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<ri:Resource created="2010-04-29T12:06:33Z" 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>EGRET blazars in VIPS</title><shortName>J/ApJ/671/1355</shortName><identifier>ivo://CDS.VizieR/J/ApJ/671/1355</identifier><altIdentifier>doi:10.26093/cds/vizier.16711355</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Taylor G.B.</name></creator><creator><name>Healey S.E.</name></creator><creator><name>Helmboldt J.F.</name></creator><creator><name>Tremblay S.</name></creator><creator><name>Fassnacht C.D.,Walker R.C.</name></creator><creator><name>Sjouwerman L.O.</name></creator><creator><name>Pearson T.J.</name></creator><creator><name>Readhead A.C.S.</name></creator><creator><name>Weintraub L.,Gehrels N.</name></creator><creator><name>Romani R.W.</name></creator><creator><name>Michelson P.F.</name></creator><creator><name>Blandford R.D.</name></creator><creator><name>Cotter G.</name></creator><date role="Updated">2017-06-30T05:49:17Z</date><date role="Created">2010-04-29T12:06:33Z</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><subject>quasars</subject><subject>bl-lacertae-objects</subject><subject>redshifted</subject><description>We examine the radio properties of EGRET-detected blazars observed as part of the VLBA Imaging and Polarimetry Survey (VIPS). VIPS has a flux limit roughly an order of magnitude below the MOJAVE survey and most other samples that have been used to study the properties of EGRET blazars. At lower flux levels, radio flux density does not directly correlate with gamma-ray flux density. We do find that the EGRET-detected blazars tend to have higher brightness temperatures, greater core fractions, and possibly larger than average jet opening angles. A weak correlation is also found with jet length and with polarization. All of the well-established trends can be explained by systematically larger Doppler factors in the gamma-ray-loud blazars, consistent with the measurements of higher apparent velocities found in monitoring programs carried out at radio frequencies above 10 GHz.</description><source format="bibcode">2007ApJ...671.1355T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/671/1355</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/123/79">J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/97">J/ApJS/175/97 : CGRaBS: survey of {gamma}-ray blazar candidates (Healey+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/326/1455">J/MNRAS/326/1455 : The CLASS blazar survey. I. (Marcha+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/329/877">J/MNRAS/329/877 : The CLASS blazar survey. II. (Caccianiga+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/348/937">J/MNRAS/348/937 : The CLASS blazar survey. III. (Caccianiga+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/590/109">J/ApJ/590/109 : Gamma-ray blazar in northern sky (Sowards-Emmerd+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/171/61">J/ApJS/171/61 : All-Sky Survey of Flat-Spectrum Radio Sources (Healey+ 2007)</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/671/1355</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/671/1355</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/671/1355</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/671/1355</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/671/1355</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/671/1355</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/671/1355/table1 (EGRET Identifications)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/671/1355/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/671/1355/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/671/1355/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>115.83</ra><dec>54.8</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/671/1355/VIPS (VIPS source properties and brightness)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/671/1355/VIPS?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/671/1355/VIPS?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/671/1355/VIPS?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>121.754222222</ra><dec>51.294075</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4695 4822 5423 5816 5817 6069 6088 6646 6647 7004 7255 7426 8514 9442 9460 9723 10064 10189 10201 10213 10224 10250 10337 10340 10524 10527 10548 10551 10910 10932 26614 26620 28083 28479 28492 28493</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/671/1355?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/671/1355/table1</name><description>EGRET Identifications</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Maximum separation among the dominant Gaussian components</description><unit>mas</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PAjet</name><description>? 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