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<ri:Resource created="2011-06-22T09:12:41Z" 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>zCOSMOS 10K sample group catalog to z=1</title><shortName>J/ApJ/697/1842</shortName><identifier>ivo://CDS.VizieR/J/ApJ/697/1842</identifier><altIdentifier>doi:10.26093/cds/vizier.16971842</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Knobel C.</name></creator><creator><name>Lilly S.J.</name></creator><creator><name>Iovino A.</name></creator><creator><name>Porciani C.</name></creator><creator><name>Kovac K.</name></creator><creator><name>Cucciati O.,Finoguenov A.</name></creator><creator><name>Kitzbichler M.G.</name></creator><creator><name>Carollo C.M.</name></creator><creator><name>Contini T.</name></creator><creator><name>Kneib J.-P.,Le Fevre O.</name></creator><creator><name>Mainieri V.</name></creator><creator><name>Renzini A.</name></creator><creator><name>Scodeggio M.</name></creator><creator><name>Zamorani G.,Bardelli S.</name></creator><creator><name>Bolzonella M.</name></creator><creator><name>Bongiorno A.</name></creator><creator><name>Caputi K.</name></creator><creator><name>Coppa G.,de la Torre S.</name></creator><creator><name>de Ravel L.</name></creator><creator><name>Franzetti P.</name></creator><creator><name>Garilli B.</name></creator><creator><name>Kampczyk P.,Lamareille F.</name></creator><creator><name>Le Borgne J.-F.</name></creator><creator><name>Le Brun V.</name></creator><creator><name>Maier C.</name></creator><creator><name>Mignoli M.</name></creator><creator><name>Pello R.,Peng Y.</name></creator><creator><name>Montero E.P.</name></creator><creator><name>Ricciardelli E.</name></creator><creator><name>Silverman J.D.</name></creator><creator><name>Tanaka M.,Tasca L.</name></creator><creator><name>Tresse L.</name></creator><creator><name>Vergani D.</name></creator><creator><name>Zucca E.</name></creator><creator><name>Abbas U.</name></creator><creator><name>Bottini D.</name></creator><creator><name>Cappi A.,Cassata P.</name></creator><creator><name>Cimatti A.</name></creator><creator><name>Fumana M.</name></creator><creator><name>Guzzo L.</name></creator><creator><name>Koekemoer A.M.</name></creator><creator><name>Leauthaud A.,Maccagni D.</name></creator><creator><name>Marinoni C.</name></creator><creator><name>McCracken H.J.</name></creator><creator><name>Memeo P.</name></creator><creator><name>Meneux B.</name></creator><creator><name>Oesch P.,Pozzetti L.</name></creator><creator><name>Scaramella R.</name></creator><date role="Updated">2017-11-29T11:49:02Z</date><date role="Created">2011-06-22T09:12:41Z</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>catalogs</subject><subject>redshifted</subject><description>We present a galaxy group catalog spanning the redshift range 0.1&lt;~z&lt;~1 in the ~1.7deg^2^ COSMOS field, based on the first ~10000 zCOSMOS spectra. The performance of both the Friends-of-Friends (FOF) and Voronoi-Delaunay method (VDM) approaches to group identification has been extensively explored and compared using realistic mock catalogs. We find that the performance improves substantially if groups are found by progressively optimizing the group-finding parameters for successively smaller groups, and that the highest fidelity catalog, in terms of completeness and purity, is obtained by combining the independently created FOF and VDM catalogs. The final completeness and purity of this catalog, both in terms of the groups and of individual members, compares favorably with recent results in the literature. The current group catalog contains 102 groups with N&gt;=5 spectroscopically confirmed members, with a further ~700 groups with 2&lt;=N&lt;=4. Most of the groups can be assigned a velocity dispersion and a dark-matter mass derived from the mock catalogs, with quantifiable uncertainties. The fraction of zCOSMOS galaxies in groups is about 25% at low redshift and decreases toward ~15% at z~0.8. The zCOSMOS group catalog is broadly consistent with that expected from the semianalytic evolution model underlying the mock catalogs.</description><source format="bibcode">2009ApJ...697.1842K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/697/1842</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/VII/256">VII/256 : Groups of Galaxies from CfA2 Redshift Survey (Mahtessian++, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/86">VII/86 : Groups of Galaxies. I. 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