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<ri:Resource created="2013-12-05T13:19:51Z" 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>AGNs detected by 60 month Swift/BAT survey</title><shortName>J/ApJ/749/21</shortName><identifier>ivo://CDS.VizieR/J/ApJ/749/21</identifier><altIdentifier>doi:10.26093/cds/vizier.17490021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ajello M.</name></creator><creator><name>Alexander D.M.</name></creator><creator><name>Greiner J.</name></creator><creator><name>Madejski G.M.</name></creator><creator><name>Gehrels N.</name></creator><creator><name>Burlon D.</name></creator><date role="Updated">2018-02-06T05:28:04Z</date><date role="Created">2013-12-05T13:19:51Z</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>x-ray-sources</subject><subject>surveys</subject><subject>redshifted</subject><description>Surveys above 10 keV represent one of the best resources to provide an unbiased census of the population of active galactic nuclei (AGNs). We present the results of 60 months of observation of the hard X-ray sky with Swift/Burst Alert Telescope (BAT). In this time frame, BAT-detected (in the 15-55keV band) 720 sources in an all-sky survey of which 428 are associated with AGNs, most of which are nearby. Our sample has negligible incompleteness and statistics a factor of ~2 larger over similarly complete sets of AGNs. Our sample contains (at least) 15 bona fide Compton-thick AGNs and 3 likely candidates. Compton-thick AGNs represent ~5% of AGN samples detected above 15keV. We use the BAT data set to refine the determination of the log N-log S of AGNs which is extremely important, now that NuSTAR prepares for launch, toward assessing the AGN contribution to the cosmic X-ray background. We show that the log N-log S of AGNs selected above 10 keV is now established to ~10% precision. We derive the luminosity function of Compton-thick AGNs and measure a space density of 7.9^+4.1^_-2.9_x10^-5^/Mpc3 for objects with a de-absorbed luminosity larger than 2x10^42^erg/s. As the BAT AGNs are all mostly local, they allow us to investigate the spatial distribution of AGNs in the nearby universe regardless of absorption. We find concentrations of AGNs that coincide spatially with the largest congregations of matter in the local (&lt;=85Mpc) universe. There is some evidence that the fraction of Seyfert 2 objects is larger than average in the direction of these dense regions.</description><source format="bibcode">2012ApJ...749...21A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/749/21</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/207/19">J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 2004-2010 (Baumgartner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/58">J/ApJ/728/58 : Swift-BAT survey of AGNs (Burlon+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/739/57">J/ApJ/739/57 : Ultra hard X-ray AGNs in the Swift/BAT survey (Koss+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/510/A48">J/A+A/510/A48 : Palermo Swift-BAT Hard X-ray Catalogue (Cusumano+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/524/A64">J/A+A/524/A64 : The 54-month Palermo BAT-survey catalogue (Cusumano+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/378">J/ApJS/186/378 : Hard X-ray survey from Swift-BAT 2004-2006 (Tueller+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/603">J/ApJ/699/603 : Evolution of Swift/BAT blazars (Ajello+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/681/113">J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/673/96">J/ApJ/673/96 : BAT X-ray Survey. III. (Ajello+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/678/102">J/ApJ/678/102 : BAT X-ray survey. I. 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