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<ri:Resource created="2024-04-05T10:00:57Z" 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>Seyfert 1 AGNs with X-ray sp. from NuSTAR+Swift</title><shortName>J/ApJ/927/42</shortName><identifier>ivo://CDS.VizieR/J/ApJ/927/42</identifier><altIdentifier>doi:10.26093/cds/vizier.19270042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kamraj N.</name></creator><creator><name>Brightman M.</name></creator><creator><name>Harrison F.A.</name></creator><creator><name>Stern D.</name></creator><creator><name>Garcia J.A.,Balokovic M.</name></creator><creator><name>Ricci C.</name></creator><creator><name>Koss M.J.</name></creator><creator><name>Mejia-Restrepo J.E.</name></creator><creator><name>Oh K.,Powell M.C.</name></creator><creator><name>Urry C.M.</name></creator><date role="Updated">2024-11-06T20:24:02Z</date><date role="Created">2024-04-05T10:00:57Z</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>seyfert-galaxies</subject><subject>redshifted</subject><description>The corona is an integral component of active galactic nuclei (AGNs) which produces the bulk of the X-ray emission above 1-2keV. However, many of its physical properties and the mechanisms powering this emission remain a mystery. In particular, the temperature of the coronal plasma has been difficult to constrain for large samples of AGNs, as constraints require high-quality broadband X-ray spectral coverage extending above 10keV in order to measure the high-energy cutoff, which provides constraints on the combination of coronal optical depth and temperature. We present constraints on the coronal temperature for a large sample of Seyfert 1 AGNs selected from the Swift/BAT survey using high-quality hard X-ray data from the NuSTAR observatory combined with simultaneous soft X-ray data from Swift/XRT or XMM-Newton. When applying a physically motivated, nonrelativistic disk-reflection model to the X-ray spectra, we find a mean coronal temperature kT_e_=84+/-9keV. We find no significant correlation between the coronal cutoff energy and accretion parameters such as the Eddington ratio and black hole mass. We also do not find a statistically significant correlation between the X-ray photon index, {Gamma}, and Eddington ratio. This calls into question the use of such relations to infer properties of supermassive black hole systems.</description><source format="bibcode">2022ApJ...927...42K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/927/42</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/B/swift">B/swift : Swift Master Catalog (HEASARC, 2004-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/xmm">B/xmm : XMM-Newton Obs. Log (XMM-Newton Science Operation Center, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/76">VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/417">J/A+A/505/417 : Second INTEGRAL AGN catalogue (Beckmann+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1177">J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/19">J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 6yrs (Baumgartner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/3309">J/MNRAS/466/3309 : X-ray flux variability of AGN (Rani+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/836/99">J/ApJ/836/99 : NuSTAR serendipitous survey: 40-month cat. (Lansbury+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/850/74">J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/233/17">J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/4">J/ApJS/235/4 : 105-month Swift-BAT all-sky hard X-ray survey (Oh+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/869/171">J/ApJ/869/171 : Chandra observations of NuSTAR sources (Tomsick+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A31">J/A+A/640/A31 : R-Gamma correlation of Swift/BAT AGN (Panagiotou+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/257/61">J/ApJS/257/61 : X-ray spectral study of 57 local U/LIRGs (Yamada+, 2021)</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/ApJ/927/42</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/927/42</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/927/42</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/927/42</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/927/42</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/927/42</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/ApJ/927/42/table1 (Redshifts, black hole masses and best-fit spectral parameters from fitting broadband X-ray data)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/927/42/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/927/42/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/927/42/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>51.2594781</ra><dec>-41.9048939</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/134 731 941 1405 2505 3075 4439 4488 4540 5972 6097 6923 6928 7277 7571 7642 7713 7921 8029 8071 8216 8299 8812 8922 10454 10912 10927 10991 11388 11490 12025 12251 12254 12921 13179 13186 14534 14541 14858 16184 16301 16333 17075 17408 17727 17814 17846 18524 18683 19283 19296 19373 19767 22890 24848 25182 25572 25580 25585 26148 27382 27477 27501 27803 28060 28275 28517 29795 29906 31833 32279 32344 32658 32931 33282 33394 33930 34034 34065 34104 34294 34458 34730 34768 34812 34881 35038 36015 36775 36786 38268 39295 40838 41014 42120 42852 43632 43634 43649 43877 43983 45222 46124 47169 47222 48022</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/927/42?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/927/42/table1</name><description>Redshifts, black hole masses and best-fit spectral parameters from fitting broadband X-ray data</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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