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<ri:Resource created="2012-04-11T13:19:43Z" 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>Extended radio emission in MOJAVE blazars</title><shortName>J/ApJ/710/764</shortName><identifier>ivo://CDS.VizieR/J/ApJ/710/764</identifier><altIdentifier>doi:10.26093/cds/vizier.17100764</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kharb P.</name></creator><creator><name>Lister M.L.</name></creator><creator><name>Cooper N.J.</name></creator><date role="Updated">2017-12-22T05:33:23Z</date><date role="Created">2012-04-11T13:19:43Z</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>galaxy-classification-systems</subject><subject>radio-continuum-emission</subject><subject>quasars</subject><subject>redshifted</subject><subject>bl-lacertae-objects</subject><description>We present the results of a study on the kiloparsec-scale radio emission in the complete flux density limited MOJAVE sample, comprising 135 radio-loud active galactic nuclei. New 1.4GHz Very Large Array (VLA) radio images of six quasars and previously unpublished images of 21 blazars are presented, along with an analysis of the high-resolution (VLA A-array) 1.4GHz emission for the entire sample. While extended emission is detected in the majority of the sources, about 7% of the sources exhibit only radio core emission. We expect more sensitive radio observations, however, to detect faint emission in these sources, as we have detected in the erstwhile "core-only" source, 1548+056. The kiloparsec-scale radio morphology varies widely across the sample. Many BL Lac objects exhibit extended radio power and kiloparsec-scale morphology typical of powerful FRII jets, while a substantial number of quasars possess radio powers intermediate between FRIs and FRIIs.</description><source format="bibcode">2010ApJ...710..764K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/710/764</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/VII/258">VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/706/1253">J/ApJ/706/1253 : MOJAVE VII. Blazar jet acceleration (Homan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/1874">J/AJ/138/1874 : MOJAVE. VI. Kinematic analysis of blazar jets (Lister+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3718">J/AJ/137/3718 : 15GHz monitoring of AGN jets with VLBA (Lister+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/171/376">J/ApJS/171/376 : MOJAVE. III. VLA 1.4GHz images (Cooper+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1262">J/AJ/131/1262 : Circular polarization images at 15GHz of AGN jets (Homan+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1389">J/AJ/130/1389 : Linear polarization of AGN jets at 15GHz (Lister+, 2005)</relatedResource><relatedResource>http://www.physics.purdue.edu/MOJAVE/ : MOJAVE program homepage</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/710/764</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/710/764</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/710/764</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/710/764</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/710/764</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/710/764</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/710/764/table1 (MOJAVE sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/710/764/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/710/764/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/710/764/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.5578869</ra><dec>-6.3931486</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/556 579 911 1263 1509 1546 1701 2143 2836 3024 3096 3675 3820 3886 4285 4695 4770 4820 5693 5767 5848 6252 6507 6641 6853 6984 7389 7896 7969 8031 8299 8487 8717 9442 9460 9632 9633 9676 9723 10163 10249 10422 10548 12047 12352 12580 12619 13230 13352 13496 13693 13927 14737 14744 15023 15067 15286 15494 15936 16027 16059 16093 16298 17184 17351 17579 17857 18035 18378 18506 18624 18661 18669 19088 19101 19190 19398 19567 19593 19831 20099 20935 21266 21358 21564 21768 21935 21960 21968 21972 22363 22375 22396 22658 22917 23099 23121 23127 23323 23416 23691 24084 24571 25016 25196 25255 25302 25630 26131 26292 26303 27060 27310 27417 27423 27765 28083 28479 29570 29675 29714 31430 31451 31559 31664 31894 32660 32764 36785 44805 44908 48595 48798 48846 48965</spatial><spectral>9.276497240453405e-25 9.276497240453405e-25</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/710/764?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/710/764/table1</name><description>MOJAVE sample</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Apparent V-band magnitude (2)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Type</name><description>Blazar classification (3)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Pol</name><description>[Y/N]? Highly optically polarized?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ipk</name><description>Peak intensity in radio map in Jy/beam</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_Ipk</name><description>[d] Flag on Ipk (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Irms</name><description>rms intensity in radio map in Jy/beam (4)</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Freq</name><description>Central observing frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>beta</name><description>? 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