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<ri:Resource created="2024-05-02T09:06:07Z" status="active" updated="2026-02-10T20:08:26Z" 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>Blazars properties</title><shortName>J/other/RAA/23.K</shortName><identifier>ivo://CDS.VizieR/J/other/RAA/23.K5009</identifier><altIdentifier>doi:10.26093/cds/vizier/dx/cdkvfaaj</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhang H.</name></creator><creator><name>Zhang H.J.</name></creator><date role="Updated">2026-02-10T20:08:26Z</date><date role="Created">2024-05-02T09:06:07Z</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>gamma-ray-astronomy</subject><subject>bl-lacertae-objects</subject><subject>black-holes</subject><subject>magnetic-fields</subject><subject>stellar-masses</subject><description>We analyzed the relationship between several basic parameters describing supermassive black holes such as jet power, black hole spin, accretion disk magnetic field, black hole mass, etc. We found that there is a general correlation between these parameters, such as jet power is significantly positively correlated with black hole spin, while black hole mass is significantly negatively correlated with black hole spin. To apprehend these relationships, we consider the Blandford-Znajek model to be superior to the Blandford-Payne model. It is also found that the intrinsic gamma luminosity of the FSRQs has a positive correlation with the accretion disk magnetic field, while the intrinsic gamma luminosity of the BL Lacs has a negative correlation with the accretion disk magnetic field. A feedback effect may exist between accretion disk accretion rate and magnetic field, which may be the key to the evolution between BL Lacs and FSRQs. There is no significant difference in the jet power and jet generation efficiency of FSRQs and BL Lacs, which suggests that the jets are generated by the same mechanism. The contribution rate of accretion rate to jet generation efficiency is high, while the contribution rate of accretion rate to jet power is very low.</description><source format="bibcode">2023RAA....23k5009Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/RAA/23.K5009</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></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/other/RAA/23.K5009</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/RAA/23.K5009</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/RAA/23.K5009</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/other/RAA/23.K5009</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/other/RAA/23.K5009</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/other/RAA/23.K5009</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/other/RAA/23.K5009/table1 (The samples)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/other/RAA/23.K5009/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/other/RAA/23.K5009/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/other/RAA/23.K5009/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>180.7646133</ra><dec>60.5219897</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/438 579 808 911 1509 2234 2741 2836 3024 3128 4285 4572 4695 4770 4820 4880 4940 5139 5154 5201 5371 5390 5458 5546 5693 5795 5817 5870 6018 6167 6777 7346 7389 7426 7446 7709 7896 7969 8199 8299 8466 8487 8699 8830 9003 9075 9442 9460 9545 9629 9676 9723 9914 10249-10250 10352 10422 10426 10466 10548 10681 10971 11081 11177 11242 11430 11777 12173 12386 12466 12475 12599 12687 13352 13410 13485 13572 13729 13927 14854 15286 16027 16059 16298 16971 17364 17665 18035 18092 18624 18853 19023 19109 19190 19398 19593 19622 19878 20099 20888 21266 21358 21437 21935 21968 21972 22305 22363 22396 22501 22558 22730 22950 23383 23416 23436 23691 23897 24084 25501 25649 26303 26983 27060 27243 27310 27433 28083 28370 28479 28492 28517 28673 29772 30446 31430 31451 31664 31757 31894 33774 34038 34461 34637 34767 35119 35370 36090 36665 38766 43451 44730 45943 46204 46835 47512 48300</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/other/RAA/23.K5009?format=ascii</footprint><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/other/RAA/23.K5009/table1</name><description>The samples</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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