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<ri:Resource created="2013-02-01T15:28:07Z" 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 variability of compact, flat-spectrum AGNs</title><shortName>J/AJ/142/108</shortName><identifier>ivo://CDS.VizieR/J/AJ/142/108</identifier><altIdentifier>doi:10.26093/cds/vizier.51420108</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koay J.Y.</name></creator><creator><name>Macquart J.-P.</name></creator><creator><name>Rickett B.J.</name></creator><creator><name>Bignall H.E.</name></creator><creator><name>Lovell J.E.J.,Reynolds C.</name></creator><creator><name>Jauncey D.L.</name></creator><creator><name>Pursimo T.</name></creator><creator><name>Kedziora-Chudczer L.</name></creator><creator><name>Ojha R.</name></creator><date role="Updated">2017-12-06T07:38:54Z</date><date role="Created">2013-02-01T15:28:07Z</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-sources</subject><description>The 4.9GHz Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey detected a drop in interstellar scintillation (ISS) for sources at redshifts z&gt;~2, indicating an apparent increase in angular diameter or a decrease in flux density of the most compact components of these sources relative to their extended emission. This can result from intrinsic source size effects or scatter broadening in the intergalactic medium (IGM) in excess of the expected (1+z)^1/2^ angular diameter scaling of brightness temperature limited sources resulting from cosmological expansion. We report here 4.9GHz and 8.4GHz observations and data analysis for a sample of 140 compact, flat-spectrum sources which may allow us to determine the origin of this angular diameter-redshift relation by exploiting their different wavelength dependences. In addition to using ISS as a cosmological probe, the observations provide additional insight into source morphologies and the characteristics of ISS.</description><source format="bibcode">2011AJ....142..108K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/108</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/ApJ/689/108">J/ApJ/689/108 : MASIV survey. II. 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