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<ri:Resource created="2009-05-16T23:49:51Z" 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>Radial kinematics in bright cluster galaxies</title><shortName>J/MNRAS/391/1009</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/391/1009</identifier><altIdentifier>doi:10.26093/cds/vizier.73911009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Loubser S.I.</name></creator><creator><name>Sansom A.E.</name></creator><creator><name>Sanchez-Blazquez P.</name></creator><creator><name>Soechting I.K.,Bromage G.E.</name></creator><date role="Updated">2024-07-07T20:17:18Z</date><date role="Created">2009-05-16T23:49:51Z</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>radial-velocity</subject><subject>galaxy-kinematics</subject><description>This is the first of a series of papers devoted to the investigation of a large sample of brightest cluster galaxies (BCGs), their kinematic and stellar population properties, and the relationships between those and the properties of the cluster. We have obtained high signal-to-noise ratio, long-slit spectra of these galaxies with Gemini and William Herschel Telescope with the primary purpose of investigating their stellar population properties. This paper describes the selection methods and criteria used to compile a new sample of galaxies, concentrating on BCGs previously classified as containing a halo (cD galaxies), together with the observations and data reduction. 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