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II</title><shortName>J/AJ/131/114</shortName><identifier>ivo://CDS.VizieR/J/AJ/131/114</identifier><altIdentifier>doi:10.26093/cds/vizier.51310114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Burgess A.M.</name></creator><creator><name>Hunstead R.W.</name></creator><date role="Updated">2017-06-02T08:37:36Z</date><date role="Created">2013-11-06T09:57:28Z</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>active-galactic-nuclei</subject><subject>radio-continuum-emission</subject><subject>astronomical-object-identification</subject><description>Of the 228 sources in the Molonglo Southern 4Jy sample (MS4, Cat. J/AJ/131/100), the 133 with angular sizes &lt;35" have been imaged at 5GHz at 2"-4" resolution with the Australia Telescope Compact Array. 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