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<ri:Resource created="2016-08-25T08:43:04Z" 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>Stellar MFP for massive quiescent z&lt;0.7 galaxies</title><shortName>J/ApJ/821/101</shortName><identifier>ivo://CDS.VizieR/J/ApJ/821/101</identifier><altIdentifier>doi:10.26093/cds/vizier.18210101</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zahid H.J.</name></creator><creator><name>Damjanov I.</name></creator><creator><name>Geller M.J.</name></creator><creator><name>Hwang H.S.</name></creator><creator><name>Fabricant D.G.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2016-08-25T08:43:04Z</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-kinematics</subject><subject>absolute-magnitude</subject><description>We examine the evolution of the relation between stellar mass surface density, velocity dispersion, and half-light radius --the stellar mass fundamental plane (MFP)-- for quiescent galaxies at z&lt;0.6. We measure the local relation from galaxies in the Sloan Digital Sky Survey and the intermediate redshift relation from ~500 quiescent galaxies with stellar masses 10&lt;~log(M*/M_{sun}_)&lt;~11.5. Nearly half of the quiescent galaxies in our intermediate redshift sample are compact. After accounting for important selection and systematic effects, the velocity dispersion distribution of galaxies at intermediate redshifts is similar to that of galaxies in the local universe. Galaxies at z&lt;0.6 appear to be smaller (&lt;~0.1dex) than galaxies in the local sample. The orientation of the stellar MFP is independent of redshift for massive quiescent galaxies at z&lt;0.6 and the zero-point evolves by ~0.04dex. Compact quiescent galaxies fall on the same relation as the extended objects. We confirm that compact quiescent galaxies are the tail of the size and mass distribution of the normal quiescent galaxy population.</description><source format="bibcode">2016ApJ...821..101Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/821/101</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/265">VII/265 : COSMOS Morphological Catalog (V1.1) (Tasca+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/578/A134">J/A+A/578/A134 : Compact early-type galaxies in SDSS (Saulder+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/35">J/ApJS/213/35 : SHELS: galaxy redshift survey for R&lt;=20.6 (Geller+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/775/106">J/ApJ/775/106 : CANDELS passive &amp; massive early-type gal. 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