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<ri:Resource created="2022-02-02T09:38:44Z" 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>Radio properties of Swift/BAT AGNs</title><shortName>J/ApJ/900/125</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/125</identifier><altIdentifier>doi:10.26093/cds/vizier.19000125</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rusinek K.</name></creator><creator><name>Sikora M.</name></creator><creator><name>Koziel-Wierzbowska D.</name></creator><creator><name>Gupta M.</name></creator><date role="Updated">2022-05-18T12:48:10Z</date><date role="Created">2022-02-02T09:38:44Z</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>radio-sources</subject><subject>redshifted</subject><subject>galaxy-classification-systems</subject><description>We address the very large diversity of jet production efficiency in active galactic nuclei (AGNs) by using data on low-redshift AGNs selected from the Swift/BAT catalog and having black hole (BH) masses larger than 10^8.5^M_{sun}_. Most of these AGNs accrete at intermediate rates and have bolometric luminosities dominated by mid-IR radiation. Our sample contains 14% radio-loud (RL), 6% radio-intermediate, and 80% radio-quiet (RQ) AGNs. All RL objects are found to have extended radio structures, and most of them have classical FR II morphology. Converting their radio loudness to jet production efficiency, we find that the median of this efficiency is on the order of ({epsilon}_d_/0.1)%, where {epsilon}_d_=L_bol_/(dM/dt)c^2^ is the radiation efficiency of the accretion disk. Without knowing the contribution of jets to the radio emission in RQ AGNs, we are only able to estimate their efficiencies using upper limits. Their median is found to be 0.002({epsilon}_d_/0.1)%. Our results suggest that some threshold conditions must be satisfied to allow the production of strong, relativistic jets in RL AGNs. We discuss several possible scenarios and argue that the production of collimated, relativistic jets must involve the Blandford-Znajek mechanism and can be activated only in those AGNs whose lifetime is longer than the time required to enter the magnetically arrested disk (MAD). Presuming that MAD is required to collimate relativistic jets, we expect that the weak nonrelativistic jets observed in some RQ AGNs are produced by accretion disks rather than by rotating BHs.</description><source format="bibcode">2020ApJ...900..125R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/125</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/eso">B/eso : ESO Science Archive Catalog (ESO, 1991-2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/81">VIII/81 : Sydney University Molonglo Sky Survey (SUMSS V2.1) (Mauch+ 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/92">VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/132/31">J/A+AS/132/31 : Kinematical models for double radio sources (Nilsson 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/164/307">J/ApJS/164/307 : NICMOS observations of 3CR radio sources (Madrid+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/815">J/ApJ/658/815 : Radio loudness of active galactic nuclei (Sikora+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/42">J/AJ/137/42 : Matched SDSS and FIRST Sample (Rafter+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/1013">J/MNRAS/415/1013 : FR II radio galaxies in SDSS (Koziel-Wierzbowska+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/62">J/ApJ/765/62 : SDSS-DR7 opt. spectra analysis of radio gal. (Sikora+, 2013)</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/ApJ/870/31">J/ApJ/870/31 : BAT AGN spectroscopic survey. XI. IR phot. (Ichikawa+, 2019)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home page</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/900/125</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/900/125</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/900/125</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/900/125</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/900/125</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/900/125</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/900/125/table4 (Swift/BAT 314 AGNs used in this study)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/900/125/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/900/125/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/900/125/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>0.4419922</ra><dec>-76.9539781</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/43 406 815 879 941 953 1093 1405 1526 1919 2004 2147 2206 2216 2251 2276 2531 3233 3309 3502 3771 4369 4535 4540 4589 4784 4834 5018 5097 5284 5395 5463 5996 6113 6212 6386 6502 6583 6920 6923 6928 6977 7166 7422 7502 7628 7713 7728 7815 7959 8030 8071 8216 8641 8658 8812 8845 8868 9099 9231 9375 9490 9665 9942 10118 10141 10348 10707 10788 10847 10991 11158 11490 11615 11658 11668 11683 11842 11898 11991 12025 12251 12254 12547 12921 13079 13179 13273 13511 13541 13707 13720 14744 14858 15135 15331 15351 16100 16184 16301 16333 16690 16805 16853 17075 17448 17525 17548 17627 17727 17748 17795 17814 17964 17992 18083 18365 18402 18524 18683 18769 18794 19070 19283 19373 19433 19499 19746 19932 20079 20107 20309 20489 20556 20676 20750 21016 21186 21245 21905 21953 22186 22365 22626 22632 22890 23167 23476 24022 24228 24288 24699 24842 24848 25035 25403 25553 25580 25619 25676 25742 25965 26071 26148 26375 26393 26509 26515 26547 26650 26767 26861 26874 27382 27477 27504 27699 27767 27803 27815 27976 28060 28153 28259 28275 28352 28471 28545 28609 28626 30140 31401 31940 32028 32143 32279 32344 32447 32456 32658 32931 33038 33239 33282 33394 33398 33571 33716 33924 33928 33930 33958 34065 34190 34412 34414 34430 34499 34531 34669 34726 34768 34812 34881 34907 34983 35038 35049 35085 35246 35263 35521 35608 35741 35934 36005 36158 36216 36382 36396 36552 36595 36668 36786 36890 37054 37068 38113 38129 38205 38479 38704 38923 38948 39149 39295 39322 39717 39722 39778 40838 41014 41087 41499 41982 42005 42009 42179 43359 43452 43634 43667 43695 43768 43877 43983 44448 44507 44517 44526 44551 44668 44790 44892 45220 45222 45258 45446 45500 45883 45985 46005 46101 46124 46281 46424 46544 47027 47064 47074 47169 47308 47971 48022 48394 48491 48614 48798 49042</spatial><spectral>9.276497240453405e-25 9.276497240453405e-25</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/900/125?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/900/125/table4</name><description>Swift/BAT 314 AGNs used in this study</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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