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<ri:Resource created="2009-02-14T06:42:47Z" 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>VRizK photometry of RDCSJ0910+54 cluster</title><shortName>J/A+A/489/571</shortName><identifier>ivo://CDS.VizieR/J/A+A/489/571</identifier><altIdentifier>doi:10.26093/cds/vizier.34890571</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tanaka M.</name></creator><creator><name>Finoguenov A.</name></creator><creator><name>Kodama T.</name></creator><creator><name>Morokuma T.</name></creator><creator><name>Rosati P.</name></creator><creator><name>Stanford S.A.,Eisenhardt P.</name></creator><creator><name>Holden B.</name></creator><creator><name>Mei S.</name></creator><date role="Updated">2009-02-14T05:48:12Z</date><date role="Created">2009-02-14T06:42:47Z</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><subject>galaxies</subject><subject>photometry</subject><description>We report on the environmental dependence of properties of galaxies around the RDCSJ0910+54 cluster at z=1.1. We obtained multi-band wide-field images of the cluster with Suprime-Cam and MOIRCS on Subaru and WFCAM on UKIRT. Also, an intensive spectroscopic campaign was carried out using LRIS on Keck and FOCAS on Subaru. 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