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<ri:Resource created="2017-10-04T09:39:37Z" 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>Fermi blazars with Doppler factors</title><shortName>J/ApJ/835/L38</shortName><identifier>ivo://CDS.VizieR/J/ApJ/835/L38</identifier><altIdentifier>doi:10.26093/cds/vizier.18359038</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fan J.H.</name></creator><creator><name>Yang J.H.</name></creator><creator><name>Xiao H.B.</name></creator><creator><name>Lin C.</name></creator><creator><name>Constantin D.</name></creator><creator><name>Luo G.Y.</name></creator><creator><name>Pei Z.Y.,Hao J.M.</name></creator><creator><name>Mao Y.W.</name></creator><date role="Updated">2017-11-03T14:09:35Z</date><date role="Created">2017-10-04T09:39:37Z</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>x-ray-sources</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>bl-lacertae-objects</subject><subject>quasars</subject><description>Blazars are an extreme subclass of active galactic nuclei. Their rapid variability, luminous brightness, superluminal motion, and high and variable polarization are probably due to a beaming effect. However, this beaming factor (or Doppler factor) is very difficult to measure. Currently, a good way to estimate it is to use the timescale of their radio flares. In this Letter, we use multiwavelength data and Doppler factors reported in the literature for a sample of 86 flaring blazars detected by Fermi to compute their intrinsic multiwavelength data and intrinsic spectral energy distributions and investigate the correlations among observed and intrinsic data. Quite interestingly, intrinsic data show a positive correlation between luminosity and peak frequency, in contrast with the behavior of observed data, and a tighter correlation between {gamma}-ray luminosity and the lower-energy ones. For flaring blazars detected by Fermi, we conclude that (1) observed emissions are strongly beamed; (2) the anti-correlation between luminosity and peak frequency from the observed data is an apparent result, the correlation between intrinsic data being positive; and (3) intrinsic {gamma}-ray luminosity is strongly correlated with other intrinsic luminosities.</description><source format="bibcode">2017ApJ...835L..38F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/835/L38</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/ApJS/123/79">J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/436/799">J/A+A/436/799 : X- &amp; gamma-ray fluxes of {gamma}-ray-loud blazars (Fan+, 2005)</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/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/AJ/138/1874">J/AJ/138/1874 : MOJAVE. 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Kinematic analysis of blazar jets (Lister+, 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/ApJS/199/31">J/ApJS/199/31 : Fermi LAT second source catalog (2FGL) (Nolan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/541/A160">J/A+A/541/A160 : Planck + X/{gamma} observations of blazars (Giommi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/761/125">J/ApJ/761/125 : X and {gamma} spectral indexes of Fermi blazars (Fan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/25">J/ApJS/208/25 : Swift X-ray observations of 1FGL sources (Takeuchi+, 2013)</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/ApJS/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</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/ApJS/224/26">J/ApJS/224/26 : Spectral energy distributions of Roma BZCAT blazars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/226/20">J/ApJS/226/20 : X-ray, opt. + radio SEDs of Fermi blazars (Fan+, 2016)</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/835/L38</accessURL><mirrorURL title="VizieR at IUCAA: 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