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<ri:Resource created="2026-04-01T09:31:08Z" status="active" updated="2026-05-04T07:43:19Z" 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>AGB Carbon rich stars SED fitting results</title><shortName>J/A+A/708/A120</shortName><identifier>ivo://CDS.VizieR/J/A+A/708/A120</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liberatori A.</name></creator><creator><name>Hatzidimitriou D.</name></creator><creator><name>Antoniadis K.</name></creator><creator><name>Pastorelli G.,Trabucchi M.</name></creator><creator><name>Groenewegen M.A.T.</name></creator><creator><name>Bossini D.</name></creator><creator><name>Girardi L.</name></creator><creator><name>Marigo P.,Bressan A.</name></creator><creator><name>Kallimanis I.N.</name></creator><creator><name>Costa G.</name></creator><creator><name>Katsis V.</name></creator><creator><name>Vasilopoulos G.,Chatzipetros S.</name></creator><date role="Updated">2026-05-04T07:43:19Z</date><date role="Created">2026-04-01T09:31:08Z</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>carbon-stars</subject><subject>late-type-stars</subject><subject>stellar-mass-loss</subject><subject>stellar-evolutionary-models</subject><subject>visible-astronomy</subject><description>Carbon stars on the asymptotic giant branch are major contributors to the dust enrichment of galaxies, with gas mass-loss rate values up to dM/dt=10^-4^M_[sun}_/yr. They represent the final evolutionary stage of low- and intermediate-mass stars, during which recurrent dredge-up episodes enrich their atmospheres with carbon and trigger the formation of dust. Through their intense winds, they inject large amounts of newly formed carbonaceous dust into the interstellar medium, playing a central role in the chemical evolution of galaxies. Their stellar and dust properties have been studied for decades, with a particular focus on the carbon stars in the Magellanic Clouds (MCs). Our aim is to homogeneously analyse the Gaia DR3 Golden Sample of Carbon Stars through the spectral energy distribution (SED) fitting. Our focus is on sources belonging to the Milky Way (MW) and the MCs. Our dataset consists of 14747 stars with complete multi-band photometry from Gaia, 2MASS, and WISE, combined with recent distance and extinction estimates. For a subsample of Mira variables made of 2494 stars, we also modelled multi-band light curves to obtain accurate mean magnitudes. Stellar and circumstellar properties were derived by fitting the observations with a large grid of synthetic models computed with the DUSTY radiative transfer code, using COMARCS model atmospheres as input. For each target, we determined stellar and dust parameters such as the effective temperature, optical depth, and gas mass-loss rate. The resulting distributions reveal typical effective temperatures of around 3150K. Mass-loss rates range from 10^-11^ to 10^-4^M_{sun}_/yr. The average dust temperature at the inner bound of the dust shell is about Td=1000K. We also observe a correlation between photometric variability amplitude and mass-loss rate. This homogeneous framework provides a unified view of carbon stars across environments spanning a wide range of metallicities, supported by strong statistical coverage. Our results show that some of the physical properties of carbon stars exhibit a dependence on the galactic environment. However, these dependences do not necessarily reflect intrinsic metallicity effects, but are influenced by differences in luminosity distributions and by the selection biases affecting the available samples. The use of Gaia and WISE introduces combined selection effects that are significant, limiting the detection of both the most dust-enshrouded objects and the less luminous sources in the Magellanic Clouds. While this limits the completeness of the comparison, the observed trends remain statistically robust within the selected samples.</description><source format="bibcode">2026A&amp;A...708A.120L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A120</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 source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+, 2013)</relatedResource><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/J/A+A/661/A147">J/A+A/661/A147 : Galactic interstellar dust Gaia-2MASS 3D maps</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/708/A120</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/708/A120</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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37838 37841 37845 37847 37853 37856 37858-37859 37868-37869 37871 37877 37879-37880 37882 37885 37887 37897 37901-37903 37920 37922-37923 37932-37933 37944 37946-37947 37949-37952 37954-37956 37966 37968 37975 37985 37988-37989 37992 37994-37995 37998-37999 38014 38016-38018 38024-38025 38028 38031 38042-38043 38046-38047 38049-38051 38060-38062 38065 38068 38074 38078 38082-38083 38088 38090 38113 38117 38120 38126 38128 38139 38155 38167 38186 38255 38304 38412-38414 38416-38417 38424 38426-38428 38433-38434 38436 38444-38445 38461 38466 38479 38504-38505 38525 38528-38529 38531-38532 38534 38537-38541 38548 38552 38554-38556 38562 38567-38568 38571-38572 38580 38583 38586 38592 38594 38596 38602 38609 38614 38617 38624 38637 38648 38656 38660 38699 38789 38916 38918-38919 38944 38946 38953 38998-38999 39028 39039 39134 39141 39148 39157 39173 39175 39185-39187 39193 39195-39197 39199 39201 39205 39208-39209 39211 39216-39217 39224 39227-39228 39231 39237-39238 39248 39251 39253-39254 39261-39263 39269-39273 39275 39278-39280 39282 39284 39286-39287 39289-39292 39294-39295 39300 39302-39303 39305 39307 39309 39311 39313-39315 39321-39323 39328-39329 39335-39336 39342 39345-39346 39356-39358 39362-39366 39372-39374 39376 39378 39381-39382 39390-39391 39396 39398-39399 39409-39411 39415 39440 39487 39518 39523 39527 39529 39540 39546 39548 39622 39675 39681 39686 39697-39700 39702 39705 39708-39709 39711 39716 39719 39722 39726 39748 39750-39751 39764 39766-39768 39770-39772 39775 39784-39785 39787 39789-39791 39795 39800-39802 39807 39828-39829 39831 39834-39835 39840 39842 39855 39857-39858 39860 39862 39864 39869 39871 39873-39877 39884-39886 39888 39890-39892 39894 39896-39898 39904 39906 39912-39913 39915-39917 39920 39922 39928 39930-39931 39936 39944-39945 39947 39949 39951 39955 39962 39968-39969 39971 39974 39977-39979 39985 39991 39995 40022 40032 40064 40066 40069 40072 40075 40078 40084 40087 40089 40093 40097-40099 40101 40103 40106-40107 40110 40115 40120-40122 40128 40139 40150 40168 40235 40244 40339 40360-40361 40392 40448-40449 40458 40460-40462 40467 40471 40476 40480 40482 40488-40489 40491 40501 40504 40506 40508 40510 40523 40549 40552 40559 40576-40577 40579 40581 40584-40586 40588 40590 40592 40597-40598 40601-40603 40616 40618 40620-40621 40626-40627 40631 40633 40635 40641 40658 40664 40666 40690-40691 40703 40756 40762 40788 40832 40836 40863 40869 40875 40967 41202 41204 41215 41266 41314 41335 41367 41381 41384 41387 41390-41391 41396 41406 41435 41440 41446 41453-41455 41458 41460 41462 41481 41488 41502 41504 41519 41533 41535 41542 41544-41545 41550 41554 41556 41558-41560 41563-41564 41567 41570-41573 41575 41592-41594 41596 41603 41608 41614-41615 41617-41619 41633-41635 41652-41654 41656-41658 41660-41661 41663 41668-41670 41678-41680 41687 41689-41691 41696-41697 41699-41700 41702-41703 41705-41708 41716 41719 41721-41723 41728 41731 41733-41734 41747 41750-41754 41756 41758-41759 41764-41766 41771 41775 41782 41785-41787 41790 41796-41798 41800 41807-41809 41812 41827 41830-41831 41834-41836 41841-41842 41844 41846-41847 41851 41854-41857 41859 41861-41863 41868 41872-41874 41881 41883-41884 41888 41894 41900 41904 41910 41913 41920-41921 41924-41925 41934 41937 41944 41949 41955 41965 42018 42045 42047 42057 42079 42081 42088-42089 42098 42109 42120 42122 42126-42127 42135 42137 42139 42144 42146-42147 42149-42151 42156-42158 42164-42166 42168-42169 42176 42181 42183-42185 42189-42191 42194-42196 42198 42201-42206 42208-42209 42213-42214 42218-42220 42222 42226-42228 42231-42232 42234-42236 42248 42274 42279 42283 42287 42291 42294 42296 42299 42309 42316 42319 42323 42325 42330 42333 42339 42341-42343 42345-42347 42368-42369 42377 42386 42389-42390 42398 42400-42402 42406-42407 42410 42413-42416 42418-42419 42421-42423 42425-42430 42432 42434-42435 42440 42444 42447-42448 42450 42452 42458 42464 42466-42467 42471 42474 42476 42478 42484 42486-42487 42500 42502-42503 42506-42508 42510-42511 42521 42526-42527 42529 42532-42533 42536-42537 42540 42547-42549 42558 42560-42561 42563 42569-42570 42572-42573 42577 42579 42584-42585 42589 42602 42612 42614 42629 42643 42694-42695 42717 42719 42740 42755-42758 42769-42771 42773 42776-42777 42783-42784 42787-42788 42790 42796 42801 42806-42807 42816 42819-42821 42826 42828 42831-42833 42835 42844-42846 42864 42868 42871 42876 42906-42907 42909 42932 42952 42962 42965 42976 42981 42996 43027 43029-43031 43034-43035 43039 43044-43046 43056 43059 43066 43073-43074 43081 43087-43089 43096-43097 43100 43104-43105 43136-43138 43141 43144-43145 43150 43154 43161 43163 43168 43174 43176-43177 43194 43203 43264-43265 43281-43282 43292 43300-43301 43320 43342 43522 43526 43532-43533 43572 43650 43703 43799 44310 44867 44898 45146 45279 45380 45658 46037 46215 46513 46729 46834 47039 47138 47266 47376 47542 47664 47717 47754 47757 47781 47802 47832 47855 47860 47865 47868 47871 47885 47894 47897 47903 47911 47917 47919 47925 47927 47947 47961 47968-47969 47978 47993 48001-48003 48005-48009 48011 48019-48020 48025-48026 48033-48034 48044 48046 48050 48056 48062 48064 48067 48216 48679 48690 48761 48787 48813 48847-48848</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/708/A120?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/708/A120/catalog</name><description>Catalogue of stellar and dust parameters (table 3)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>AllWISE</name><description>AllWISE ID (AllWISE_id)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>LMC</name><description>[0/1] True = Large Magellanic Cloud member (lmc)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Windex</name><description>Gaia-2MASS Wesenheit index (Wesenheit_function)</description><unit>mag</unit><ucd>phot.color.reddFree</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>2MASS</name><description>2MASS ID (2MASS_id)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>GaiaDR3</name><description>Gaia DR3 unique source identifier (GaiaDR3_ID)</description><ucd>meta.id;meta.main</ucd></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2016) (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>e_RA_ICRS</name><description>Uncertainty in right ascension (ra_error)</description><unit>deg</unit><ucd>stat.error;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2016) (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>e_DE_ICRS</name><description>Uncertainty in declination (dec_error)</description><unit>deg</unit><ucd>stat.error;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>plx</name><description>Gaia parallax (parallax)</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_plx</name><description>Uncertainty in Gaia parallax (parallax_error)</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PM</name><description>Total proper motion from Gaia (pm)</description><unit>mas/yr</unit><ucd>pos.pm</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRA</name><description>Proper motion in right ascension from Gaia (pmra)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmRA</name><description>Uncertainty in pmra from Gaia (pmra_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>Proper motion in declination from Gaia (pmdec)</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmDE</name><description>Uncertainty in pmdec from Gaia (pmdec_error)</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Distpc</name><description>Distance from parallax or adopted value from Bailer-Jones et al. (2021AJ....161..147B, Cat. I/352) (distance_pc)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ext</name><description>Line-of-sight extinction from Lallement et al. (2022A&amp;A...661A.147L, Cat. J/A+A/661/A147) 3D maps (ext)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Ext</name><description>Uncertainty in extinction (exterr)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>minchi2r</name><description>Minimum chi2 value from SED fit (MinChisquared)</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Teff</name><description>Effective temperature (Teff)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tdust</name><description>Inner dust shell temperature (Tdust)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Stellar mass (Mass)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AmC</name><description>Fraction of amorphous carbon dust (always 1.0) (AmC)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lbol</name><description>Bolometric luminosity (Lbol)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>tau</name><description>Optical depth (tau at 0.55um) (Tau)</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>C/O</name><description>Carbon-to-oxygen ratio (C/O)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>logtau</name><description>Logarithmic optical depth (tau at 0.55um) (Tau_log)</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dM/dt</name><description>Gas mass-loss rate (Mass_Loss_Rate)</description><unit>solMass/yr</unit><ucd>arith.rate</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>log(dM/dt)</name><description>Logarithmic gas mass-loss rate (Mass_Loss_Rate_log)</description><unit>log(solMass.yr**-1)</unit><ucd>arith.rate</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_minchi2r</name><description>Uncertainty on minimum chi2 (MinChisquared_sigma)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Teff</name><description>Uncertainty in effective temperature (Teff_sigma)</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Tdust</name><description>Uncertainty in inner dust shell temperature (Tdust_sigma)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Mass</name><description>Uncertainty in stellar mass (Mass_sigma)</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_logtau</name><description>Uncertainty in log optical depth (Tau_sigma_log)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_log(dM/dt)</name><description>Uncertainty in log(Mass-Loss Rate) (Mass_Loss_Rate_sigma_log)</description><unit>log(solMass.yr**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>meanFluxR</name><description>Mean observed/model flux ratio for all filters used in the fit (offset_observ_over_bestmodel)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MW</name><description>[0/1] True = Milky Way member (mw)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>SMC</name><description>[0/1] True = Small Magellanic Cloud member (smc)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Period</name><description>? Pulsation period from multiband light curve fit (Period)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Gmaglc</name><description>? Mean G magnitude from light curve fit (Gmag_lcurve)</description><unit>mag</unit><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>BPmaglc</name><description>? Mean BP magnitude from light curve fit (BPmag_lcurve)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RPmaglc</name><description>? Mean RP magnitude from light curve fit (RPmag_lcurve)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>AmpBP</name><description>? Gaia BP-band amplitude from light curve fit (BP_Amplitude)</description><unit>mag</unit><ucd>src.var.amplitude;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>AmpRP</name><description>? Gaia RP-band amplitude from light curve fit (RP_Amplitude)</description><unit>mag</unit><ucd>src.var.amplitude;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>AmpG</name><description>? Gaia G-band amplitude from light curve fit (G_Amplitude)</description><unit>mag</unit><ucd>src.var.amplitude;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Mira</name><description>[0/1]? 1 = identified Mira variable (Mira)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>BPMAG</name><description>Absolute BP magnitude (M_BP)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPMAG</name><description>Absolute RP magnitude (M_RP)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>GMAG</name><description>Absolute G magnitude (M_G)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>JMAG</name><description>Absolute J magnitude (M_J)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HMAG</name><description>Absolute J magnitude (M_H)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1MAG</name><description>Absolute W1 magnitude (M_W1)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W2MAG</name><description>Absolute W2 magnitude (M_W2)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W3MAG</name><description>Absolute W3 magnitude (M_W3)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W4MAG</name><description>Absolute W4 magnitude (M_W4)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>KMAG</name><description>Absolute K magnitude (M_K)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Gmag</name><description>Uncertainty in G magnitude (e_Gmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_BPmag</name><description>Uncertainty in BP magnitude (e_BPmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RPmag</name><description>Uncertainty in RP magnitude (e_RPmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Jmag</name><description>? Uncertainty in J magnitude (e_Jmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>? Uncertainty in H magnitude (e_Hmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Kmag</name><description>? Uncertainty in K magnitude (e_Kmag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W1mag</name><description>? Uncertainty in W1 magnitude (e_W1mag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W2mag</name><description>? Uncertainty in W2 magnitude (e_W2mag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W3mag</name><description>? Uncertainty in W3 magnitude (e_W3mag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W4mag</name><description>? Uncertainty in W4 magnitude (e_W4mag)</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>OGLE</name><description>OGLE ID (if available) (OGLE_ID)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column></table></schema></tableset></ri:Resource>