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<ri:Resource created="2011-09-08T13:56:03Z" 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>RX J105453.3+552102 cluster SDSS photometry</title><shortName>J/A+A/527/A143</shortName><identifier>ivo://CDS.VizieR/J/A+A/527/A143</identifier><altIdentifier>doi:10.26093/cds/vizier.35270143</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aguerri J.A.L.</name></creator><creator><name>Girardi M.</name></creator><creator><name>Boschin W.</name></creator><creator><name>Barrena R.</name></creator><creator><name>Mendez-Abreu J.,Sanchez-Janssen R.</name></creator><creator><name>Borgani S.</name></creator><creator><name>Castro-Rodriguez N.</name></creator><creator><name>Corsini E.M.,Del Burgo C.</name></creator><creator><name>D'Onghia E.</name></creator><creator><name>Iglesias-Paramo J.</name></creator><creator><name>Napolitano N.</name></creator><creator><name>Vilchez J.M.</name></creator><date role="Updated">2011-09-18T11:00:51Z</date><date role="Created">2011-09-08T13:56:03Z</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>photometry</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><description>The most accepted scenario for the origin of fossil groups is that they are galaxy associations in which the merging rate was fast and efficient. These systems have assembled half of their mass at early epoch of the Universe, subsequently growing by minor mergers, and therefore could contain a fossil record of the galaxy structure formation. We have started an observational project in order to characterize a large sample of fossil groups. 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