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<ri:Resource created="2012-03-16T15:27:50Z" 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>AGN Fermi/LAT {gamma}-ray and 37GHz fluxes</title><shortName>J/A+A/535/A69</shortName><identifier>ivo://CDS.VizieR/J/A+A/535/A69</identifier><altIdentifier>doi:10.26093/cds/vizier.35350069</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nieppola E.</name></creator><creator><name>Tornikoski M.</name></creator><creator><name>Valtaoja E.</name></creator><creator><name>Leon-Tavares J.</name></creator><creator><name>Hovatta T.,Laehteenmaeki A.</name></creator><creator><name>Tammi J.</name></creator><date role="Updated">2018-01-04T08:22:13Z</date><date role="Created">2012-03-16T15:27:50Z</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>quasars</subject><subject>radio-sources</subject><subject>gamma-ray-astronomy</subject><description>Although the Fermi mission has increased our knowledge of {gamma}-ray AGN, many questions remain, such as the site of {gamma}-ray production, the emission mechanism, and the factors that govern the strength of the emission. Using data from a high radio band, 37GHz, uncontaminated by other radiation components besides the jet emission, we study these questions with averaged flux densities over the the first year of Fermi operations. We look for possible correlations between the 100MeV-100GeV band used by the Fermi satellite and 37GHz radio band observed at the Aalto University Metsahovi Radio Telescope, as well as for differences between the {gamma}-ray emission of different AGN subsamples. We use data averaged over the 1FGL period. Our sample includes 249 northern AGN, including a complete sample of 68 northern AGN with a measured average flux density exceeding 1Jy.</description><source format="bibcode">2011A&amp;A...535A..69N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A69</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/J/ApJS/188/405">J/ApJS/188/405 : Fermi-LAT first source catalog (1FGL) (Abdo+, 2010)</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/A+A/535/A69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A69</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/535/A69</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/535/A69</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/535/A69</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/A+A/535/A69/table1 (The sample sources used in this study and their classifications)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/535/A69/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/535/A69/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/535/A69/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>4.37</ra><dec>-5.18</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/100 250 398 447 514 556 579 911 1085 1263 1701 2091 2122 2228 2295 2331 2340 2414 2836 3023-3024 3085 3431 3876 3882 3886 4255 4572 4695 4770 4820 4964 5072 5139 5311 5361 5423 5483 5817 5915 6015 6018 6021 6067 6088 6167 6348 6368 6507 6647 6777 6815 6963 6996 7001 7037-7038 7045 7346 7354 7426 7446 7515 7548 7570 7640 7896 7969 8067 8071 8205 8299 8374 8466 8515 8613 8915 8945 8972 9049 9075 9196 9442 9460 9566 9570 9612 9632 9711 9723 10071 10195 10249 10280 10422 10512 10572 10599 10656 10669 10800 10921 11081 11153 11212 11321 11374 11444 11449 11522 11631 11639 11649 11683 12173 12218 12231 12323 12444 12466 12599 12604 12619 13352 13367 13485 13586 13613 13666 13673 13705 13820 13927 15059 15067 15147 15211 15247 15286 15969 16027 16058 16170 16281 16298 17364 17516 17579 17857 17917 17927 18035 18119 18259 18270 18315 18624 18661 18718 19088 19190 19370 19398 19523 19622 19756 19789 19831 19890 19907 19918 20083 20099 20141 20325 21358 21437 21758 21768 21935 21960 21968 21972 22305 22363 22396 22917 22950 23011 23015 23099 23121 23127 23134 23222 23306 23383 23416 23897 24027 24084 24123 25630 25677 25818 25864 26131 26292 26303 26340 26550 26898 27060 27217 27243 27433 27524 27765 28083 28342 28352 28454 28479 28492 28498 28517 28542 28546 29570 29675 30012 30193 30570 31190 31430 31451 31663 31665 31894 32261 32311 32345 32621 40762 44908 45011 48985 49071</spatial><spectral>2.4516457410139638e-23 2.4516457410139638e-23</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/535/A69?format=ascii</footprint><waveband>Gamma-ray</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/535/A69/table1</name><description>The sample sources used in this study and their classifications</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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