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<ri:Resource created="2024-07-02T07:39:14Z" status="active" updated="2025-05-19T09:50:00Z" 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>LEGA-C parameters for 877 galaxies</title><shortName>J/ApJ/936/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/936/9</identifier><altIdentifier>doi:10.26093/cds/vizier.19360009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Van der Wel A.</name></creator><creator><name>van Houdt J.</name></creator><creator><name>Bezanson R.</name></creator><creator><name>Franx M.</name></creator><creator><name>D'Eugenio F.,Straatman C.</name></creator><creator><name>Bell E.F.</name></creator><creator><name>Muzzin A.</name></creator><creator><name>Sobral D.</name></creator><creator><name>Maseda M.V.</name></creator><creator><name>de Graaff A.,Holden B.P.</name></creator><date role="Updated">2024-11-06T20:27:31Z</date><date role="Created">2024-07-02T07:39:14Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>astrometry</subject><description>Dynamical models for 673 galaxies at z=0.6-1.0 with spatially resolved (long-slit) stellar kinematic data from LEGA-C are used to calibrate virial mass estimates defined as M_vir_=K{sigma}'_*,int_^2^R, with Ka scaling factor, {sigma}'_*,int_ the spatially integrated stellar velocity second moment from the LEGA-C survey, and R the effective radius measured from a Sersic profile fit to Hubble Space Telescope imaging. The sample is representative for M*&gt;3x10^10^M{sun} and includes all types of galaxies, irrespective of morphology and color. We demonstrate that using R=Rsma (the semimajor axis length of the ellipse that encloses 50% of the light) in combination with an inclination correction on {sigma}'_*,int_ produces an unbiased Mvir. We confirm the importance of projection effects on {sigma}'_*,int_ by showing the existence of a similar residual trend between virial mass estimates and inclination for the nearby early-type galaxies in the ATLAS3D survey. Also, as previously shown, when using a Sersic profile-based R estimate, a Sersic index-dependent correction to account for nonhomology in the radial profiles is required. With respect to analogous dynamical models for low-redshift galaxies from the ATLAS3D survey we find a systematic offset of 0.1dex in the calibrated virial constant for LEGA-C, which may be due to physical differences between the galaxy samples or an unknown systematic error. Either way, with our work we establish a common mass scale for galaxies across 8Gyr of cosmic time with a systematic uncertainty of at most 0.1dex.</description><source format="bibcode">2022ApJ...936....9V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/936/9</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/J/MNRAS/414/888">J/MNRAS/414/888 : ATLAS3D project. III. (Emsellem+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/24">J/ApJS/203/24 : Structural param of galaxies in CANDELS (van der Wel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/8">J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/777/18">J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/85">J/ApJ/771/85 : Dyn masses of z~2 quiescent galaxies (van de Sande+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/72">J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/1332">J/MNRAS/454/1332 : SFR in galaxies at redshift z~0.8 (Shetty+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/60">J/ApJ/858/60 : z~0.8 quiescent galaxy kinem from LEGA-C (Bezanson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/476/1765">J/MNRAS/476/1765 : MaNGA E and S galaxies properties (Li+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/27">J/ApJS/239/27 : LEGA-C DR2; galaxies in the COSMOS field (Straatman+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/877/103">J/ApJ/877/103 : Half-mass radii ~7000 galaxies at 1.0&lt;=z&lt;=2.5 (Suess+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/923/11">J/ApJ/923/11 : Stellar kinematics of LEGA-C galaxies (van Houdt+, 2021)</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/ApJ/936/9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/936/9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/936/9</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/936/9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/936/9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/936/9</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/936/9/table1 (*LEGA-C JAM parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/936/9/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/936/9/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/936/9/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>150.3810833</ra><dec>1.7800278</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/6814 6/27247</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/936/9?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/936/9/table1</name><description>*LEGA-C JAM parameters</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LEGA</name><description>[5/4061] LEGA-C DR3 identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>UV</name><description>[4792/260858] Ultra-VISTA identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Lg</name><description>[7.46/11.91] g band luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL/M1</name><description>[-1.18/2.76] log g band Mass-to-light ratio (1)</description><unit>log(solMass.solLum**-1)</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>[13/83] Inclination</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_logL/M1</name><description>[0.02/8.31] The 16% percentile uncertainty in logL/M1</description><unit>log(solMass.solLum**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logL/M1</name><description>[0.02/4.25] The 84% percentile uncertainty in logL/M1</description><unit>log(solMass.solLum**-1)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logL/M2</name><description>[-0.72/10.78] log g band Mass-to-light ratio (2)</description><unit>log(solMass.solLum**-1)</unit><ucd>phys.composition.massLightRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL/M2</name><description>[0.01/0.14] The 16% percentile uncertainty in logL/M2</description><unit>log(solMass.solLum**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_logL/M2</name><description>[0.01/0.16] The 84% percentile uncertainty in logL/M2</description><unit>log(solMass.solLum**-1)</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fDM</name><description>[0.0/0.94] Dark matter fraction</description><ucd>phys.mass;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_fDM</name><description>[0.0/0.7] The 16% percentile uncertainty in fDM</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_fDM</name><description>[0.04/1.0] The 84% percentile uncertainty in fDM</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Betaz</name><description>[-0.27/0.45] Vertical anisotropy (3)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Betaz</name><description>[0.08/0.46] The 16% percentile uncertainty in Betaz</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Betaz</name><description>[0.04/0.4] The 84% percentile uncertainty in Betaz</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_i</name><description>[3/6] The 50% percentile uncertainty in i</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>