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<ri:Resource created="2010-09-13T13:51:25Z" 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>A 3.5mm polarimetric survey of radio-loud AGNs</title><shortName>J/ApJS/189/1</shortName><identifier>ivo://CDS.VizieR/J/ApJS/189/1</identifier><altIdentifier>doi:10.26093/cds/vizier.21890001</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Agudo I.</name></creator><creator><name>Thum C.</name></creator><creator><name>Wiesemeyer H.</name></creator><creator><name>Krichbaum T.P.</name></creator><date role="Updated">2017-06-27T06:38:22Z</date><date role="Created">2010-09-13T13:51:25Z</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>bl-lacertae-objects</subject><subject>active-galactic-nuclei</subject><subject>quasars</subject><subject>radio-sources</subject><subject>redshifted</subject><subject>apparent-magnitude</subject><description>We present the results from the first large (&gt;100 sources) 3.5mm polarimetric survey of radio-loud active galactic nuclei (AGNs). This wavelength is favorable within the radio-millimeter range for measuring the intrinsic linearly polarized emission from AGNs, since in general it is only marginally affected by Faraday rotation of the electric vector position angle and depolarization. The I, Q, U, and V Stokes parameter observations were performed with the XPOL polarimeter at the IRAM 30m Telescope on different observing epochs from 2005 July (when most of the measurements were made) to 2009 October. Our sample consists of 145 flat-radio-spectrum AGNs with declination &gt;-30{deg} (J2000.0) and flux density &gt;~1Jy at ~86GHz, as measured at the IRAM 30m Telescope from 1978 to 1994. This constraint on the radio spectrum causes our sample to be dominated by blazars, which allows us to conduct new statistical studies on this class of high-luminosity, relativistically beamed emitters. Over our entire source sample, the luminosity of the jets is anticorrelated with the degree of linear polarization. Consistent with previous findings claiming larger Doppler factors for brighter {gamma}-ray blazars, quasars listed in our sample, and in the Fermi Large Area Telescope Bright Source Catalog (LBAS, Abdo et al., 2009ApJ...700..597A), show larger luminosities than non-LBAS ones, but our data do not allow us to confirm the same for BL Lac objects. Our new data can be used to estimate the 3.5mm AGN contribution to measurements of the linear polarization of the cosmic microwave background, such as those performed by the Planck satellite.</description><source format="bibcode">2010ApJS..189....1A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/189/1</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/B/iram">B/iram : Plateau de Bure Interferometer Observation Log (IRAM 1991-2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/5">VIII/5 : Bright Extragalactic Radio Sources (1Jy) (Kuehr+, 1981)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/66">VIII/66 : IRAM observations in pre-star forming regions (Falgarone+ 1998-2001)</relatedResource><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/AJ/87/859">J/AJ/87/859 : Polarisation of 404 radio sources at 6 and 20cm (Perley, 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/99/297">J/ApJS/99/297 : First Caltech-Jodrell Bank VLBI Survey. III (Xu+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/131/95">J/ApJS/131/95 : VSOP 5 GHz continuum survey (Fomalont+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/609/539">J/ApJ/609/539 : Kinematics of parsec-scale radio jets (Kellermann+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1418">J/AJ/130/1418 : AGN jet kinematics (Jorstad+, 2005)</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 ivo-id="ivo://CDS.VizieR/J/ApJ/626/95">J/ApJ/626/95 : Gamma-ray blazar candidates (Sowards-Emmerd+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/46">J/ApJS/183/46 : Fermi/LAT bright gamma-ray source list (0FGL) (Abdo+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/476/L17">J/A+A/476/L17 : 86 and 43GHz observations of NRAO 150 (Agudo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/119">J/A+A/484/119 : Multi-epoch VLBI survey of CJF sources (Britzen+, 2008)</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/ApJS/189/1</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/189/1</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/189/1</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/189/1</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/189/1</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/189/1</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/ApJS/189/1/survey (Properties of the sources, and polarimetry results)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/189/1/survey?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/189/1/survey?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/189/1/survey?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.488063333</ra><dec>38.337463611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/180 556 579 911 1238 1263 1546 1701 1782 2414 2836 3024 3096 3675 3886 4572 4695 4770 4820 5154 5458 5693 5767 6164 6507 6641 6853 7346 7570 7653 7896 7969 8057 8299 8717 8858 9442 9460 9545 9612 9632 9633 9723 10163 10422 10432 11430 11640 11715 12301 12352 12580 13156 13230 13410 13496 13927 14338 14608 14641 14737 14744 14842 15023 15067 15286 15494 15681 16049 16059 16093 16281 16298 17184 17541 17579 17909 18002 18035 18214 18506 18661 18669 18907 19088 19101 19190 19398 20099 20468 21121 21196 21266 21358 21564 21768 21935 21968 21972 22363 22658 22917 23099 23121 23127 23323 23691 24084 24571 24845 25016 25196 25255 25302 25630 25864 26131 26292 27060 27765 28167 28479 29016 29072 29218 29570 29675 31430 31451 31559 31664 31894 35801 38763 40527 42901 44247 44805 44908 46964 47080 48023 48595 48798 48965</spatial><spectral>5.711671767393909e-23 5.711671767393909e-23</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/189/1?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/189/1/survey</name><description>Properties of the sources, and polarimetry results</description><column><name>Year</name><description>Year of observations</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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