Spec MatisseGauguin using RVS spectra and Monte Carlo realisations (nife_gspspec_upper)</description><ucd>phys.abund.Z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWCN0</name><description>? Equivalent width of cyoanogen line (cn0ew_gspspec)</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EWCN0</name><description>? Uncertainty of equivalent width of cyanogen absorption line (cn0ew_gspspec_uncertainty)</description><unit>nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CN0</name><description>? Central wavelength of cyanogen line (cn0_gspspec_centralline)</description><unit>nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CN0W</name><description>? Width of cyoanogen line (cn0_gspspec_width)</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DIB</name><description>? DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda)</description><unit>nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DIB</name><description>? Uncertainty on DIB central wavelength from GSP-Spec MatisseGauguin using RVS spectra (dib_gspspec_lambda_uncertainty)</description><unit>nm</unit><ucd>stat.error;em.wl.central</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWDIB</name><description>? Equivalent width of the DIB from GSP-Spec MatisseGauguin using RVS spectra (dibew_gspspec)</description><unit>0.1nm</unit><ucd>stat.value;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EWDIB</name><description>? Global uncertainty on DIB equivalent width value using DIB algorithm (dibew_gspspec_uncertainty)</description><unit>0.1nm</unit><ucd>stat.value;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>s_EWDIB</name><description>? Uncertainty on DIB equivalent width value occuring from noise part (dibewnoise_gspspec_uncertainty)</description><unit>0.1nm</unit><ucd>stat.value;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DIBp0</name><description>? Depth (p_0 parameter) of the DIB derived from a Gaussian model fit (dibp0_gspspec)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DIBp2</name><description>? Width (p_2 parameter) of the DIB derived from a Gaussian model fit (dibp2_gspspec)</description><unit>0.1nm</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_DIBp2</name><description>? Uncertainty on the dibp2Gspspec parameter (dibp2_gspspec_uncertainty)</description><unit>0.1nm</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>q_DIB</name><description>[-2/5]? Quality flag of the DIB computation (dibqf_gspspec)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>chi2</name><description>? Logarithm of the goodness-of-fit for the GSP-Spec MatisseGauguin parameters (logchisq_gspspec)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EWHa</name><description>? Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha)</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EWHa</name><description>? Uncertainty of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_uncertainty)</description><unit>nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>f_EWHa</name><description>[0/9]? Quality flag of the Halpha pseudo-equivalent width from ESP-ELS (ew_espels_halpha_flag)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EWHamod</name><description>? Halpha pseudo-equivalent width from ESP-ELS measured on the synthetic spectrum (ew_espels_halpha_model)</description><unit>nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>ClassELS</name><description>Adopted ELS class label from ESP-ELS (classlabel_espels)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>f_ClassELS</name><description>? Quality flag of the adopted ELS class label from ESP-ELS (classlabel_espels_flag)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>PWC</name><description>? Probability from ESP-ELS of being a Wolf-Rayet star of type WC (classprob_espels_wcstar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PWN</name><description>? Probability from ESP-ELS of being a Wolf-Rayet star of type WN (classprob_espels_wnstar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PBe</name><description>? Probability from ESP-ELS of being a Be Star (classprob_espels_bestar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PTTau</name><description>? Probability from ESP-ELS of being a T Tauri Star (classprob_espels_ttauristar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PHAe/Be</name><description>? Probability from ESP-ELS of being a Herbig Ae/Be Star (classprob_espels_herbigstar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PdMactive</name><description>? Probability from ESP-ELS of being an active M dwarf Star (classprob_espels_dmestar)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>PPN</name><description>? Probability from ESP-ELS of being a planetary nebula (classprob_espels_pne)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0-HS</name><description>? Monochromatic interstellar extinction (azero_esphs)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A0-HS</name><description>? Uncertainty at a 68% confidence level on A_0_ from ESP-HS (azero_esphs_uncertainty)</description><unit>mag</unit><ucd>stat.error;phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG-HS</name><description>? Intersterstellar extinction in G band from ESP-HS (ag_esphs)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_AG-HS</name><description>? Uncertainty on A_G_ from ESP-HS (ag_esphs_uncertainty)</description><unit>mag</unit><ucd>stat.error;phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)-HS</name><description>? Reddening E(G_BP_-G_RP_) from ESP-HS (ebpminrp_esphs)</description><unit>mag</unit><ucd>phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_E(BP-RP)-HS</name><description>? Uncertainty on E(G_BP_-G_RP_) from ESP-HS (ebpminrp_esphs_uncertainty)</description><unit>mag</unit><ucd>stat.error;phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Teff-HS</name><description>? Effective temperature from ESP-HS (teff_esphs)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Teff-HS</name><description>? Uncertainty at a 68% confidence level on the effective temperature from ESP-HS (teff_esphs_uncertainty)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg-HS</name><description>? Surface gravity from ESP-HS (logg_esphs)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logg-HS</name><description>? Uncertainty at a 68% confidence level on the surface gravity from ESP-HS (logg_esphs_uncertainty)</description><unit>log(cm.s**-2)</unit><ucd>stat.error;phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>vsini-HS</name><description>? Projected rotational velocity from ESP-HS (vsini_esphs)</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vsini-HS</name><description>? Uncertainty on the projected rotational velocity from ESP-HS (vsini_esphs_uncertainty)</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flags-HS</name><description>? Quality flag of the ESP-HS parametrisation (flags_esphs) (2)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SpType-ELS</name><description>Spectral type from ESP-ELS (spectraltype_esphs)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>CA-CS</name><description>? Chromospheric activity index from ESP-CS (activityindex_espcs)</description><unit>nm</unit><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_CA-CS</name><description>? Uncertainty in the chromospheric activity index from ESP-CS (activityindex_espcs_uncertainty)</description><unit>nm</unit><ucd>stat.error;spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>n_CA-CS</name><description>[12M] Source of input stellar parameters for the computation of the activity index by ESP-CS (activityindex_espcs_input)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Teff-UCD</name><description>? Effective temperature estimate from ESP-UCD based on the RP spectrum (teff_espucd)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Teff-UCD</name><description>? Uncertainty of the effective temperature estimate produced by ESP-UCD (teff_espucd_uncertainty)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flags-UCD</name><description>[0/21]? Quality flags of the ESP-UCD parameter estimates (flags_espucd) (3)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Rad-Flame</name><description>? Radius of the star from FLAME using teff_gspphot and lum_flame (radius_flame)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad-Flame</name><description>? Lower confidence level (16%) of radiusFlame (radius_flame_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad-Flame</name><description>? Upper confidence level (84%) of radiusFlame (radius_flame_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lum-Flame</name><description>? Luminosity of the star from FLAME using G band magnitude, extinction (ag_gspphot), parallax or distance, and a bolometric correction bc_flame (lum_flame)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Lum-Flame</name><description>? Lower confidence level (16%) of lumFlame (lum_flame_lower)</description><unit>solLum</unit><ucd>phys.luminosity;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Lum-Flame</name><description>? Upper confidence level (84%) of lumFlame (lum_flame_upper)</description><unit>solLum</unit><ucd>phys.luminosity;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mass-Flame</name><description>? Mass of the star from FLAME using stellar models, lum_flame, and teff_gspphot (mass_flame)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Mass-Flame</name><description>? Lower confidence level (16%) of mass of the star from FLAME (mass_flame_lower)</description><unit>solMass</unit><ucd>phys.mass;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Mass-Flame</name><description>? Upper confidence level (84%) of mass of the star from FLAME (mass_flame_upper)</description><unit>solMass</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age-Flame</name><description>? Age of the star from FLAME using stellar models (age_flame)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Age-Flame</name><description>? Lower confidence level (84%) of age of the star from FLAME (age_flame_lower)</description><unit>Gyr</unit><ucd>time.age;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Age-Flame</name><description>? Upper confidence level (84%) of age of the star from FLAME (age_flame_upper)</description><unit>Gyr</unit><ucd>time.age;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flags-Flame</name><description>[0/22]? Flags indicating quality and processing information from FLAME (flags_flame) (4)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Evol</name><description>? Evolutionary stage of the star from FLAME using stellar models (evolstage_flame)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>z-Flame</name><description>? Gravitational redshift from FLAME using radiusFlame and loggGspphot (gravredshift_flame)</description><unit>km/s</unit><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_z-Flame</name><description>? Lower confidence level (16%) of gravitational redshift from FLAME (gravredshift_flame_lower)</description><unit>km/s</unit><ucd>src.redshift;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_z-Flame</name><description>? Upper confidence level (84%) of gravitational redshift from FLAME (gravredshift_flame_upper)</description><unit>km/s</unit><ucd>src.redshift;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BolCorr</name><description>? Bolometric correction used to derive lumFlame (bc_flame)</description><unit>mag</unit><ucd>phot.mag.bc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[M/H]-MSC</name><description>? Metallicity of the source treated as a binary system from MSC using BP/RP spectra and parallax (mh_msc)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_[M/H]-MSC</name><description>? Upper confidence level (84%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_upper)</description><ucd>phys.abund;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_[M/H]-MSC</name><description>? Lower confidence level (16%) of the metallicity from MSC using BP/RP spectra and parallax (mh_msc_lower)</description><ucd>phys.abund;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0-MSC</name><description>? Monochromatic extinction A0 at 541.4nm of the source treated as a binary system from MSC using BP/RP spectra and parallax (azero_msc)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_A0-MSC</name><description>? Upper confidence level (84%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_A0-MSC</name><description>? Lower confidence level (16%) of monochromatic extinction A0 at 547.7nm from MSC using BP/RP spectra and parallax (azero_msc_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Dist-MSC</name><description>? Distance from MSC using BP/RP spectra and parallax (distance_msc)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist-MSC</name><description>? Upper confidence level (84%) of distance from MSC using BP/RP spectra and parallax (distance_msc_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist-MSC</name><description>? Lower confidence level (16%) of distance from MSC using BP/RP spectra and parallax (distance_msc_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff1-MSC</name><description>? Effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff1-MSC</name><description>? Upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff1-MSC</name><description>? Lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff2-MSC</name><description>? Effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff2-MSC</name><description>? Upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff2-MSC</name><description>? Lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg1-MSC</name><description>? Surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg1-MSC</name><description>? Upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg1-MSC</name><description>? Lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (logg_msc1_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg2-MSC</name><description>? Surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg2-MSC</name><description>? Upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg2-MSC</name><description>? Lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (logg_msc2_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG-MSC</name><description>? Extinction in G band from MSC using BP/RP spectra and parallax (ag_msc)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_AG-MSC</name><description>? Upper confidence level (84%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_upper)</description><unit>mag</unit><ucd>phys.absorption;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_AG-MSC</name><description>? Lower confidence level (16%) of extinction in G band from MSC using BP/RP spectra and parallax (ag_msc_lower)</description><unit>mag</unit><ucd>phys.absorption;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logpost-MSC</name><description>? Goodness-of-fit score (normalised log-posterior) of MSC MCMC (logposterior_msc)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp-MSC</name><description>? Mean MCMC acceptance rate of MSC MCMC (mcmcaccept_msc)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>drift-MSC</name><description>? Mean drift of the MSC MCMC chain in units of parameter standard deviation (mcmcdrift_msc)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flag-MSC</name><description>[0/1]? Flag indicating quality information from MSC (flags_msc) (5)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NOAId</name><description>? Identifier of the OA SOM map neuron that represents the source (neuron_oa_id)</description><ucd>stat.fit.param</ucd><flag>nullable</flag></column><column><name>NOADist</name><description>? Distance between the source XP spectra and the OA neuron XP prototype that represents the source (neuron_oa_dist)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NOADistRank</name><description>[0/95]? Percentile rank according to the distance distribution of the OA neuron that represents the source (neuron_oa_dist_percentile_rank)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Flags-NOA</name><description>? Flags indicating quality and processing information from OA (flags_oa) (6)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>I/355/paramsup</name><description>Additional parameters from the Apsis processing chain, compared to the main table astrophysical parameters, from modules that produce more than one result for a parameter (473020612 sources) (astrophysical_parameters_supp)</description><column><name>Source</name><description>Source Identifier (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>Lib</name><description>Name of library that achieves the highest mean log-posterior in MCMC samples from GSP-Phot Aeneas (libname_best_gspphot)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Teff</name><description>? Effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for MARCS library using BP/RP spectra (teff_gspphot_marcs_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg</name><description>? Surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for MARCS library using BP/RP spectra (logg_gspphot_marcs_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]</name><description>? Iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mh_gspphot_marcs_upper)</description><ucd>stat.value;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas for MARCS library using BP/RP spectra (distance_gspphot_marcs_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0</name><description>? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0</name><description>? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0</name><description>? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for MARCS library using BP/RP spectra (azero_gspphot_marcs_upper)</description><unit>mag</unit><ucd>stat.value;phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG</name><description>? Extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ag_gspphot_marcs_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ABP</name><description>? Extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ABP</name><description>? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ABP</name><description>? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (abp_gspphot_marcs_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ARP</name><description>? Extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ARP</name><description>? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ARP</name><description>? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for MARCS library using BP/RP spectra (arp_gspphot_marcs_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)</name><description>? Reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs)</description><unit>mag</unit><ucd>phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)</name><description>? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)</name><description>? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for MARCS library using BP/RP spectra (ebpminrp_gspphot_marcs_upper)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GMAG</name><description>? Absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_GMAG</name><description>? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs_lower)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_GMAG</name><description>? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for MARCS library using BP/RP spectra (mg_gspphot_marcs_upper)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad</name><description>? Radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad</name><description>? Lower confidence level (16%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad</name><description>? Upper confidence level (84%) of radius from GSP-Phot Aeneas for MARCS library using BP/RP spectra (radius_gspphot_marcs_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logpost</name><description>? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for MARCS library (logposterior_gspphot_marcs)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp</name><description>? MCMC acceptance rate of GSP-Phot Aeneas MCMC for MARCS library (mcmcaccept_gspphot_marcs)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff-Phx</name><description>? Effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff-Phx</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff-Phx</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (teff_gspphot_phoenix_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg-Phx</name><description>? Surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg-Phx</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg-Phx</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (logg_gspphot_phoenix_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]-Phx</name><description>? Iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]-Phx</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]-Phx</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mh_gspphot_phoenix_upper)</description><ucd>stat.value;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist-Phx</name><description>? Distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist-Phx</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist-Phx</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (distance_gspphot_phoenix_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0Phoenix</name><description>? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0Phoenix</name><description>? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0Phoenix</name><description>? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (azero_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>stat.value;phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG-Phx</name><description>? Extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG-Phx</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG-Phx</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ag_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ABP-Phx</name><description>? Extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ABP-Phx</name><description>? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ABP-Phx</name><description>? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (abp_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ARP-Phx</name><description>? Extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ARP-Phx</name><description>? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ARP-Phx</name><description>? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (arp_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)-Phx</name><description>? Reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix)</description><unit>mag</unit><ucd>phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)-Phx</name><description>? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)-Phx</name><description>? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (ebpminrp_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GMAG-Phx</name><description>? Absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_GMAG-Phx</name><description>? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix_lower)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_GMAG-Phx</name><description>? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (mg_gspphot_phoenix_upper)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad-Phx</name><description>? Radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad-Phx</name><description>? Lower confidence level (16%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad-Phx</name><description>? Upper confidence level (84%) of radius from GSP-Phot Aeneas for PHOENIX library using BP/RP spectra (radius_gspphot_phoenix_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logpost-Phx</name><description>? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for PHOENIX library (logposterior_gspphot_phoenix)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp-Phx</name><description>? MCMC acceptance rate of GSP-Phot Aeneas MCMC for PHOENIX library (mcmcaccept_gspphot_phoenix)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff-OB</name><description>? Effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff-OB</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff-OB</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for OB library using BP/RP spectra (teff_gspphot_ob_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg-OB</name><description>? Surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg-OB</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg-OB</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for OB library using BP/RP spectra (logg_gspphot_ob_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]-OB</name><description>? Iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]-OB</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]-OB</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for OB library using BP/RP spectra (mh_gspphot_ob_upper)</description><ucd>stat.value;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist-OB</name><description>? Distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist-OB</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist-OB</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas for OB library using BP/RP spectra (distance_gspphot_ob_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0-OB</name><description>? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0-OB</name><description>? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0-OB</name><description>? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for OB library using BP/RP spectra (azero_gspphot_ob_upper)</description><unit>mag</unit><ucd>stat.value;phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG-OB</name><description>? Extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG-OB</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG-OB</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for OB library using BP/RP spectra (ag_gspphot_ob_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ABP-OB</name><description>? Extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ABP-OB</name><description>? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ABP-OB</name><description>? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for OB library using BP/RP spectra (abp_gspphot_ob_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ARP-OB</name><description>? Extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ARP-OB</name><description>? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ARP-OB</name><description>? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for OB library using BP/RP spectra (arp_gspphot_ob_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)-OB</name><description>? Reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob)</description><unit>mag</unit><ucd>phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)-OB</name><description>? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob_lower)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)-OB</name><description>? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for OB library using BP/RP spectra (ebpminrp_gspphot_ob_upper)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GMAG-OB</name><description>? Absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_GMAG-OB</name><description>? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob_lower)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_GMAG-OB</name><description>? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for OB library using BP/RP spectra (mg_gspphot_ob_upper)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad-OB</name><description>? Radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad-OB</name><description>? Lower confidence level (16%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad-OB</name><description>? Upper confidence level (84%) of radius from GSP-Phot Aeneas for OB library using BP/RP spectra (radius_gspphot_ob_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logpost-OB</name><description>? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for OB library (logposterior_gspphot_ob)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp-OB</name><description>? MCMC acceptance rate of GSP-Phot Aeneas MCMC for OB library (mcmcaccept_gspphot_ob)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff-A</name><description>? Effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Teff-A</name><description>? Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Teff-A</name><description>? Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas for A library using BP/RP spectra (teff_gspphot_a_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg-A</name><description>? Surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg-A</name><description>? Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg-A</name><description>? Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas for A library using BP/RP spectra (logg_gspphot_a_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]-A</name><description>? Iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]-A</name><description>? Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]-A</name><description>? Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas for A library using BP/RP spectra (mh_gspphot_a_upper)</description><ucd>stat.value;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist-A</name><description>? Distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Dist-A</name><description>? Lower confidence level (16%) of distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a_lower)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Dist-A</name><description>? Upper confidence level (84%) of distance from GSP-Phot Aeneas for A library using BP/RP spectra (distance_gspphot_a_upper)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>A0-A</name><description>? Monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0-A</name><description>? Lower confidence level (16%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.V;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0-A</name><description>? Upper confidence level (84%) of monochromatic extinction A_0 at 547.7nm from GSP-Phot Aeneas for A library using BP/RP spectra (azero_gspphot_a_upper)</description><unit>mag</unit><ucd>stat.value;phys.absorption;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG-A</name><description>? Extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG-A</name><description>? Lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG-A</name><description>? Upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas for A library using BP/RP spectra (ag_gspphot_a_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ABP-A</name><description>? Extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ABP-A</name><description>? Lower confidence level (16%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ABP-A</name><description>? Upper confidence level (84%) of extinction in G_BP band from GSP-Phot Aeneas for A library using BP/RP spectra (abp_gspphot_a_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ARP-A</name><description>? Extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_ARP-A</name><description>? Lower confidence level (16%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a_lower)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_ARP-A</name><description>? Upper confidence level (84%) of extinction in G_RP band from GSP-Phot Aeneas for A library using BP/RP spectra (arp_gspphot_a_upper)</description><unit>mag</unit><ucd>phys.absorption;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)-A</name><description>? Reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a)</description><unit>mag</unit><ucd>phot.color.excess;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)-A</name><description>? Lower confidence level (16%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a_lower)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)-A</name><description>? Upper confidence level (84%) of reddening E(BP-RP) from GSP-Phot Aeneas for A library using BP/RP spectra (ebpminrp_gspphot_a_upper)</description><unit>mag</unit><ucd>phot.color.excess;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GMAG-A</name><description>? Absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a)</description><unit>mag</unit><ucd>phys.magAbs;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_GMAG-A</name><description>? Lower confidence level (16%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a_lower)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_GMAG-A</name><description>? Upper confidence level (84%) of absolute magnitude M_G from GSP-Phot Aeneas for A library using BP/RP spectra (mg_gspphot_a_upper)</description><unit>mag</unit><ucd>phys.magAbs;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Rad-A</name><description>? Radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Rad-A</name><description>? Lower confidence level (16%) of radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Rad-A</name><description>? Upper confidence level (84%) of radius from GSP-Phot Aeneas for A library using BP/RP spectra (radius_gspphot_a_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logpost-A</name><description>? Goodness-of-fit score (mean log-posterior of MCMC) of GSP-Phot Aeneas MCMC for A library (logposterior_gspphot_a)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Accp-A</name><description>? MCMC acceptance rate of GSP-Phot Aeneas MCMC for A library (mcmcaccept_gspphot_a)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff-ANN</name><description>? Effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Teff-ANN</name><description>? Lower confidence level (16%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann_lower)</description><unit>K</unit><ucd>phys.temperature.effective;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Teff-ANN</name><description>? Upper confidence level (84%) of effective temperature from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (teff_gspspec_ann_upper)</description><unit>K</unit><ucd>phys.temperature.effective;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logg-ANN</name><description>? Surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_logg-ANN</name><description>? Lower confidence level (16%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann_lower)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_logg-ANN</name><description>? Upper confidence level (84%) of surface gravity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (logg_gspspec_ann_upper)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[M/H]-ANN</name><description>? Global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[M/H]-ANN</name><description>? Lower confidence level (16%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann_lower)</description><ucd>phys.abund.Fe;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[M/H]-ANN</name><description>? Upper confidence level (84%) of global metallicity from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (mh_gspspec_ann_upper)</description><ucd>stat.value;phys.abund.Fe;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[alpha/Fe]-ANN</name><description>? Abundance of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_[alpha/Fe]-ANN</name><description>? Lower confidence level (16%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann_lower)</description><ucd>phys.abund;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_[alpha/Fe]-ANN</name><description>? Upper confidence level (84%) of alpha-elements with respect to iron from GSP-Spec ANN using RVS spectra and Monte Carlo realisations (alphafe_gspspec_ann_upper)</description><ucd>phys.abund;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logpost-ANN</name><description>? Logarithm of the goodness-of-fit for the GSP-Spec ANN parameters (logchisq_gspspec_ann)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flags-ANN</name><description>? Catalogue flags for GSP-Spec ANN (flags_gspspec_ann) (1)</description><ucd>meta.code.status</ucd><flag>nullable</flag></column><column><name>Rad-Flame</name><description>? Radius of the star from FLAME using teffGspspec and lumFlameSpec (radius_flame_spec)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Rad-Flame</name><description>? Lower confidence level (16%) of radiusFlameSpec (radius_flame_spec_lower)</description><unit>solRad</unit><ucd>phys.size.radius;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Rad-Flame</name><description>? Upper confidence level (84%) of radiusFlameSpec (radius_flame_spec_upper)</description><unit>solRad</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lum-Flame</name><description>? Luminosity of the star from FLAME using G band magnitude (lum_flame_spec)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Lum-Flame</name><description>? Lower confidence level (16%) of lumFlameSpec (lum_flame_spec_lower)</description><unit>solLum</unit><ucd>phys.luminosity;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Lum-Flame</name><description>? Upper confidence level (84%) of lumFlameSpec (lum_flame_spec_upper)</description><unit>solLum</unit><ucd>phys.luminosity;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mass-Flame</name><description>? Mass of the star from FLAME using stellar models (mass_flame_spec)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Mass-Flame</name><description>? Lower confidence level (16%) of massFlameSpec (mass_flame_spec_lower)</description><unit>solMass</unit><ucd>phys.mass;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Mass-Flame</name><description>? Upper confidence level (84%) of massFlameSpec (mass_flame_spec_upper)</description><unit>solMass</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Age-Flame</name><description>? Age of the star from FLAME using stellar models (age_flame_spec)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Age-Flame</name><description>? Lower confidence level (16%) of ageFlameSpec (age_flame_spec_lower)</description><unit>Gyr</unit><ucd>time.age;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Age-Flame</name><description>? Upper confidence level (84%) of ageFlameSpec (age_flame_spec_upper)</description><unit>Gyr</unit><ucd>time.age;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flag-Flame</name><description>[0/2]? Flag indicating quality of parameters from FLAME using GSP-Spec parameters (flags_flame_spec) (2)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Evol</name><description>? Evolutionary stage of the star from FLAME using stellar models (evolstage_flame_spec)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>z-Flame</name><description>? Gravitational redshift from FLAME using GSP-Spec parameters (gravredshift_flame_spec)</description><unit>km/s</unit><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_z-Flame</name><description>? Lower confidence interval of gravredshiftFlameSpec (gravredshift_flame_spec_lower)</description><unit>km/s</unit><ucd>src.redshift;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_z-Flame</name><description>? Upper confidence interval of gravredshiftFlameSpec (gravredshift_flame_spec_upper)</description><unit>km/s</unit><ucd>src.redshift;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BolCorr</name><description>? Bolometric correction applied to derive lumFlameSpec using GSP-Spec parameters (bc_flame_spec)</description><unit>mag</unit><ucd>phot.mag.bc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>I/355/tgextmap</name><description>Total Galactic Extinction (TGE) map for extinction parameters A0</description><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>A0</name><description>? Mean A_0_ extinction parameter (a0) (1)</description><unit>mag</unit><ucd>phys.absorption.coeff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A0</name><description>? Uncertainty for the mean A_0_ (a0_uncertainty)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_A0</name><description>? Minimum A_0_ value used for the HEALPix of interest (a0_min)</description><unit>mag</unit><ucd>phys.absorption.coeff;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_A0</name><description>? Maximum A_0_ value used for the HEALPix of interest (a0_max)</description><unit>mag</unit><ucd>phys.absorption.coeff;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ntracers</name><description>Number of tracers used (num_tracers_used)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HPId</name><description>Unique HEALPix index number for which the total Galactic extinction parameters are estimated (healpix_id)</description><ucd>pos.healpix</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HPlevel</name><description>[6/9] HEALPix level used (healpix_level) n</description><ucd>pos.healpix</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>foptHP</name><description>[0/1] Flag to indicate whether a given HEALPix level is the optimum (1) or not (0) (optimum_hpx_flag) (2)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Status</name><description>[0/3] Exit status for TGE (status) (3)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>I/355/tgextopt</name><description>Optimum version of the Total Galactic Extinction Map, derived from the table tgextmap.dat (total_galactic_extinction_map) at a single HELPix level 9</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>HPId</name><description>Unique HEALPix index number for which the total Galactic extinction parameters are estimated (healpix_id)</description><ucd>pos.healpix</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>A0</name><description>? Median A_0_ extinction parameter (a0) (1)</description><unit>mag</unit><ucd>phys.absorption.coeff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A0</name><description>? Uncertainty for the mean A_0_ (a0_uncertainty)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ntracers</name><description>Number of tracers used (num_tracers_used)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Status</name><description>[0/3] Exit status for TGE (status) (2)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HPlevel</name><description>[6/9] Number indicating which HEALPix level was chosen to populate this HEALPix (optimum_hpx_level)</description><ucd>pos.healpix</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>I/355/oaninfo</name><description>Content of a Self-Organized Map calculated from a dataset composed by outliers by the Apsis module OA (oa_neuron_information)</description><column><name>CentDist</name><description>Squared Euclidean distance between the centroid XP spectrum and the neuron XP prototype (centroid_distance)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>SOMID</name><description>Self-Organized Map identifier (som_id)</description><ucd>meta.id</ucd></column><column><name>NeuId</name><description>Neuron identifier (neuron_id)</description><ucd>meta.id</ucd></column><column><name>NeuRowIdx</name><description>[0/29] Row index of the neuron in the Self-Organised Map lattice (neuron_row_index)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NeuColIdx</name><description>[0/29] Column index of the neuron in the Self-Organised Map lattice (neuron_column_index)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>hits</name><description>Number of sources populating the neuron (hits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CentId</name><description>Identifier of the Gaia source that minimizes the classification distance to the neuron (centroid_id)</description><ucd>meta.id</ucd></column><column><name>TempDist</name><description>? Squared Euclidean distance between the reference XP template and the neuron XP prototype (template_distance)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>Mean G value for the sources that belong to the neuron (g_mag_mean)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_Gmag</name><description>Standard deviation of G values for the sources that belong to the neuron (g_mag_std_dev)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_Gmag</name><description>Minimum G value for the sources that belong to the neuron (g_mag_min)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_Gmag</name><description>Maximum G value for the sources that belong to the neuron (g_mag_max)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BPmag</name><description>Mean G_BP_ value for the sources that belong to the neuron (bp_mag_mean)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_BPmag</name><description>Standard deviation of G_BP_ values for the sources that belong to the neuron (bp_mag_std_dev)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_BPmag</name><description>Minimum value of G_BP_ for the sources that belong to the neuron (bp_mag_min)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_BPmag</name><description>Maximum value of G_BP_ for the sources that belong to the neuron (bp_mag_max)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPmag</name><description>Mean G_RP_ value for the sources that belong to the neuron neuron (rp_mag_mean)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_RPmag</name><description>Standard deviation of G_RP_ values for the sources that belong to the neuron (rp_mag_std_dev)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_RPmag</name><description>Minimum value of G_RP_ for the sources that belong to the neuron (rp_mag_min)</description><unit>mag</unit><ucd>phot.mag;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_RPmag</name><description>Maximum value of G_RP_ for the sources that belong to the neuron (rp_mag_max)</description><unit>mag</unit><ucd>phot.mag;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRA</name><description>Mean value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_mean)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_pmRA</name><description>Standard deviation of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_std_dev)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_pmRA</name><description>Minimum value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_min)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_pmRA</name><description>Maximum value of the proper motion in right ascension for the sources that belong to the neuron (pm_ra_max)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>Mean value of the proper motion in declination for the sources that belong to the neuron (pm_dec_mean)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_pmDE</name><description>Standard deviation of the proper motion in declination for the sources that belong to the neuron (pm_dec_std_dev)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_pmDE</name><description>Minimum value of the proper motion in declination for the sources that belong to the neuron (pm_dec_min)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_pmDE</name><description>Maximum value of the proper motion in declination for the sources that belong to the neuron (pm_dec_max)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Plx</name><description>Mean parallax value for the sources that belong to the neuron (parallax_mean)</description><unit>mas</unit><ucd>pos.parallax.trig;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_Plx</name><description>Standard deviation of the parallax values for the sources that belong to the neuron (parallax_std_dev)</description><unit>mas</unit><ucd>stat.error;pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_Plx</name><description>Minimum parallax value for the sources that belong to the neuron (parallax_min)</description><unit>mas</unit><ucd>pos.parallax.trig;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_Plx</name><description>Maximum parallax value for the sources that belong to the neuron (parallax_max)</description><unit>mas</unit><ucd>pos.parallax.trig;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>GLON</name><description>[] Mean galactic latitude for the sources that belong to the neuron (gal_latitude_mean)</description><unit>deg</unit><ucd>pos.galactic.lat;stat.mean</ucd></column><column><name>s_GLON</name><description>Standard deviation of the galactic latitude values for the sources that belong to the neuron (gal_latitude_std_dev)</description><unit>deg</unit><ucd>stat.error;pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_GLON</name><description>Minimum galactic latitude for the sources that belong to the neuron (gal_latitude_min)</description><unit>deg</unit><ucd>pos.galactic.lat;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_GLON</name><description>Maximum galactic latitude for the sources that belong to the neuron (gal_latitude_max)</description><unit>deg</unit><ucd>pos.galactic.lat;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>intraDist</name><description>Mean value of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_mean)</description><ucd>pos.distance;stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_intraDist</name><description>Standard deviation of the squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_std_dev)</description><ucd>stat.value;stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_intraDist</name><description>Minimum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_min)</description><ucd>stat.value;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_intraDist</name><description>Maximum squared Euclidean distance between each of the XP sources in the neuron and the neuron prototype (intra_neuron_distance_max)</description><ucd>stat.value;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>interDist</name><description>Mean value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_mean)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_interDist</name><description>Standard deviation of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_std_dev)</description><ucd>stat.value;stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_interDist</name><description>Minimum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_min)</description><ucd>stat.value;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_interDist</name><description>Maximum value of the squared Euclidean distance between the neuron XP prototype and the XP prototypes of its immediate neighbours (inter_neuron_distance_max)</description><ucd>stat.value;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dist25</name><description>25th percentile value for the intra-neuron distance distribution (distance_percentile25)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dist50</name><description>50th percentile value for the intra-neuron distance distribution (distance_percentile50)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dist68</name><description>68th percentile value for the intra-neuron distance distribution (distance_percentile68)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dist75</name><description>75th percentile value for the intra-neuron distance distribution (distance_percentile75)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dist99</name><description>95th percentile value for the intra-neuron distance distribution (distance_percentile95)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>distFWHM</name><description>Full Width at Half Maximum value for the intra-neuron distance distribution (distance_fwhm)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>distSkew</name><description>Skewness value for the intra-neuron distance distribution (distance_skew)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>distKur</name><description>Kurtosis value for the intra-neuron distance distribution (distance_kurtosis)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>distiqr</name><description>Inter-Quartile Range value for the intra-neuron distance distribution (distance_i_q_r)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>distFWHMn</name><description>Normalized FWHM value for the intra-neuron distance distribution (distance_fwhm_norm)</description><ucd>stat.value</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Quality</name><description>[0/6] Quality category assigned to the neuron (quality_category)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NBP</name><description>Mean value of the number of BP transits for the sources that belong to the neuron (bp_transits_mean)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_NBP</name><description>Standard deviation of the number of BP transits for the sources that belong to the neuron (bp_transits_std_dev)</description><ucd>meta.number;stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_NBP</name><description>Minimum value of the number of BP transits for the sources that belong to the neuron (bp_transits_min)</description><ucd>meta.number;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_NBP</name><description>Maximum value of the number of BP transits for the sources that belong to the neuron (bp_transits_max)</description><ucd>meta.number;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NRP</name><description>Mean value of the number of RP transits for the sources that belong to the neuron (rp_transits_mean)</description><ucd>meta.number;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_NRP</name><description>Standard deviation of the number of RP transits for the sources that belong to the neuron (rp_transits_std_dev)</description><ucd>meta.number;stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_NRP</name><description>Minimum value of the number of RP transits for the sources that belong to the neuron (rp_transits_min)</description><ucd>meta.number;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B_NRP</name><description>Maximum value of the number of RP transits for the sources that belong to the neuron (rp_transits_max)</description><ucd>meta.number;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RUWE</name><description>Mean value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_mean)</description><ucd>stat.weight;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_RUWE</name><description>Standard deviation of the renormalised unit weight error for the sources that belong to the neuron (ruwe_std_dev)</description><ucd>stat.weight;stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_RUWE</name><description>Minimum value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_min)</description><ucd>stat.weight;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_RUWE</name><description>Maximum value of the renormalised unit weight error for the sources that belong to the neuron (ruwe_max)</description><ucd>stat.weight;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E(BP/RP)</name><description>Mean value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_mean)</description><ucd>arith.factor;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_E(BP/RP)</name><description>Standard deviation of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_std_dev)</description><ucd>arith.factor;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_E(BP/RP)</name><description>Minimum value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_min)</description><ucd>arith.factor;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_E(BP/RP)</name><description>Maximum value of the BP/RP flux excess for the sources that belong to the neuron (bprp_mean_flux_excess_max)</description><ucd>arith.factor;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BP-RP</name><description>Mean value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_mean)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>s_BP-RP</name><description>Standard deviation of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_std_dev)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_BP-RP</name><description>Minimum value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_min)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_BP-RP</name><description>Maximum value of the G_BP_-G_RP_ colour for the sources that belong to the neuron (bprp_colour_max)</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Class</name><description>? Astronomical class estimated for the neuron (class_label)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Template</name><description>Name of the template used to describe the neuron (template_name)</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column></table><table><name>I/355/oaxpsp</name><description>Prototype BP/RP spectrum corresponding to each of the neurons of the Self-Organised-Map produced by the Apsis module OA (oa_neuron_xp_spectra)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>NeuId</name><description>Neuron identifier (neuron_id)</description><ucd>meta.id</ucd></column><column><name>NeuRowIdx</name><description>[0/29] Row index of the neuron in the Self-Organised Map lattice (neuron_row_index)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NeuColIdx</name><description>[0/29] Column index of the neuron in the Self-Organised Map lattice (neuron_column_index)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>XPFlux</name><description>Normalised flux at wavelength XPlambda for the preprocessed XP spectrum that best represents the neuron (prototype) (xp_spectrum_prototype_flux)</description><ucd>phot.flux;stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>XPlambda</name><description>Wavelength associated with the XP spectrum flux values (xp_spectrum_prototype_wavelength)</description><unit>nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>XPFluxTemp</name><description>? Normalised flux at wavelength XPlambda for the preprocessed XP spectrum corresponding to the neuron template (xp_spectrum_template_flux)</description><ucd>phot.flux;stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>I/355/epphot</name><description>Light curves for a given object in bands G, BP and RP (555868797 rows) (epoch_photometry)</description><column><name>e_FRP</name><description>? RP band flux error (rp_flux_error)</description><ucd>stat.error;phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPrVFlag</name><description>[0/1] BP transit photometry rejected by variability processing (variability_flag_bp_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>TransitID</name><description>Transit unique identifier (transit_id)</description><ucd>meta.id</ucd></column><column><name>FG</name><description>? Transit averaged G band flux (g_transit_flux)</description><ucd>phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FG</name><description>? Transit averaged G band flux error (g_transit_flux_error)</description><ucd>stat.error;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFG</name><description>? Transit averaged G band flux divided by its error (g_transit_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>? Transit averaged G band Vega magnitude (g_transit_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NG</name><description>[0-9] Number of CCD observations contributing to transit averaged G band flux (g_transit_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TimeBP</name><description>? BP CCD transit observing time JD-2455197.5 (bp_obs_time)</description><unit>d</unit><ucd>time.epoch;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FBP</name><description>? BP band flux (bp_flux)</description><ucd>phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FBP</name><description>? BP band flux error (bp_flux_error)</description><ucd>stat.error;phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFBP</name><description>? BP band flux divided by its error (bp_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPmag</name><description>? BP band Vega magnitude (bp_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>TimeRP</name><description>? RP CCD transit observing time JD-2455197.5 (rp_obs_time)</description><unit>d</unit><ucd>time.epoch;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>FRP</name><description>? RP band flux (rp_flux)</description><ucd>phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RFRP</name><description>? RP band flux divided by its error (rp_flux_over_error)</description><ucd>stat.snr;phot.flux;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPmag</name><description>? RP band Vega magnitude (rp_mag)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>noisyFlag</name><description>[0/1] G band flux scatter larger than expected by photometry processing (all CCDs considered) (photometry_flag_noisy_data)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SMuFlag</name><description>[0/1] SM transit unavailable by photometry processing (photometry_flag_sm_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF1uFlag</name><description>[0/1] AF1 transit unavailable by photometry processing (photometry_flag_af1_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF2uFlag</name><description>[0/1] AF2 transit unavailable by photometry processing (photometry_flag_af2_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF3uFlag</name><description>[0/1] AF3 transit unavailable by photometry processing (photometry_flag_af3_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF4uFlag</name><description>[0/1] AF4 transit unavailable by photometry processing (photometry_flag_af4_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF5uFlag</name><description>[0/1] AF5 transit unavailable by photometry processing (photometry_flag_af5_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF6uFlag</name><description>[0/1] AF6 transit unavailable by photometry processing (photometry_flag_af6_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF7uFlag</name><description>[0/1] AF7 transit unavailable by photometry processing (photometry_flag_af7_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF8uFlag</name><description>[0/1] AF8 transit unavailable by photometry processing (photometry_flag_af8_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF9uFlag</name><description>[0/1] AF9 transit unavailable by photometry processing (photometry_flag_af9_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BPuFlag</name><description>[0/1] BP transit unavailable by photometry processing (photometry_flag_bp_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPuFlag</name><description>[0/1] RP transit unavailable by photometry processing (photometry_flag_rp_unavailable)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SMrFlag</name><description>[1] SM transit rejected by photometry processing (photometry_flag_sm_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF1rFlag</name><description>[0/1] AF1 transit rejected by photometry processing (photometry_flag_af1_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF2rFlag</name><description>[0/1] AF2 transit rejected by photometry processing (photometry_flag_af2_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF3rFlag</name><description>[0/1] AF3 transit rejected by photometry processing (photometry_flag_af3_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF4rFlag</name><description>[0/1] AF4 transit rejected by photometry processing (photometry_flag_af4_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF5rFlag</name><description>[0/1] AF5 transit rejected by photometry processing (photometry_flag_af5_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF6rFlag</name><description>[0/1] AF6 transit rejected by photometry processing (photometry_flag_af6_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF7rFlag</name><description>[0/1] AF7 transit rejected by photometry processing (photometry_flag_af7_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF8rFlag</name><description>[0/1] AF8 transit rejected by photometry processing (photometry_flag_af8_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AF9rFlag</name><description>[0/1] AF9 transit rejected by photometry processing (photometry_flag_af9_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BPrFlag</name><description>[0/1] BP transit rejected by photometry processing (photometry_flag_bp_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPrFlag</name><description>[0/1] RP transit rejected by photometry processing (photometry_flag_rp_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GrVFlag</name><description>[0/1] Average G transit photometry rejected by variability processing (variability_flag_g_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPrVFlag</name><description>[0/1] RP transit photometry rejected by variability processing (variability_flag_rp_reject)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>TimeG</name><description>? Transit averaged G band observing time JD-2455197.5 (g_transit_time)</description><unit>d</unit><ucd>time.epoch;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag><flag>indexed</flag></column></table><table><name>I/355/gcrf3xm</name><description>Full cross-match information for the Gaia-CRF3 sources (Gaia_Crf3_Xm)</description><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>OCARSname</name><description>The name for this source in OCARS (ocars_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>Source</name><description>Gaia source identifier (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>ICRF3sx</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 S/X (icrf3sx)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ICRF3k</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 K (icrf3k)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ICRF3xka</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in ICRF3 X/Ka (icrf3xka)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>OCARS</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in OCARS, www.gaoran.ru/english/as/ac_vlbi/#OCARS (ocars)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AW15</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in allWISE, SECREST et al., 2015ApJS..221...12S, Cat. J/ApJS/221/12 (aw15)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>R90</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the catalogue R90, Assef at al., 2018ApJS..234...23A, Cat. J/ApJS/234/32 (r90)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M65</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in Milliquas v6.5 (m65)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>C75</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the catalogue C75, Assef at al., 2018ApJS..234...23A, Cat. J/ApJS/234/32 (c75)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>DR14q</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the catalogue SDSS DR14Q, Paris et al., 2018A&amp;A...613A..51P, Cat. VII/286 (dr14q)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LQAC5</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in LQAC-5, Souchay et al., 2019A&amp;A...624A.145S, Cat. J/A+A/624/A145 (lqac5)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LAMOST5</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the LAMOST QSO catalogue (lamost5)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LQRF</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in LQRF, Andrei et al., 2009A&amp;A...505..385A, Cat. I/313 (lqrf)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LQRFname</name><description>? The name for this source in LQRF (lqrf_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>2QZ</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in 2QZ, Croom et al., 2004MNRAS.349.1397C, Cat. VII/241 (cat2qz)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BZCAT5</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in Roma-BZCAT, Massaro et al., 2015Ap&amp;SS.357...75M, Cat. VII/274 (bzcat5)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BZCAT5name</name><description>The name for this source in Roma-BZCAT (bzcat5_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>2WHSPJ</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in 2WHSPJ (cat2whspj)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2WHSPJname</name><description>The name for this source in 2WHSPJ, Chang et al., 2017A&amp;A...598A..17C, Cat. J/A+A/598/A17 (cat2whspj_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>ALMA19</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the ALMA calibrator catalogue, BONATO et al., 2019MNRAS.485.1188B, Cat. J/MNRAS/485/1188 (alma19)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GUW</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in Gaia-unWISE, Su et al., 2019MNRAS.489.4741S (guw)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B19</name><description>[0/1] The flag describing if the Gaia-CRF3 source was found in the Gaia DR2 quasar and galaxy classification catalogue, Bailer-Jones et al., 2019MNRAS.490.5615B, Cat VII/285 (b19)</description><ucd>meta.code.status</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>B19name</name><description>? The name for this source in the Gaia DR2 quasar and galaxy classification catalogue (b19_name)</description><ucd>meta.id.cross</ucd><flag>nullable</flag></column><column><name>ICRFname</name><description>The ICRF name of the source (icrf_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>IERSname</name><description>The IERS name of the source (iers_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>AW15name</name><description>The name for this source in allWISE (aw15_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>R90name</name><description>The name for this source in R90 (r90_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>M65name</name><description>The name for this source in Milliquas v6.5, Flesch, Cat. VII/290 (m65_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>C75name</name><description>The name for this source in C75 (c75_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>DR14qname</name><description>The name for this source in SDSS DR14Q (dr14q_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>LQAC5name</name><description>The name for this source in LQAC-5 (lqac5_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>LAMOST5name</name><description>The name for this source in the LAMOST QSO catalogue, Luo et al., Cat. V/164 (lamost5_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>2QZname</name><description>The name for this source in 2QZ (cat2qz_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>ALMA19name</name><description>The name for this source in the ALMA calibrator catalogue (alma19_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>GUWname</name><description>The name for this source in Gaia-unWISE (guw_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column></table><table><name>I/355/rvsmean</name><description>RVS mean sampled spectrum table (2400147645 lines) (rvs_mean_spectrum)</description><column><name>Flux</name><description>? Normalized flux (flux) (1)</description><ucd>phot.flux;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Flux</name><description>? Uncertainties in Flux (flux_error) (1)</description><ucd>stat.error;phot.flux;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RAICRS</name><description>Right Ascension ICRS ar Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEICRS</name><description>Declination ICRS ar Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>NTransit</name><description>Number of combined transits (combined_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NcCCD</name><description>Number of combined CCD spectra (combined_ccds)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NdCDD</name><description>Number of deblended CCD spectra (deblended_ccds)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>[846/870] Wavelength (wavelength) (1)</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>I/355/xpsummary</name><description>Auxiliary information about the mean BP/RP spectrum (219197643 sources) (xp_summary)</description><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>NBPbases</name><description>? Number of bases that are relevant for the representation of this mean BP spectrum (bp_n_relevant_bases)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPrelsh</name><description>? Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum (bp_relative_shrinking)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NBP</name><description>? Number of measurements used for the BP spectrum generation (bp_n_measurements)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NBPrej</name><description>? Number of rejected measurements in the BP spectrum generation (bp_n_rejected_measurements)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPstddev</name><description>? Standard deviation for the BP spectrum representation (bp_standard_deviation)</description><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPchi2r</name><description>? Chi squared for the BP spectrum representation (bp_chi_squared)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NTransBP</name><description>? Number of transits contributing to the mean in BP (bp_n_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NcTransBP</name><description>? Number of contaminated transits in BP (bp_n_contaminated_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NbTransBP</name><description>? Number of blended transits in BP (bp_n_blended_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NRPbases</name><description>Number of bases that are relevant for the representation of this mean RP spectrum (rp_n_relevant_bases)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NRPrelsh</name><description>Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum (rp_relative_shrinking)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NRP</name><description>Number of measurements used for the RP spectrum generation (rp_n_measurements)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NRPrej</name><description>Number of rejected measurements in the RP spectrum generation (rp_n_rejected_measurements)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPstdev</name><description>Standard deviation for the RP spectrum representation (rp_standard_deviation)</description><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPchi2r</name><description>Chi squared for the RP spectrum representation (rp_chi_squared)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NTransRP</name><description>Number of transits contributing to the mean in RP (rp_n_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NcTransRP</name><description>Number of contaminated transits in RP (rp_n_contaminated_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NbTransRP</name><description>Number of blended transits in RP (rp_n_blended_transits)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>I/355/xpsample</name><description>BP/RP externally calibrated sampled mean spectrum (11822651939 rows) (xp_sampled_mean_spectrum)</description><column><name>RA_ICRS</name><description>Right Ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>lambda</name><description>Wavelength (wavelength) (1)</description><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Flux</name><description>Mean BP + RP combined spectrum flux (flux)</description><unit>W.m**-2.nm**-1</unit><ucd>phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>Mean BP + RP combined spectrum flux error (flux_error)</description><unit>W.m**-2.nm**-1</unit><ucd>stat.error;phot.flux;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>I/355/xpsamp</name><description>Definition of XP spectra standard sampling schemes (xp_sampling)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>Band</name><description>[BP RP] BP or RP photometric band (band)</description><ucd>instr.bandpass</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>lambda</name><description>Wavelength (wavelength) (1)</description><unit>nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Func</name><description>[0/54] Basis function index (basis_function)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SampCoeff</name><description>Sampling matrix coefficient (sampling_coefficient)</description><unit>ph.s**-1.m**-2.nm**-1</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>I/355/xpmerge</name><description>Coefficients used to merge the BP and RP externally calibrated sampled spectra into the final merged product (xp_merge)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>lambda</name><description>Wavelength (wavelength) (1)</description><unit>nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>weightBP</name><description>BP flux weight (bp_weight)</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>weightRP</name><description>RP flux weight (rp_weight)</description><ucd>stat.weight</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>I/355/xpcont</name><description>Mean BP and RP spectra based on the continuous representation in basis functions (219197643 rows) (gaia_dr3_xpcont)</description><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SolID</name><description>Solution Identifier (solution_id)</description><ucd>meta.version</ucd></column><column><name>BPDOF</name><description>? Degrees of freedom for the BP spectrum representation (bp_degrees_of_freedom)</description><ucd>stat.fit.dof</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>NBP</name><description>? Number of measurements used for the BP spectrum generation (bp_n_measurements)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPNrej</name><description>? Number of rejected measurements in the BP spectrum generation (bp_n_rejected_measurements)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPstddev</name><description>? Standard deviation for the BP spectrum representation (bp_standard_deviation)</description><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPchi2r</name><description>? Chi squared for the BP spectrum representation (bp_chi_squared)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>NBPbases</name><description>? Number of bases that are relevant for the representation of this mean BP spectrum (bp_n_relevant_bases)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPrelsh</name><description>? Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean BP spectrum (bp_relative_shrinking)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPDOF</name><description>Degrees of freedom for the RP spectrum representation (rp_degrees_of_freedom)</description><ucd>stat.fit.dof</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NRP</name><description>Number of measurements used for the RP spectrum generation (rp_n_measurements)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPNrej</name><description>Number of rejected measurements in the RP spectrum generation (rp_n_rejected_measurements)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPstddev</name><description>Standard deviation for the RP spectrum representation (rp_standard_deviation)</description><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPchi2r</name><description>Chi squared for the RP spectrum representation (rp_chi_squared)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>NRPbases</name><description>Number of bases that are relevant for the representation of this mean RP spectrum (rp_n_relevant_bases)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPrelsh</name><description>Measure of the relative shrinking of the coefficient vector when truncation is applied for the mean RP spectrum (rp_relative_shrinking)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BPrecnoS</name><description>Starting record number in the separated bp_coeff/e_bp_coeff file (added by CDS) (bp_start_recno)</description><ucd>meta.number</ucd></column><column><name>BPNelem</name><description>[0/55] Number of elements in the separated bp_coeff/e_bp_coeff file (always 55 except for 1 line) (added by CDS) (bp_n_elems)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>BPcorrrecnoS</name><description>Starting record number in the separated bp_coeff_corr file (added by CDS) (bp_corr_start_recno)</description><ucd>meta.number</ucd></column><column><name>BPcorrNelem</name><description>[0/1485] Number of elements in the separated bp_coeff_corr file (added by CDS) (always 1485 except for 1 line) (bp_corr_n_elems)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPrecnoS</name><description>Starting record number in the separated rp_coeff/e_rp_coeff file (added by CDS) (rp_start_recno)</description><ucd>meta.number</ucd></column><column><name>RPNelem</name><description>Number of elements in the separated rp_coeff/e_rp_coeff file (always 55) (rp_n_elems)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RPcorrrecnoS</name><description>Starting record number in the separated rp_coeff_corr file (added by CDS) (rp_corr_start_recno)</description><ucd>meta.number</ucd></column><column><name>RPcorrNelem</name><description>[1485] Number of elements in the separated rp_coeff_corr file (added by CDS) (rp_corr_n_elems)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>I/355/spectra</name><description>Gaia DR3 spectra view (34468373 sources)</description><column><name>RA_ICRS</name><description>? Right ascension (ICRS) at Ep=2016.0 (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DE_ICRS</name><description>? Declination (ICRS) at Ep=2016.0 (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>Source</name><description>Unique source identifier (unique within a particular Data Release) (source_id)</description><ucd>meta.id;meta.main</ucd></column><column><name>plotXPsamp</name><description>spectra Plot by CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>dataXPSamp</name><description>spectra TSV by CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>