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<ri:Resource created="2004-04-19T22:59:50Z" 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>Radio and Infrared observations of EROs</title><shortName>J/ApJ/581/844</shortName><identifier>ivo://CDS.VizieR/J/ApJ/581/844</identifier><altIdentifier>doi:10.26093/cds/vizier.15810844</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Smail I.</name></creator><creator><name>Owen F.N.</name></creator><creator><name>Morrison G.E.</name></creator><creator><name>Keel W.C.</name></creator><creator><name>Ivison R.J.</name></creator><creator><name>Ledlow M.J.</name></creator><date role="Updated">2004-04-19T23:01:08Z</date><date role="Created">2004-04-19T22:59:50Z</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>infrared-sources</subject><subject>infrared-photometry</subject><subject>radio-sources</subject><description>We present the results from a sensitive multiwavelength analysis of the properties of extremely red objects (EROs). Our analysis employs deep RIzJHK photometry of an 8.5'x8.5' region to select a sample of 68 EROs with (R-K)&gt;=5.3 and brighter than K=20.5 (5{sigma}). We combine this photometric data set with an extremely deep 1.4GHz radio map of the field obtained from the VLA. 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