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<ri:Resource created="2019-05-03T11:16:00Z" 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>z~0.8 quiescent galaxy kinematics from LEGA-C</title><shortName>J/ApJ/858/60</shortName><identifier>ivo://CDS.VizieR/J/ApJ/858/60</identifier><altIdentifier>doi:10.26093/cds/vizier.18580060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bezanson R.</name></creator><creator><name>van der Wel A.</name></creator><creator><name>Pacifici C.</name></creator><creator><name>Noeske K.</name></creator><creator><name>Barisic I.</name></creator><creator><name>Bell E.F.,Brammer G.B.</name></creator><creator><name>Calhau J.</name></creator><creator><name>Chauke P.</name></creator><creator><name>van Dokkum P.</name></creator><creator><name>Franx M.</name></creator><creator><name>Gallazzi A.,van Houdt J.</name></creator><creator><name>Labbe I.</name></creator><creator><name>Maseda M.V.</name></creator><creator><name>Munos-Mateos J.C.</name></creator><creator><name>Muzzin A.</name></creator><creator><name>van deSande J.</name></creator><creator><name>Sobral D.</name></creator><creator><name>Straatman C.</name></creator><creator><name>Wu P.-F.</name></creator><date role="Updated">2019-07-26T14:15:00Z</date><date role="Created">2019-05-03T11:16:00Z</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>spectroscopy</subject><subject>redshifted</subject><subject>galaxy-classification-systems</subject><subject>galaxy-kinematics</subject><description>We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at z=0.6-1 from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20kpc, or to an average of 2.7Re. Combined with central stellar velocity dispersions ({sigma}0) this provides the first determination of the dynamical state of a sample selected by a lack of star formation activity at large lookback time. The most massive galaxies (M_*_&gt;2x10^11^M_{sun}_) generally show no or little rotation measured at 5 kpc (|V_5_|/{sigma}_0_&lt;0.2 in eight of ten cases), while ~64% of less massive galaxies show significant rotation. This is reminiscent of local fast- and slow- rotating ellipticals and implies that low- and high-redshift quiescent galaxies have qualitatively similar dynamical structures. We compare |V_5_|/{sigma}_0_ distributions at z~0.8 and the present day by re-binning and smoothing the kinematic maps of 91 low-redshift quiescent galaxies from the Calar Alto Legacy Integral Field Area (CALIFA) survey and find evidence for a decrease in rotational support since z~1. This result is especially strong when galaxies are compared at fixed velocity dispersion; if velocity dispersion does not evolve for individual galaxies then the rotational velocity at 5kpc was an average of 94+/-22% higher in z~0.8 quiescent galaxies than today. Considering that the number of quiescent galaxies grows with time and that new additions to the population descend from rotationally supported star-forming galaxies, our results imply that quiescent galaxies must lose angular momentum between z~1 and the present, presumably through dissipationless merging, and/or that the mechanism that transforms star-forming galaxies also reduces their rotational support.</description><source format="bibcode">2018ApJ...858...60B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/858/60</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/A+AS/141/371">J/A+AS/141/371 : Low-mass stars evolutionary tracks (Girardi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/703">J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/665/1067">J/ApJ/665/1067 : Velocities in Cl 0024+16 and MS 0451-03 (Moran+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/382/109">J/MNRAS/382/109 : Massive galaxies in Extended Groth Strip (Trujillo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/1364">J/ApJ/706/1364 : SINS survey of high-redshift gal. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>[80755/240174] Muzzin+ (2013, J/ApJS/206/8) UltraVISTA catalog (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>zspec</name><description>[0.5/1.1] Spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM</name><description>[10.2/11.6] log_10 Stellar (Mass/M_sun) (2)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Re</name><description>[0.07/2.6] Effective radius along the major axis</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Re</name><description>[0/0.04] Uncertainty in Re</description><unit>arcsec</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>q</name><description>[0.2/1] Projected axis ratio, b/a</description><ucd>phys.size.axisRatio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_q</name><description>[0/0.01] Uncertainty in q</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>[-45/45] Major axis position angle, east of north</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PA</name><description>[0.1/1.5] Uncertainty in PA</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n</name><description>[0.5/6] Sersic Index</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_n</name><description>[0.01/0.3] Uncertainty in n</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V5</name><description>[-164/154] Average line-of-sight rot. velocity at 5kpc</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V5</name><description>[1/23]? 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