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<ri:Resource created="2025-02-26T13:24:29Z" status="active" updated="2025-05-21T20:14:45Z" 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>Fermi jetted AGN with reliable redshift</title><shortName>J/ApJ/944/157</shortName><identifier>ivo://CDS.VizieR/J/ApJ/944/157</identifier><altIdentifier>doi:10.26093/cds/vizier.19440157</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen Y.</name></creator><creator><name>Gu Q.</name></creator><creator><name>Fan J.</name></creator><creator><name>Yu X.</name></creator><creator><name>Ding N.</name></creator><creator><name>Xiong D.</name></creator><creator><name>Guo X.</name></creator><date role="Updated">2025-05-21T20:14:45Z</date><date role="Created">2025-02-26T13:24:29Z</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>gamma-ray-astronomy</subject><subject>radio-sources</subject><subject>bl-lacertae-objects</subject><subject>quasars</subject><subject>seyfert-galaxies</subject><subject>redshifted</subject><subject>black-holes</subject><description>We collect a large sample with a reliable redshift detected by the Fermi satellite after 10yr of data (4FGL-DR2), including blazars, gamma-ray narrow-line Seyfert 1 galaxies ({gamma}NLS1s), and radio galaxies. The spectral energy distributions of these Fermi sources are fitted by using a second-degree polynomial, and some important parameters including spectral curvature, synchrotron peak frequency, and peak luminosity are obtained. Based on those parameters, we discuss the Fermi blazar sequence and the particle acceleration mechanism. Our main results are as follows: (i) By studying the relationship between the synchrotron peak frequency and the synchrotron peak frequency luminosity, jet kinetic power, and gamma-ray luminosity for jetted active galactic nuclei (AGNs), we find an "L" shape in the Fermi blazar sequence. (ii) There is a significant anticorrelation between the Compton dominance, the black hole spin, and the synchrotron peak frequency for jetted AGNs, respectively. These results support that the {gamma}NLS1s and radio galaxies belong to the Fermi blazar sequence. (iii) On the basis of previous work, statistical or stochastic acceleration mechanisms can be used to explain the relationship between the synchrotron peak frequency and synchrotron curvature. For different subclasses, the correlation slopes are different, which implies that the Fermi sources of different subclasses have different acceleration mechanisms. (iv) Flat-spectrum radio quasars and {gamma}NLS1s have a higher median spin of a black hole than BL Lac objects and radio galaxies.</description><source format="bibcode">2023ApJ...944..157C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/944/157</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/IX/67">IX/67 : Incremental Fermi LAT 4th source cat. (4FGL-DR3) (Fermi-LAT col., 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/739">J/A+A/375/739 : Hard X-ray properties of blazars (Donato+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/441">J/A+A/445/441 : SED of BL Lacertae objects (Nieppola+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/859">J/ApJ/686/859 : Radio sources at 0.327, 1.4, 4.5, 8.5GHz (Birzan+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/867">J/A+A/488/867 : Synchrotron peak frequency of 135 AGN (Nieppola+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/30">J/ApJ/716/30 : SED of Fermi bright blazars (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/742/27">J/ApJ/742/27 : 15GHz and jet properties of MOJAVE blazars (Lister+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/740/98">J/ApJ/740/98 : Synchrotron peak for blazars and radio gal. (Meyer+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/14">J/ApJ/810/14 : Third catalog of LAT-detected AGNs (3LAC) (Ackermann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/448/1060">J/MNRAS/448/1060 : Fermi/LAT broad emission line blazars (Ghisellini+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/33">J/ApJS/247/33 : Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/495/981">J/MNRAS/495/981 : Jet efficiencies &amp; black hole spins in QSOs (Soares+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/505/4726">J/MNRAS/505/4726 : Study of relativistic jets in blazar objects (Keenan+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/46">J/ApJS/253/46 : Optical spectroscopy of Fermi blazars (Paliya+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/658/A12">J/A+A/658/A12 : Origins of radio emission in NLS1s (Jarvela+, 2022)</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/944/157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/944/157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/944/157</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/944/157</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/944/157</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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