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<ri:Resource created="2013-04-10T11:43:44Z" 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/{gamma}-ray correlation in AGN</title><shortName>J/ApJ/741/30</shortName><identifier>ivo://CDS.VizieR/J/ApJ/741/30</identifier><altIdentifier>doi:10.26093/cds/vizier.17410030</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ackermann M.</name></creator><creator><name>Ajello M.</name></creator><creator><name>Allafort A.</name></creator><creator><name>Angelakis E.</name></creator><creator><name>Axelsson M.,Baldini L.</name></creator><creator><name>Ballet J.</name></creator><creator><name>Barbiellini G.</name></creator><creator><name>Bastieri D.</name></creator><creator><name>Bellazzini R.,Berenji B.</name></creator><creator><name>Blandford R.D.</name></creator><creator><name>Bloom E.D.</name></creator><creator><name>Bonamente E.</name></creator><creator><name>Borgland A.W.,Bouvier A.</name></creator><creator><name>Bregeon J.</name></creator><creator><name>Brez A.</name></creator><creator><name>Brigida M.</name></creator><creator><name>Bruel P.</name></creator><creator><name>Buehler R.,Buson S.</name></creator><creator><name>Caliandro G.A.</name></creator><creator><name>Cameron R.A.</name></creator><creator><name>Cannon A.</name></creator><creator><name>Caraveo P.A.,Casandjian J.M.</name></creator><creator><name>Cavazzuti E.</name></creator><creator><name>Cecchi C.</name></creator><creator><name>Charles E.</name></creator><creator><name>Chekhtman A.,Cheung C.C.</name></creator><creator><name>Ciprini S.</name></creator><creator><name>Claus R.</name></creator><creator><name>Cohen-Tanugi J.</name></creator><creator><name>Cutini S.</name></creator><creator><name>de Palma F.,Dermer C.D.</name></creator><creator><name>do Couto e Silva E.</name></creator><creator><name>Drell P.S.</name></creator><creator><name>Dubois R.</name></creator><creator><name>Dumora D.,Escande L.</name></creator><creator><name>Favuzzi C.</name></creator><creator><name>Fegan S.J.</name></creator><creator><name>Focke W.B.</name></creator><creator><name>Fortin P.</name></creator><creator><name>Frailis M.,Fuhrmann L.</name></creator><creator><name>Fukazawa Y.</name></creator><creator><name>Fusco P.</name></creator><creator><name>Gargano F.</name></creator><creator><name>Gasparrini D.</name></creator><creator><name>Gehrels N.,Giglietto N.</name></creator><creator><name>Giommi P.</name></creator><creator><name>Giordano F.</name></creator><creator><name>Giroletti M.</name></creator><creator><name>Glanzman T.,Godfrey G.</name></creator><creator><name>Grandi P.</name></creator><creator><name>Grenier I.A.</name></creator><creator><name>Guiriec S.</name></creator><creator><name>Hadasch D.</name></creator><creator><name>Hayashida M.,Hays E.</name></creator><creator><name>Healey S.E.</name></creator><creator><name>Johannesson G.</name></creator><creator><name>Johnson A.S.</name></creator><creator><name>Kamae T.</name></creator><creator><name>Katagiri H.,Kataoka J.</name></creator><creator><name>Knodlseder J.</name></creator><creator><name>Kuss M.</name></creator><creator><name>Lande J.</name></creator><creator><name>Lee S.-H.</name></creator><creator><name>Longo F.,Loparco F.</name></creator><creator><name>Lott B.</name></creator><creator><name>Lovellette M.N.</name></creator><creator><name>Lubrano P.</name></creator><creator><name>Makeev A.,Max-Moerbeck W.</name></creator><creator><name>Mazziotta M.N.</name></creator><creator><name>McEnery J.E.</name></creator><creator><name>Mehault J.</name></creator><creator><name>Michelson P.F.,Mizuno T.</name></creator><creator><name>Monte C.</name></creator><creator><name>Monzani M.E.</name></creator><creator><name>Morselli A.</name></creator><creator><name>Moskalenko I.V.</name></creator><creator><name>Murgia S.,Naumann-Godo M.</name></creator><creator><name>Nishino S.</name></creator><creator><name>Nolan P.L.</name></creator><creator><name>Norris J.P.</name></creator><creator><name>Nuss E.</name></creator><creator><name>Ohsugi T.,Okumura A.</name></creator><creator><name>Omodei N.</name></creator><creator><name>Orlando E.</name></creator><creator><name>Ormes J.F.</name></creator><creator><name>Ozaki M.</name></creator><creator><name>Paneque D.,Pavlidou V.</name></creator><creator><name>Pelassa V.</name></creator><creator><name>Pepe M.</name></creator><creator><name>Pesce-Rollins M.</name></creator><creator><name>Pierbattista M.,Piron F.</name></creator><creator><name>Porter T.A.</name></creator><creator><name>Raino S.</name></creator><creator><name>Razzano M.</name></creator><creator><name>Readhead A.</name></creator><creator><name>Reimer A.,Reimer O.</name></creator><creator><name>Richards J.L.</name></creator><creator><name>Romani R.W.</name></creator><creator><name>Sadrozinski H.F.-W.</name></creator><creator><name>Scargle J.D.,Sgro C.</name></creator><creator><name>Siskind E.J.</name></creator><creator><name>Smith P.D.</name></creator><creator><name>Spandre G.</name></creator><creator><name>Spinelli P.</name></creator><creator><name>Strickman M.S.,Suson D.J.</name></creator><creator><name>Takahashi H.</name></creator><creator><name>Tanaka T.</name></creator><creator><name>Taylor G.B.</name></creator><creator><name>Thayer J.G.</name></creator><creator><name>Thayer J.B.,Thompson D.J.</name></creator><creator><name>Torres D.F.</name></creator><creator><name>Tosti G.</name></creator><creator><name>Tramacere A.</name></creator><creator><name>Troja E.,Vandenbroucke J.</name></creator><creator><name>Vianello G.</name></creator><creator><name>Vitale V.</name></creator><creator><name>Waite A.P.</name></creator><creator><name>Wang P.</name></creator><creator><name>Winer B.L.,Wood K.S.</name></creator><creator><name>Yang Z.</name></creator><creator><name>Ziegler M.</name></creator><date role="Updated">2017-11-06T12:23:14Z</date><date role="Created">2013-04-10T11:43:44Z</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-continuum-emission</subject><subject>gamma-ray-astronomy</subject><subject>redshifted</subject><subject>bl-lacertae-objects</subject><subject>astronomical-object-identification</subject><description>We present a detailed statistical analysis of the correlation between radio and gamma-ray emission of the active galactic nuclei (AGNs) detected by Fermi during its first year of operation, with the largest data sets ever used for this purpose. We use both archival interferometric 8.4GHz data (from the Very Large Array and ATCA, for the full sample of 599 sources) and concurrent single-dish 15GHz measurements from the Owens Valley Radio Observatory (OVRO, for a sub sample of 199 objects). Our unprecedentedly large sample permits us to assess with high accuracy the statistical significance of the correlation, using a surrogate data method designed to simultaneously account for common-distance bias and the effect of a limited dynamical range in the observed quantities.</description><source format="bibcode">2011ApJ...741...30A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/741/30</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/72">VIII/72 : CLASS survey of radio sources (Myers+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/31">J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/535/A69">J/A+A/535/A69 : AGN Fermi/LAT {gamma}-ray and 37GHz fluxes (Nieppola+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/726/16">J/ApJ/726/16 : {gamma}-ray loud blazars (Linford+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/29">J/ApJS/194/29 : Observations of blazars at 15GHz (Richards+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/L7">J/ApJ/722/L7 : Fermi/LAT detected MOJAVE AGNs (Pushkarev+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/520">J/ApJ/722/520 : Gamma-ray light curves of Fermi blazars (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/718/587">J/ApJ/718/587 : The Fermi-AT20G catalog (Mahony+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/715/429">J/ApJ/715/429 : First Fermi-LAT AGN catalog (1LAC) (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1407">J/ApJ/709/1407 : SED of the Fermi blazars (Li+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/97">J/ApJS/175/97 : CGRaBS: survey of {gamma}-ray blazar (Healey+, 2008)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/351">J/PASJ/55/351 : ATCA observations of 202 compact radio sources (Tingay+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/122/235">J/A+AS/122/235 : ROSAT active galaxies IDs (Laurent-Muehleisen+ 1997)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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