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<ri:Resource created="2023-10-04T08:49:18Z" status="active" updated="2025-05-22T20:12:01Z" 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-LAT-detected blazars fundamental parameters</title><shortName>J/ApJ/925/97</shortName><identifier>ivo://CDS.VizieR/J/ApJ/925/97</identifier><altIdentifier>doi:10.26093/cds/vizier.19250097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pei Z.</name></creator><creator><name>Fan J.</name></creator><creator><name>Yang J.</name></creator><creator><name>Huang D.</name></creator><creator><name>Li Z.</name></creator><date role="Updated">2025-05-22T20:12:01Z</date><date role="Created">2023-10-04T08:49:18Z</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>bl-lacertae-objects</subject><subject>quasars</subject><subject>gamma-ray-astronomy</subject><subject>redshifted</subject><description>Aiming to delineate the physical framework of blazars, we present an effective method to estimate four important parameters based on the idea proposed by Becker &amp; Kafatos (1995ApJ...453...83B), including the upper limit of central black hole mass M, the Doppler factor {delta}, the distance along the axis to the site of the {gamma}-ray production d (which then can be transformed into the location of {gamma}-ray-emitting region R_{gamma}_) and the propagation angle with respect to the axis of the accretion disk {Phi}. To do so, we adopt an identical sample with 809 Fermi-LAT-detected blazars which had been compiled in Pei+ (2020PASA...37...43P). These four derived parameters stepping onto the stage may shed new light on our knowledge regarding {gamma}-ray blazars. With regard to the paper of Becker &amp; Kafatos, we obtain several new perspectives, mainly in (1) putting forward an updated demarcation between BL Lacs and FSRQs based on the relation between broad-line region luminosity and disk luminosity both measured in Eddington units, i.e., L_disk_/L_Edd_=4.68x10^-3^, indicating that there are some differences between BL Lacs and FSRQs on the accretion power in the disk; (2) proposing that there is a so-called "appareling zone", a potential transition field between BL Lacs and FSRQs where the changing-look blazars perhaps reside; (3) the location of {gamma}-ray emission region is principally constrained outside the broad-line region, and for some BL Lacs are also away from the dusty molecular torus, which means the importance of emission components in the jet.</description><source format="bibcode">2022ApJ...925...97P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/925/97</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/VII/274">VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/132/83">J/A+AS/132/83 : BVRI photometry of 7 BL Lac objects (Bai+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/436/799">J/A+A/436/799 : X- &amp; gamma-ray fluxes of blazars (Fan+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/46">J/ApJS/183/46 : LAT bright gamma-ray source list (0FGL) (Abdo+, 2009)</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/715/429">J/ApJ/715/429 : First Fermi-LAT AGN catalog (1LAC) (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/541/A160">J/A+A/541/A160 : Planck + X/{gamma} obs. of blazars (Giommi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/49">J/ApJ/748/49 : Optical sp. of 1LAC broad-line blazars (Shaw+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/13.259">J/other/RAA/13.259 : {gamma}-ray Doppler factor for Fermi blazars (Fan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/14.1135">J/other/RAA/14.1135 : Doppler factor for a Fermi blazar sample (Fan+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/515.376">J/other/Nat/515.376 : Power of relativistic jets in blazars (Ghisellini+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/3568">J/MNRAS/450/3568 : Non-Fermi blazar sample (Xiong+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/451/2750">J/MNRAS/451/2750 : Blazar sequence (Xiong+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/226/20">J/ApJS/226/20 : X-ray, opt. &amp; radio SEDs of Fermi blazars (Fan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/235/39">J/ApJS/235/39 : Jet properties of {gamma}-ray-loud 3FGL AGNs (Chen, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/866/137">J/ApJ/866/137 : Bright blazars var. brightness temp. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>4FGL</name><description>4FGL name, Fermi-LAT (JHHMM.m+DDMM)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>OName</name><description>Other Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>Class</name><description>Classification (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>z</name><description>[0.018/3.11] Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha-g</name><description>[1.54/2.97] {gamma}-ray photon index</description><ucd>spect.index;em.gamma</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLg</name><description>[41.9/48.8] Log, {gamma}-ray luminosity, erg/s</description><unit>1e-07W</unit><ucd>phys.luminosity;em.gamma</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>alpha-X</name><description>[0.04/3.6] X-ray spectral index</description><ucd>spect.index;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FX1keV</name><description>[0.001/240]? 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