<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2005-08-17T21:51:56Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>8.4GHz obs. of scintillating sources</title><shortName>J/ApJ/614/607</shortName><identifier>ivo://CDS.VizieR/J/ApJ/614/607</identifier><altIdentifier>doi:10.26093/cds/vizier.16140607</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ojha R.</name></creator><creator><name>Fey A.L.</name></creator><creator><name>Jauncey D.L.</name></creator><creator><name>Lovell J.E.J.</name></creator><creator><name>Johnston K.J.</name></creator><date role="Updated">2005-08-17T21:52:02Z</date><date role="Created">2005-08-17T21:51:56Z</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-sources</subject><description>We compare the milliarcsecond-scale morphology of scintillating and nonscintillating sources. The scintillating sources are drawn from those flat-spectrum extragalactic radio sources discovered, by the Micro-Arcsecond Scintillation-Induced Variability Survey (MASIV, Lovell et al, 2003AJ....126.1699L), to have flux density variability at 5GHz on timescales from hours to days. Intrinsic source structure information is obtained from previously published and/or publicly available 8.4GHz Very Long Baseline Array images. A sample of low flux density (S_{nu}=5GHz_&lt;0.3Jy) scintillating sources was compared with a sample of high flux density (S_{nu}=5GHz_~1Jy) scintillators, as well as a sample of high flux density nonscintillators.</description><source format="bibcode">2004ApJ...614..607O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/614/607</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1570">J/AJ/128/1570 : 8.4GHz VLBA observations of scintillating sources (Ojha+ 2004)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/614/607</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/614/607</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/614/607</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/614/607</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/614/607</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/614/607</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/614/607/table1</name><description>High flux density scintillators</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Source name, based on B1950 position</description><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>S8.4GHz</name><description>Flux density at 8.4GHz</description><unit>Jy</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Epoch</name><description>Epoch of observation (most recent available)</description><flag>nullable</flag></column></table><table><name>J/ApJ/614/607/table2</name><description>High flux density nonscintillators</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Source name, based on B1950 position</description><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>S8.4GHz</name><description>Flux density at 8.4GHz</description><unit>Jy</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Epoch</name><description>Epoch of observation (most recent available)</description><flag>nullable</flag></column></table></schema></tableset></ri:Resource>