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<ri:Resource created="2022-02-01T16:43:12Z" status="active" updated="2025-06-13T15:25:00Z" 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>GDR2AP. Gaia DR2, 2MASS, AllWISE astrophys. param.</title><shortName>V/155</shortName><identifier>ivo://CDS.VizieR/V/155</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fouesneau M.</name></creator><creator><name>Andrae R.</name></creator><creator><name>Dharmawardena T.</name></creator><creator><name>Rybizki J.</name></creator><creator><name>Bailer-Jones C.A.L.,Demleitner M.</name></creator><date role="Updated">2024-06-19T14:18:59Z</date><date role="Created">2022-02-01T16:43:12Z</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>extinction</subject><subject>stellar-distance</subject><subject>stellar-masses</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Stellar physical and dynamical properties are essential knowledge to understanding the structure, formation, and evolution of our Galaxy. We produced an all-sky uniformly derived catalog of stellar astrophysical parameters (APs; age, mass, temperature, bolometric luminosity, distance, dust extinction) to give insight into the physical properties of Milky-Way stars. Exploiting the power of multi-wavelength and multi-survey observations from Gaia DR2 parallaxes and integrated photometry along with 2MASS and AllWISE photometry, we introduce an all-sky uniformly derived catalog of stellar astrophysical parameters, including dust extinction (A0) average grain size (R0) along the line of sight, for 123097070 stars. In contrast with previous works, we do not use a Galactic model as prior in our analysis. We validate our results against other literature (e.g., benchmark stars, interferometry, Bayestar, StarHorse). The limited optical information in the Gaia photometric bands or the lack of ultraviolet or spectroscopic information renders the chemistry inference prior dominated. We demonstrate that Gaia parallaxes bring sufficient leverage to explore the detailed structures of the interstellar medium in our Milky Way. In Gaia DR3, we will obtain the dispersed optical light information to break through some limitations of this analysis, allowing us to infer stellar chemistry in particular. Gaia promises us data to construct the most detailed view of the chemo-dynamics of field star populations in our Galaxy. Our catalog is available from the German Astrophysical Virtual Observatory (GAVO) at http://dc.g-vo.org/tableinfo/ gdr2ap.main where one can query it via ADQL and TAP (and soon in the Gaia Archive).</description><source format="bibcode">2022A&amp;A...662A.125F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/V/155</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 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(logA_p84)</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLbest</name><description>multivariate maximum posterior estimate for the log10 of the luminosity (logL_best)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLmax</name><description>Maximum of the logL distribution (logL_max)</description><unit>log(solLum)</unit><ucd>phys.luminosity;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLmin</name><description>Minimum of the logL distribution (logL_min)</description><unit>log(solLum)</unit><ucd>phys.luminosity;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLp16</name><description>16th percentile of the logL distribution (logL_p16)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLp25</name><description>25th percentile of the logL distribution (logL_p25)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLmed</name><description>median of the distribution of log10 of the luminosity (logL_p50)</description><unit>log(solLum)</unit><ucd>phys.luminosity;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLp75</name><description>75th percentile of the logL distribution (logL_p75)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logLp84</name><description>84th percentile of the logL distribution (logL_p84)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMbest</name><description>multivariate maximum posterior estimate for the log10 of the mass (logM_best)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMmax</name><description>Maximum of the logM distribution (logM_max)</description><unit>log(solMass)</unit><ucd>phys.mass;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMmin</name><description>Minimum of the logM distribution (logM_min)</description><unit>log(solMass)</unit><ucd>phys.mass;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMp16</name><description>16th percentile of the logM distribution (logM_p16)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMp25</name><description>25th percentile of the logM distribution (logM_p25)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMmed</name><description>median of the distribution of log10 of the mass (logM_p50)</description><unit>log(solMass)</unit><ucd>phys.mass;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMp75</name><description>75th percentile of the logM distribution (logM_p75)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logMp84</name><description>84th percentile of the logM distribution (logM_p84)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTbest</name><description>multivariate maximum posterior estimate for the log10 of the effective temperature (logT_best)</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTmax</name><description>Maximum of the logT distribution (logT_max)</description><unit>log(K)</unit><ucd>phys.temperature;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTmin</name><description>Minimum of the logT distribution (logT_min)</description><unit>log(K)</unit><ucd>phys.temperature;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTp16</name><description>16th percentile of the logT distribution (logT_p16)</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTp25</name><description>25th percentile of the logT distribution (logT_p25)</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTmed</name><description>median of the distribution of log10 of the effective temperature (logT_p50)</description><unit>log(K)</unit><ucd>phys.temperature;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTp75</name><description>75th percentile of the logT distribution (logT_p75)</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logTp84</name><description>84th percentile of the logT distribution (logT_p84)</description><unit>log(K)</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>loggbest</name><description>multivariate maximum posterior estimate for the log10 of the surface gravity (logg_best)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggmax</name><description>Maximum of the logg distribution (logg_max)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggmin</name><description>Minimum of the logg distribution (logg_min)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggp16</name><description>16th percentile of the logg distribution (logg_p16)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggp25</name><description>25th percentile of the logg distribution (logg_p25)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggmed</name><description>median of the distribution of log10 of the surface gravity (logg_p50)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggp75</name><description>75th percentile of the logg distribution (logg_p75)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggp84</name><description>84th percentile of the logg distribution (logg_p84)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Plx</name><description>Recalibrated parallax (parallax) (2)</description><unit>mas</unit><ucd>pos.parallax</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Plx</name><description>Error in recalibrated parallax (parallax_sigma) (3)</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPbest</name><description>multivariate maximum posterior estimate for the attenuation in the Gaia BP band towards this source (A_BP_best)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPmax</name><description>Maximum of the A_BP distribution (A_BP_max)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPmin</name><description>Minimum of the A_BP distribution (A_BP_min)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPp16</name><description>16th percentile of the A_BP distribution (A_BP_p16)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPp25</name><description>25th percentile of the A_BP distribution (A_BP_p25)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPmed</name><description>median of the distribution of attenuation in the Gaia BP band towards this source (A_BP_p50)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPp75</name><description>75th percentile of the A_BP distribution (A_BP_p75)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABPp84</name><description>84th percentile of the A_BP distribution (A_BP_p84)</description><unit>mag</unit><ucd>phys.absorption;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGbest</name><description>multivariate maximum posterior estimate for the attenuation in the Gaia G band towards this source (A_G_best)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGmax</name><description>Maximum of the A_G distribution (A_G_max)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGmin</name><description>Minimum of the A_G distribution (A_G_min)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGp16</name><description>16th percentile of the A_G distribution (A_G_p16)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGp25</name><description>25th percentile of the A_G distribution (A_G_p25)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGmed</name><description>median of the distribution of attenuation in the Gaia G band towards this source (A_G_p50)</description><unit>mag</unit><ucd>phys.absorption;em.opt;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGp75</name><description>75th percentile of the A_G distribution (A_G_p75)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AGp84</name><description>84th percentile of the A_G distribution (A_G_p84)</description><unit>mag</unit><ucd>phys.absorption;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPbest</name><description>multivariate maximum posterior estimate for the attenuation in the Gaia RP band towards this source (A_RP_best)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPmax</name><description>Maximum of the A_RP distribution (A_RP_max)</description><unit>mag</unit><ucd>phys.absorption;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPp16</name><description>16th percentile of the A_RP distribution (A_RP_p16)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPp25</name><description>25th percentile of the A_RP distribution (A_RP_p25)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPmed</name><description>median of the distribution of attenuation in the Gaia RP band towards this source (A_RP_p50)</description><unit>mag</unit><ucd>phys.absorption;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPp75</name><description>75th percentile of the A_RP distribution (A_RP_p75)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARPp84</name><description>84th percentile of the A_RP distribution (A_RP_p84)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BP</name><description>Recalibrated Gaia BP magnitude (BP) (4)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPbest</name><description>multivariate maximum posterior estimate for the Gaia BP magnitude (BP_best)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmax</name><description>Maximum of the BP distribution (BP_max)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmin</name><description>Minimum of the BP distribution (BP_min)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BPp16</name><description>16th percentile of the BP distribution (BP_p16)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPp25</name><description>25th percentile of the BP distribution (BP_p25)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPmed</name><description>median of the distribution of Gaia BP magnitude (BP_p50)</description><unit>mag</unit><ucd>phot.mag;em.opt.B;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPp75</name><description>75th percentile of the BP distribution (BP_p75)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BPp84</name><description>84th percentile of the BP distribution (BP_p84)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_BP</name><description>Recalibrated error from original Gaia BP magnitude (BP_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>G</name><description>Recalibrated Gaia G magnitude (G) (6)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gbest</name><description>multivariate maximum posterior estimate for the Gaia G magnitude (G_best)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmax</name><description>Maximum of the G distribution (G_max)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmin</name><description>Minimum of the G distribution (G_min)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gp16</name><description>16th percentile of the G distribution (G_p16)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gp25</name><description>25th percentile of the G distribution (G_p25)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gmed</name><description>median of the distribution of Gaia G magnitude (G_p50)</description><unit>mag</unit><ucd>phot.mag;em.opt;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gp75</name><description>75th percentile of the G distribution (G_p75)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gp84</name><description>84th percentile of the G distribution (G_p84)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_G</name><description>Recalibrated error from original Gaia G magnitude (G_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H</name><description>Recalibrated 2MASS H magnitude (H)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Hbest</name><description>multivariate maximum posterior estimate for the 2MASS H magnitude (H_best)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hmax</name><description>Maximum of the H distribution (H_max)</description><unit>mag</unit><ucd>phot.mag;em.IR.H;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hmin</name><description>Minimum of the H distribution (H_min)</description><unit>mag</unit><ucd>phot.mag;em.IR.H;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hp16</name><description>16th percentile of the H distribution (H_p16)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hp25</name><description>25th percentile of the H distribution (H_p25)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hmed</name><description>median of the distribution of 2MASS H magnitude (H_p50)</description><unit>mag</unit><ucd>phot.mag;em.IR.H;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hp75</name><description>75th percentile of the H distribution (H_p75)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Hp84</name><description>84th percentile of the H distribution (H_p84)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_H</name><description>Recalibrated error from original 2MASS H magnitude (H_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J</name><description>Recalibrated 2MASS J magnitude (J)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jbest</name><description>multivariate maximum posterior estimate for the 2MASS J magnitude (J_best)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jmax</name><description>Maximum of the J distribution (J_max)</description><unit>mag</unit><ucd>phot.mag;em.IR.J;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jmin</name><description>Minimum of the J distribution (J_min)</description><unit>mag</unit><ucd>phot.mag;em.IR.J;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jp16</name><description>16th percentile of the J distribution (J_p16)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jp25</name><description>25th percentile of the J distribution (J_p25)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jp75</name><description>75th percentile of the J distribution (J_p75)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jp84</name><description>84th percentile of the J distribution (J_p84)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_J</name><description>Recalibrated error from original 2MASS J magnitude (J_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ks</name><description>Recalibrated 2MASS Ks magnitude (Ks)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ksbest</name><description>multivariate maximum posterior estimate for the 2MASS Ks magnitude (Ks_best)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksmax</name><description>Maximum of the Ks distribution (Ks_max)</description><unit>mag</unit><ucd>phot.mag;em.IR.K;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksmin</name><description>Minimum of the Ks distribution (Ks_min)</description><unit>mag</unit><ucd>phot.mag;em.IR.K;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksp16</name><description>16th percentile of the Ks distribution (Ks_p16)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksp25</name><description>25th percentile of the Ks distribution (Ks_p25)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksmed</name><description>median of the distribution of 2MASS Ks magnitude (Ks_p50)</description><unit>mag</unit><ucd>phot.mag;em.IR.K;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksp75</name><description>75th percentile of the Ks distribution (Ks_p75)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ksp84</name><description>84th percentile of the Ks distribution (Ks_p84)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ks</name><description>Recalibrated error from original 2MASS Ks magnitude (Ks_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RP</name><description>Recalibrated Gaia RP magnitude (RP) (4)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPbest</name><description>multivariate maximum posterior estimate for the Gaia RP magnitude (RP_best)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPmax</name><description>Maximum of the RP distribution (RP_max)</description><unit>mag</unit><ucd>phot.mag;em.opt.R;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPmin</name><description>Minimum of the RP distribution (RP_min)</description><unit>mag</unit><ucd>phot.mag;em.opt.R;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPp16</name><description>16th percentile of the RP distribution (RP_p16)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPp25</name><description>25th percentile of the RP distribution (RP_p25)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPmed</name><description>median of the distribution of Gaia RP magnitude (RP_p50)</description><unit>mag</unit><ucd>phot.mag;em.opt.R;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPp75</name><description>75th percentile of the RP distribution (RP_p75)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RPp84</name><description>84th percentile of the RP distribution (RP_p84)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RP</name><description>Recalibrated error from original (RP) Gaia RP magnitude (RP_sigma) (5)</description><unit>mag</unit><ucd>stat.error;phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1</name><description>Recalibrated error from original (W1) WISE W1 magnitude (5)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1best</name><description>multivariate maximum posterior estimate for the WISE W1 magnitude (W1_best)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1max</name><description>Maximum of the W1 distribution (W1_max)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1min</name><description>Minimum of the W1 distribution (W1_min)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1p16</name><description>16th percentile of the W1 distribution (W1_p16)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1p25</name><description>25th percentile of the W1 distribution (W1_p25)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1med</name><description>median of the distribution of WISE W1 magnitude (W1_p50)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1p75</name><description>75th percentile of the W1 distribution (W1_p75)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>