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<ri:Resource created="2012-05-24T12:00:48Z" 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>2dFGRS Percolation-Inferred Galaxy Group (2PIGG)</title><shortName>J/MNRAS/348/866</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/348/866</identifier><altIdentifier>doi:10.26093/cds/vizier.73480866</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Eke V.R.</name></creator><creator><name>Baugh C.M.</name></creator><creator><name>Cole S.</name></creator><creator><name>Frenk C.S.</name></creator><creator><name>Norberg P.</name></creator><creator><name>Peacock J.A.,Baldry I.K.</name></creator><creator><name>Bland-Hawthorn J.</name></creator><creator><name>Bridges T.</name></creator><creator><name>Cannon R.</name></creator><creator><name>Colless M.,Collins C.</name></creator><creator><name>Couch W.</name></creator><creator><name>Dalton G.</name></creator><creator><name>De Propris R.</name></creator><creator><name>Driver S.P.</name></creator><creator><name>Efstathiou G.,Ellis R.S.</name></creator><creator><name>Glazebrook K.</name></creator><creator><name>Jackson C.</name></creator><creator><name>Lahav O.</name></creator><creator><name>Lewis I.</name></creator><creator><name>Lumsden S.,Maddox S.</name></creator><creator><name>Madgwick D.</name></creator><creator><name>Peterson B.A.</name></creator><creator><name>Sutherland W.</name></creator><creator><name>Taylor K.</name></creator><date role="Updated">2024-06-29T20:14:47Z</date><date role="Created">2012-05-24T12:00:48Z</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>redshifted</subject><description>The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percolation algorithm which has been thoroughly tested on mock versions of the 2dFGRS generated from cosmological N-body simulations. The tests suggest that the algorithm groups all galaxies that it should be grouping, with an additional 40 per cent of interlopers. About 55 per cent of the ~190000 galaxies considered are placed into groups containing at least two members of which ~29000 are found. Of these, ~7000 contain at least four galaxies, and these groups have a median redshift of 0.11 and a median velocity dispersion of 260km/s. 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