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<ri:Resource created="2013-03-06T15:36:57Z" status="active" updated="2025-06-13T15:25:00Z" 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>BCG C4 cluster catalog</title><shortName>J/MNRAS/379/867</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/379/867</identifier><altIdentifier>doi:10.26093/cds/vizier.73790867</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>von der Linden A.</name></creator><creator><name>Best P.N.</name></creator><creator><name>Kauffmann G.</name></creator><creator><name>White S.D.M.</name></creator><date role="Updated">2024-07-05T20:15:16Z</date><date role="Created">2013-03-06T15:36:57Z</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>galaxy-kinematics</subject><description>We use the Sloan Digital Sky Survey (SDSS) to construct a sample of 625 brightest group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in stellar mass, redshift and colour. We investigate how the systematic properties of BCGs depend on stellar mass and on their privileged location near the cluster centre. The groups and clusters that we study are drawn from the C4 catalogue of Miller et al. (2005, Cat. &lt;J/AJ/130/968&gt;) but we have developed improved algorithms for identifying the BCG and for measuring the cluster velocity dispersion. 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