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<ri:Resource created="2005-07-12T22:33:28Z" 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>The VLA-COSMOS survey</title><shortName>J/AJ/128/1974</shortName><identifier>ivo://CDS.VizieR/J/AJ/128/1974</identifier><altIdentifier>doi:10.26093/cds/vizier.51281974</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schinnerer E.</name></creator><creator><name>Carilli C.L.</name></creator><creator><name>Scoville N.Z.</name></creator><creator><name>Bondi M.</name></creator><creator><name>Ciliegi P.,Vettolani P.</name></creator><creator><name>Le Fevre O.</name></creator><creator><name>Koekemoer A.M.</name></creator><creator><name>Bertoldi F.</name></creator><creator><name>Impey C.D.</name></creator><date role="Updated">2005-07-12T22:33:41Z</date><date role="Created">2005-07-12T22:33:28Z</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>radio-continuum-emission</subject><subject>radio-galaxies</subject><description>We present a catalog of 246 radio sources found in the central 1{deg} of the COSMOS field at 1.4GHz. The VLA pilot project data have a resolution of 1.9"x1.6" and an rms noise limit of ~25-100{mu}Jy/beam covering 0.837{deg}^2. About 20 radio sources are clearly extended, and most of them appear to be double-lobed radio galaxies. 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