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<ri:Resource created="2014-06-20T11:57:15Z" 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>Long-term variability of AGN at hard X-rays</title><shortName>J/A+A/563/A57</shortName><identifier>ivo://CDS.VizieR/J/A+A/563/A57</identifier><altIdentifier>doi:10.26093/cds/vizier.35630057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Soldi S.</name></creator><creator><name>Beckmann V.</name></creator><creator><name>Baumgartner W.H.</name></creator><creator><name>Ponti G.</name></creator><creator><name>Shrader C.R.,Lubinski P.</name></creator><creator><name>Krimm H.A.</name></creator><creator><name>Mattana F.</name></creator><creator><name>Tueller J.</name></creator><date role="Updated">2017-10-09T13:33:46Z</date><date role="Created">2014-06-20T11:57:15Z</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>seyfert-galaxies</subject><subject>x-ray-sources</subject><description>Variability at all observed wavelengths is a distinctive property of active galactic nuclei (AGN). Hard X-rays provide us with a view of the innermost regions of AGN, mostly unbiased by absorption along the line of sight. Characterizing the intrinsic hard X-ray variability of a large AGN sample and comparing it to the results obtained at lower X-ray energies can significantly contribute to our understanding of the mechanisms underlying the high-energy radiation. Swift/BAT provides us with the unique opportunity to follow, on time scales of days to years and with regular sampling, the 14-195keV emission of the largest AGN sample available up to date for this kind of investigation. As a continuation of an early work using the first 9 months of BAT data, we study the amplitude of the variations and their dependence on subclass and on energy, for a sample of 110 radio quiet and radio loud AGN selected from the BAT 58-month survey.</description><source format="bibcode">2014A&amp;A...563A..57S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/563/A57</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/A+A/473/105">J/A+A/473/105 : Lockman Hole AGN variability with XMM (Mateos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/475">J/A+A/487/475 : X-ray variability of AGNs in Lockman Hole (Papadakis+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/73">J/A+A/488/73 : Variability-selected AGN in Chandra DFS (Trevese+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/497/81">J/A+A/497/81 : Variability-selected AGN in CDFS (Boutsia+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A84">J/A+A/536/A84 : X-ray variability of AGN (Vagnetti+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/108">J/AJ/142/108 : Radio variability of compact, flat-spectrum AGNs (Koay+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/737">J/ApJ/723/737 : Catalog of variability selected AGNs in GOODS (Villforth+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/97">J/ApJ/731/97 : Variable AGNs in GOODS fields (Sarajedini+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/124">J/ApJ/748/124 : AGN X-ray variability in the 4Ms catalog (Young+, 2012)</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/563/A57</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/563/A57</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/563/A57</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/563/A57</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/563/A57</mirrorURL><mirrorURL title="VizieR at SAAO: 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Type</name><description>Source classification (4)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>CRate</name><description>14-195keV average count rate (1)</description><unit>0.0001count.s**-1</unit><ucd>phot.count;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sv</name><description>[5/99] Variability estimator of 14-195keV flux</description><unit>%</unit><ucd>stat.fit.goodness;src.var</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_Sv</name><description>[1/19] Upper error on 14-195keV variability</description><unit>%</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Sv</name><description>[1/19] Lower error on 14-195keV variability</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Sv1</name><description>[3/104]? variability estimator 14-24keV flux</description><unit>%</unit><ucd>stat.fit.goodness;src.var</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E_Sv1</name><description>[2/27]? Upper error on 14-24keV variability</description><unit>%</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Sv1</name><description>[2/36]? Lower error on 14-24keV variability</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Sv2</name><description>[1/127]? variability estimator 35-100keV flux</description><unit>%</unit><ucd>stat.fit.goodness;src.var</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E_Sv2</name><description>[1/47]? Upper error on 35-100keV variability</description><unit>%</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Sv2</name><description>[1/52]? 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