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<ri:Resource created="2024-02-19T14:41:20Z" 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>Stellar parameters from Gaia DR3</title><shortName>J/A+A/669/A104</shortName><identifier>ivo://CDS.VizieR/J/A+A/669/A104</identifier><altIdentifier>doi:10.26093/cds/vizier.36690104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kordopatis G.</name></creator><creator><name>Schultheis M.</name></creator><creator><name>McMillan P.J.</name></creator><creator><name>Palicio P.A.</name></creator><creator><name>de Laverny P.,Recio-Blanco A.</name></creator><creator><name>Creevey O.</name></creator><creator><name>Alvarez M.A.</name></creator><creator><name>Andrae R.</name></creator><creator><name>Poggio E.</name></creator><creator><name>Spitoni E.,Contursi G.</name></creator><creator><name>Zhao H.</name></creator><creator><name>Oreshina-Slezak I.</name></creator><creator><name>Ordenovic C.</name></creator><creator><name>Bijaoui A.</name></creator><date role="Updated">2024-11-06T20:01:59Z</date><date role="Created">2024-02-19T14:41:20Z</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>milky-way-galaxy</subject><subject>standard-stars</subject><subject>radial-velocity</subject><subject>astrometry</subject><description>Gaia's third data release provides radial velocities for 33 million stars and spectroscopically derived atmospheric parameters for more than 5 million targets. When combined with the astrometric data, these allow us to derive orbital and stellar parameters that are key to understanding the stellar populations of the Milky Way and to perform Galactic archaeology. We used the calibrated atmospheric parameters, 2MASS and Gaia-EDR3 photometry, and parallax-based distances to compute the ages, initial stellar masses, and reddenings for the stars with spectroscopic parameters. We also derived the orbits for all of the stars with measured radial velocities and astrometry, adopting two sets of line-of-sight distances from the literature. Four different sets of ages, masses, and absolute magnitudes in different photometric bands are obtained through an isochrone fitting method, considering different combinations of input parameters. The reddenings are obtained by comparing the observed colours with those obtained from the isochrone projection. Finally, the orbits are computed adopting an axisymmetric potential of the Galaxy. Comparisons with reference catalogues of field and cluster stars suggest that reliable ages are obtained for stars younger than 9-10Gyr when the estimated relative age uncertainty is &lt;50 per cent. For older stars, ages tend to be underestimated. The most reliable stellar type for age determination are turn-off stars, even when the input atmospheric parameters have large uncertainties. Ages for giants and main-sequence stars are retrieved with uncertainties of the order of 2Gyr when extinction towards the star's line of sight is less than A_V_&lt;~2.5mag. The catalogue of ages, initial stellar masses, reddenings, galactocentric positions and velocities, as well as the stellar orbital actions, eccentricities, apocentre, pericentre and maximum distance from the Galactic plane reached during their orbits, is made publicly available to be downloaded. With this catalogue, the full chemo-dynamical properties of the extended solar neighbourhood unfold and allow us to better identify the properties of the spiral arms, to parametrise the dynamical heating of the disc, and to thoroughly study the chemical enrichment of the Milky Way.</description><source format="bibcode">2023A&amp;A...669A.104K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/669/A104</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/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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Lower confidence limit of rperidpgeo (rperi_lo_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GMAGspeck</name><description>? rms uncertainty on GMAGspeck (G_error_speck)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GaiaDR3</name><description>Gaia DR3 source ID (source_id)</description><ucd>meta.id;meta.main</ucd><flag>indexed</flag></column><column><name>RA_ICRS</name><description>Gaia DR3 right ascension (ICRS) at ep=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Gaia DR3 declination (ICRS) at ep=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Xdgeo</name><description>? Median galactocentric Cartesian X position (X_med_dgeo)</description><unit>kpc</unit><ucd>pos.cartesian.x;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Xdgeo</name><description>? Lower confidence limit of Xdgeo (X_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Xdgeo</name><description>? Upper confidence limit of Xdgeo (X_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Ydgeo</name><description>? Median galactocentric Cartesian Y position (Y_med_dgeo)</description><unit>kpc</unit><ucd>pos.cartesian.y;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Ydgeo</name><description>? Lower confidence limit of Ydgeo (Y_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Ydgeo</name><description>? Upper confidence limit of Ydgeo (Y_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Zdgeo</name><description>? Median galactocentric Cartesian Z position (Z_med_dgeo)</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Zdgeo</name><description>? Lower confidence limit of Zdgeo (Z_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Zdgeo</name><description>? Upper confidence limit of Zdgeo (Z_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rdgeo</name><description>? Median heliocentric line-of-sight distance with geometric prior from Bailer-Jones et al. (2021, Cat. I/352) (r_med_dgeo)</description><unit>kpc</unit><ucd>pos.distance;em.wl.central;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_rdgeo</name><description>? Lower confidence limit of rdgeo (r_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_rdgeo</name><description>? Upper confidence limit of rdgeo (r_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VRdgeo</name><description>? Median galactocentric radial velocity obtained using r_med_dgeo (VR_med_dgeo)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_VRdgeo</name><description>? Lower confidence limit of VRdgeo (VR_lo_dgeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_VRdgeo</name><description>? Upper confidence limit of VRdgeo (VR_hi_dgeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Vphidgeo</name><description>? 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Median galactocentric vertical velocity obtained using r_med_dgeo (VZ_med_dgeo)</description><unit>km/s</unit><ucd>phys.veloc;em.wl.central;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_rpgeo</name><description>? Upper limit of the photogeometric distance posterior (99999.999 for infinity) (r_hi_photogeo)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_VZdgeo</name><description>? Lower confidence limit of VZdgeo (VZ_lo_dgeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_VZdgeo</name><description>? Upper confidence limit of VZdgeo (VZ_hi_dgeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>edgeo</name><description>? Median eccentricity, obtained using r_med_dgeo (e_med_dgeo)</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_edgeo</name><description>? Lower confidence limit of edgeo (e_lo_dgeo)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_edgeo</name><description>? Upper confidence limit of edgeo (e_hi_dgeo)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Zmaxdgeo</name><description>? Median maximum distance from the galactic plane obtained using r_med_dgeo (Zmax_med_dgeo)</description><unit>kpc</unit><ucd>pos.cartesian.z;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Zmaxdgeo</name><description>? Lower confidence limit of Zmaxdgeo (Zmax_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Zmaxdgeo</name><description>? Upper confidence limit of Zmaxdgeo (Zmax_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rperidgeo</name><description>? 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Median apogalactic radius reached by the star, obtained using r_med_dgeo (rapo_med_dgeo)</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_rapodgeo</name><description>? Lower confidence limit of rapodgeo (rapo_lo_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_rapodgeo</name><description>? Upper confidence limit of rapodgeo (rapo_hi_dgeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Jrdgeo</name><description>? Median radial action obtained using r_med_dgeo (Jr_med_dgeo)</description><unit>km.kpc/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Jrdgeo</name><description>? Lower confidence limit of Jrdgeo (Jr_lo_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Jrdgeo</name><description>? Upper confidence limit of Jrdgeo (Jr_hi_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lzdgeo</name><description>? Median angular momentum in z-direction obtained using r_med_dgeo (Lz_med_dgeo)</description><unit>km.kpc/s</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Lzdgeo</name><description>? Lower confidence limit of Lzdgeo (-9999.99 for infinity) (Lz_lo_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Lzdgeo</name><description>? Upper confidence limit of Lzdgeo (Lz_hi_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Jzdgeo</name><description>? Median radial action obtained using r_med_dgeo (Jz_med_dgeo)</description><unit>km.kpc/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Jzdgeo</name><description>? Lower confidence limit of Jzdgeo (Jz_lo_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Jzdgeo</name><description>? Upper confidence limit of Jzdgeo (Jz_hi_dgeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Xdpgeo</name><description>? 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Upper confidence limit of Rdpgeo (r_hi_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VRdpgeo</name><description>? Median galactocentric radial velocity obtained using r_med_dpgeo (VR_med_dphotogeo)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_VRdpgeo</name><description>? Lower confidence limit of VRdpgeo (VR_lo_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_VRdpgeo</name><description>? Upper confidence limit of VRdpgeo (VR_hi_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Vphidpgeo</name><description>? Median galactocentric azimuthal velocity obtained using r_med_dpgeo (Vphi_med_dphotogeo)</description><unit>km/s</unit><ucd>phys.veloc;em.wl.central;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Vphidpgeo</name><description>? Lower confidence limit of Vphidpgeo (Vphi_lo_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Vphidpgeo</name><description>? Upper confidence limit of Vphidpgeo (Vphi_hi_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>VZdpgeo</name><description>? Median galactocentric azimuthal velocity obtained using r_med_dpgeo (VZ_med_dphotogeo)</description><unit>km/s</unit><ucd>phys.veloc;em.wl.central;stat.median</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_VZdpgeo</name><description>? Lower confidence limit of VZdpgeo (VZ_lo_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_VZdpgeo</name><description>? Upper confidence limit of VZdpgeo (VZ_hi_dphotogeo)</description><unit>km/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>edpgeo</name><description>? Median eccentricity, obtained using r_med_dpgeo (e_med_dphotogeo)</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_edpgeo</name><description>? Lower confidence limit of edpgeo (e_lo_dphotogeo)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_edpgeo</name><description>? Upper confidence limit of edpgeo (e_hi_dphotogeo)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Zmaxdpgeo</name><description>? Median maximum distance from the galactic plane obtained using r_med_dpgeo (Zmax_med_dphotogeo)</description><unit>kpc</unit><ucd>pos.cartesian.z;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Zmaxdpgeo</name><description>? Lower confidence limit of Zmaxdpgeo (Zmax_lo_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Zmaxdpgeo</name><description>? Upper confidence limit of Zmaxdpgeo (Zmax_hi_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rperidpgeo</name><description>? Median perigalactic radius reached by the star, obtained using r_med_dpgeo (rperi_med_dphotogeo)</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_rperidpgeo</name><description>? Upper confidence limit of rperidpgeo (rperi_hi_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>rapodpgeo</name><description>? Median apogalactic radius reached by the star, obtained using r_med_dpgeo (rapo_med_dphotogeo)</description><unit>kpc</unit><ucd>pos.distance;src.orbital</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_rapodpgeo</name><description>? Lower confidence limit of rapodpgeo (rapo_lo_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_rapodpgeo</name><description>? Upper confidence limit of rapodpgeo (rapo_hi_dphotogeo)</description><unit>kpc</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Jrdpgeo</name><description>? Median radial action obtained using r_med_dpgeo (Jr_med_dphotogeo)</description><unit>km.kpc/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Jrdpgeo</name><description>? Lower confidence limit of Jrdpgeo (Jr_lo_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Jrdpgeo</name><description>? Upper confidence limit of Jrdpgeo (Jr_hi_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lzdpgeo</name><description>? Median angular momentum in z-direction obtained using r_med_dpgeo (Lz_med_dphotogeo)</description><unit>km.kpc/s</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Lzdpgeo</name><description>? Lower confidence limit of Lzdpgeo (Lz_lo_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Lzdpgeo</name><description>? Upper confidence limit of Lzdpgeo (Lz_hi_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Jzdpgeo</name><description>? Median vertical action obtained using r_med_dpgeo (Jz_med_dphotogeo)</description><unit>km.kpc/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Jzdpgeo</name><description>? Lower confidence limit of Jzdpgeo (Jz_lo_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>B_Jzdpgeo</name><description>? Upper confidence limit of Jzdpgeo (Jz_hi_dphotogeo)</description><unit>km.kpc/s</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teffspec</name><description>? Projected Teff adopting the calibrated GSP-Spec parameters only (Teff_spec)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>loggspec</name><description>? Projected logg adopting the calibrated GSP-Spec parameters only (logg_spec)</description><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>metaspec</name><description>? Projected [M/H] adopting the calibrated GSP-Spec parameters only (meta_spec)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>agespec</name><description>? Inferred age adopting the calibrated GSP-Spec parameters only (age_spec)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_agespec</name><description>? rms uncertainty on agespec (age_error_spec)</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Minispec</name><description>? Inferred initial stellar mass adopting the calibrated GSP-Spec parameters only (M_ini_spec)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Minispec</name><description>? rms uncertainty on (M_ini_error_spec)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAGspec</name><description>? Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters only (G_spec)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPMAGspec</name><description>? Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters only (G_BP_spec)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPMAGspec</name><description>? Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters only (G_RP_spec)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GMAGspec</name><description>? rms uncertainty on GMAGspec (G_error_spec)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_BPMAGspec</name><description>? rms uncertainty on BPMAGspec (G_BP_error_spec)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RPMAGspec</name><description>? rms uncertainty on RPMAGspec (G_RP_error_spec)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teffspecjhk</name><description>? Projected Teff adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (Teff_specjhk)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>loggspecjhk</name><description>? Projected logg adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (logg_specjhk)</description><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>metaspecjhk</name><description>? Projected [M/H] adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (meta_specjhk)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPMAGspecjhk</name><description>? Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (G_RP_specjhk)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GMAGspecjhk</name><description>? rms uncertainty on GMAGspecjhk (G_error_specjhk)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_BPMAGspecjhk</name><description>? rms uncertainty on BPMAGspecjhk (G_BP_error_specjhk)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RPMAGspecjhk</name><description>? rms uncertainty on RPMAGspecjhk (G_RP_error_specjhk)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>agespecjhk</name><description>? Inferred age adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (age_specjhk)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_agespecjhk</name><description>? rms uncertainty on adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (age_error_specjhk)</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Minispecjhk</name><description>? Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (M_ini_specjhk)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Minispecjhk</name><description>? rms uncertainty on Minispecjhk (M_ini_error_specjhk)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAGspecjhk</name><description>? Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (G_specjhk)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPMAGspecjhk</name><description>? Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks absolute magnitudes (G_BP_specjhk)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teffspecjhkg</name><description>? Projected Teff adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (Teff_specjhkg)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>loggspecjhkg</name><description>? Projected logg adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (logg_specjhkg)</description><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>metaspecjhkg</name><description>? Projected [M/H] adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (meta_specjhkg)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>agespecjhkg</name><description>? Inferred age adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (age_specjhkg)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_agespecjhkg</name><description>? rms uncertainty on agespecjhkg (age_error_specjhkg)</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Minispecjhkg</name><description>? Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (M_ini_specjhkg)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Minispecjhkg</name><description>? rms uncertainty on Minispecjhkg (M_ini_error_specjhkg)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAGspecjhkg</name><description>? Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (G_specjhkg)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPMAGspecjhkg</name><description>? Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (G_BP_specjhkg)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPMAGspecjhkg</name><description>? Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the J;H;Ks;G absolute magnitudes (G_RP_specjhkg)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GMAGspecjhkg</name><description>? rms uncertainty on GMAGspecjhkg (G_error_specjhkg)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_BPMAGspecjhkg</name><description>? rms uncertainty on BPMAGspecjhkg (G_BP_error_specjhkg)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RPMAGspecjhkg</name><description>? rms uncertainty on RPMAGspecjhkg (G_RP_error_specjhkg)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teffspeck</name><description>? Projected Teff adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (Teff_speck)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>loggspeck</name><description>? Projected logg adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (logg_speck)</description><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>metaspeck</name><description>? Projected [M/H] adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (meta_speck)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>agespeck</name><description>? Inferred age adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (age_speck)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_agespeck</name><description>? rms uncertainty on agespeck (age_error_speck)</description><unit>Gyr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Minispeck</name><description>? Inferred initial stellar mass adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (M_ini_speck)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Minispeck</name><description>? rms uncertainty on Minispeck (M_ini_error_speck)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAGspeck</name><description>? Inferred absolute G magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (G_speck)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPMAGspeck</name><description>? Inferred absolute BP magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (G_BP_speck)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPMAGspeck</name><description>? Inferred absolute RP magnitude adopting the calibrated GSP-Spec parameters and the Ks absolute magnitude (G_RP_speck)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_BPMAGspeck</name><description>? rms uncertainty on BPMAGspeck (G_BP_error_speck)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RPMAGspeck</name><description>? rms uncertainty on RPMAGspeck (G_RP_error_speck)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Teff</name><description>? Adopted projected Teff (Teff)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logg</name><description>? Adopted projected logg (logg)</description><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>meta</name><description>? Adopted projected [M/H] (meta)</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>age</name><description>? Inferred age (age)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_age</name><description>? rms uncertainty on age (age_error)</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mini</name><description>? Inferred initial stellar mass (M_ini)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Mini</name><description>? rms uncertainty on Mini (M_ini_error)</description><unit>solMass</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMAG</name><description>? Inferred absolute G magnitude (G)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPMAG</name><description>? Inferred absolute BP magnitude (G_BP)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPMAG</name><description>? Inferred absolute RP magnitude (G_RP)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_GMAG</name><description>? rms uncertainty on GMAG (G_error)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_BPMAG</name><description>? rms uncertainty on BPMAG (G_BP_error)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RPMAG</name><description>? rms uncertainty on RPMAG (G_RP_error)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E(BP-RP)</name><description>? Inferred reddening using the projected GBP and GRP (EBPRP)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_E(BP-RP)</name><description>? rms uncertainty on E(BP-RP) (EBPRP_error)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>pflavour</name><description>Adopted projection flavour for inferred ages and masses (spec, specjhk, specjhkg, speck or nan) (pflavour)</description><ucd>pos.cartesian</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>rgeo</name><description>Median of the geometric distance posterior (r_med_geo)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_rgeo</name><description>Lower limit of the geometric distance posterior (r_lo_geo)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_rgeo</name><description>Upper limit of the geometric distance posterior (r_hi_geo)</description><unit>pc</unit><ucd>pos.distance;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rpgeo</name><description>? Median of the photogeometric distance posterior (r_med_photogeo)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_rpgeo</name><description>? Lower limit of the photogeometric distance posterior (r_lo_photogeo)</description><unit>pc</unit><ucd>pos.distance;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>