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<ri:Resource created="2005-02-23T12:40:14Z" 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>HST observations of Extremely Red Objects</title><shortName>J/MNRAS/330/1</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/330/1</identifier><altIdentifier>doi:10.26093/cds/vizier.73300001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smith G.P.</name></creator><creator><name>Smail I.</name></creator><creator><name>Kneib J.-P.</name></creator><creator><name>Czoske O.</name></creator><creator><name>Ebeling H.</name></creator><creator><name>Edge A.C.,Pello R.</name></creator><creator><name>Ivison R.J.</name></creator><creator><name>Packham C.</name></creator><creator><name>Le Borgne J.-F.</name></creator><date role="Updated">2024-06-27T20:18:01Z</date><date role="Created">2005-02-23T12:40:14Z</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>gravitational-lensing</subject><subject>galaxies</subject><subject>photometry</subject><subject>infrared-photometry</subject><description>We present the results of a survey for extremely red objects (EROs) undertaken in the fields of 10 massive galaxy cluster lenses at z~0.2, combining sensitive, high-resolution Hubble Space Telescope imaging with deep, half-arcsecond K-band imaging from UKIRT. 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