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<ri:Resource created="2014-03-31T10:17:05Z" 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>IR properties of Swift/BAT X-ray AGNs</title><shortName>J/ApJ/754/45</shortName><identifier>ivo://CDS.VizieR/J/ApJ/754/45</identifier><altIdentifier>doi:10.26093/cds/vizier.17540045</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ichikawa K.</name></creator><creator><name>Ueda Y.</name></creator><creator><name>Terashima Y.</name></creator><creator><name>Oyabu S.</name></creator><creator><name>Gandhi P.</name></creator><creator><name>Matsuta K.,Nakagawa T.</name></creator><date role="Updated">2017-09-29T09:02:31Z</date><date role="Created">2014-03-31T10:17:05Z</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>infrared-sources</subject><subject>surveys</subject><description>We investigate the mid- (MIR) to far-infrared (FIR) properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert Telescope (BAT) all-sky hard X-ray (14-195 keV) survey, based on the cross correlation with the AKARI infrared survey catalogs complemented by those with Infrared Astronomical Satellite and Wide-field Infrared Survey Explorer. Out of 135 non-blazer AGNs in the Swift/BAT nine-month catalog, we obtain the MIR photometric data for 128 sources either in the 9, 12, 18, 22, and/or 25 {mu}m band. We find good correlation between their hard X-ray and MIR luminosities over three orders of magnitude (42 &lt; log {lambda}L_{lambda}_(9, 18 {mu}m) &lt; 45), which is tighter than that with the FIR luminosities at 90 {mu}m. This suggests that thermal emission from hot dusts irradiated by the AGN emission dominate the MIR fluxes. Both X-ray unabsorbed and absorbed AGNs follow the same correlation, implying isotropic infrared emission, as expected in clumpy dust tori rather than homogeneous ones. We find excess signals around 9 {mu}m in the averaged infrared spectral energy distribution from heavy obscured "new type" AGNs with small scattering fractions in the X-ray spectra. This could be attributed to the polycyclic aromatic hydrocarbon emission feature, suggesting that their host galaxies have strong starburst activities.</description><source format="bibcode">2012ApJ...754...45I</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/754/45</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/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/298">II/298 : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/297">II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/156">II/156 : IRAS Faint Source Catalog, |b| &gt; 10, Version 2.0 (Moshir+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A67">J/A+A/561/A67 : 54-month Palermo BAT cat. sources classification (Parisi, 2014)</relatedResource><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/753/104">J/ApJ/753/104 : AGN identifications from AKARI and Swift (Matsuta+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/21">J/ApJ/749/21 : AGNs detected by 60 month Swift/BAT survey (Ajello+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/541/A160">J/A+A/541/A160 : Planck + X/{gamma} observations of blazars (Giommi+, 2012)</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/ApJ/681/113">J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/678/102">J/ApJ/678/102 : BAT X-ray survey. 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