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<ri:Resource created="2005-08-18T14:34:51Z" 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>VSOP 5GHz AGN Survey. IV</title><shortName>J/ApJ/616/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/616/110</identifier><altIdentifier>doi:10.26093/cds/vizier.16160110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Horiuchi S.</name></creator><creator><name>Fomalont E.B.</name></creator><creator><name>Scott W.K.</name></creator><creator><name>Taylor A.R.</name></creator><creator><name>Lovell J.E.J.,Moellenbrock G.A.</name></creator><creator><name>Dodson R.</name></creator><creator><name>Murata Y.</name></creator><creator><name>Hirabayashi H.</name></creator><creator><name>Edwards P.G.,Gurvits L.I.</name></creator><creator><name>Shen Z.-Q.</name></creator><date role="Updated">2005-08-18T14:35:08Z</date><date role="Created">2005-08-18T14:34:51Z</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>active-galactic-nuclei</subject><subject>radio-continuum-emission</subject><subject>surveys</subject><description>The VLBI Space Observatory Programme (VSOP) mission is a Japanese-led project to study radio sources with submilliarcsecond angular resolution, using an orbiting 8m telescope on board the satellite HALCA with a global Earth-based array of telescopes. A major program is the 5GHz VSOP Survey Program, which we supplement here with Very Long Baseline Array observations to produce a complete and flux density-limited sample. Using statistical methods of analysis of the observed visibility amplitude versus projected (u, v) spacing, we have determined the angular size and brightness temperature distribution of bright radio emission from active galactic nuclei.</description><source format="bibcode">2004ApJ...616..110H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/616/110</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/131/95">J/ApJS/131/95 : VSOP 5 GHz continuum survey (Fomalont+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/52/997">J/PASJ/52/997 : VSOP 5 GHz AGN Survey (Hirabayashi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/155/33">J/ApJS/155/33 : VSOP 5 GHz AGN Survey. 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