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<ri:Resource created="2011-03-23T14:45:16Z" 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>Ellipticities of cluster early-type galaxies</title><shortName>J/ApJ/693/617</shortName><identifier>ivo://CDS.VizieR/J/ApJ/693/617</identifier><altIdentifier>doi:10.26093/cds/vizier.16930617</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Holden B.P.</name></creator><creator><name>Franx M.</name></creator><creator><name>Illingworth G.D.</name></creator><creator><name>Postman M.</name></creator><creator><name>van der Wel A.,Kelson D.D.</name></creator><creator><name>Blakeslee J.P.</name></creator><creator><name>Ford H.</name></creator><creator><name>Demarco R.</name></creator><creator><name>Mei S.</name></creator><date role="Updated">2018-01-04T08:21:51Z</date><date role="Created">2011-03-23T14:45:16Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>infrared-photometry</subject><subject>photometry</subject><subject>redshifted</subject><description>We have compiled a sample of early-type cluster galaxies from 0&lt;z&lt;1.3 and measured the evolution of their ellipticity distributions. Our sample contains 487 galaxies in 17 z&gt;0.3 clusters with high-quality space-based imaging and a comparable sample of 210 galaxies in 10 clusters at z&lt;0.05. We select early-type galaxies (elliptical and S0 galaxies) that fall within the cluster R_200_, and which lie on the red-sequence in the magnitude range -19.3&gt;M_B_&gt;-21, after correcting for luminosity evolution as measured by the fundamental plane.</description><source format="bibcode">2009ApJ...693..617H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/693/617</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/ApJS/184/271">J/ApJS/184/271 : Photometry of galaxies in 3 clusters (Chiboucas+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/176/374">J/ApJS/176/374 : WARPS-II Cluster catalog. 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