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<ri:Resource created="2023-05-05T13:38:11Z" status="active" updated="2025-09-09T14:15:18Z" 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>gamma-ray properties of FR-Is and BL Lacs</title><shortName>J/PASP/135/A4101</shortName><identifier>ivo://CDS.VizieR/J/PASP/135/A4101</identifier><altIdentifier>doi:10.26093/cds/vizier.61354101</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ye X.-H.</name></creator><creator><name>Zeng X.-T.</name></creator><creator><name>Huang D.-Y.</name></creator><creator><name>Zhang Z.</name></creator><creator><name>Pei Z.-Y.</name></creator><creator><name>Fan J.-H.</name></creator><date role="Updated">2025-09-09T14:15:18Z</date><date role="Created">2023-05-05T13:38:11Z</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-galaxies</subject><subject>bl-lacertae-objects</subject><subject>gamma-ray-astronomy</subject><subject>redshifted</subject><description>Our knowledge of Giga-electron volt (GeV) radio galaxies has been revolutionized by the Fermi-LAT Telescope, which provides an excellent opportunity to study the physical properties of GeV radio galaxies. According to the radio power and morphology, radio galaxies can be separated into Fanaroff-Riley Type I radio galaxies (FR-Is) and Type II radio galaxies (FR-IIs). In this paper, we consider the unification of FR-Is and BL Lacertae objects (BL Lacs), and assume FR-Is to be a standard candle to discuss the beaming effect for Fermi-LAT-detected FR-Is. Our main conclusions are as follows: (1) The estimated Doppler factors for 30 Fermi-LAT-detected FR-Is are in a range of {delta}_I_=0.88-7.49. The average Doppler factor (&lt;{delta}_I_&gt;=2.56+/-0.30) of the 30 FR-Is is smaller than that (&lt;{delta}_BL_&gt;=10.28+/-2.03) of the 126 Fermi-LAT-detected BL Lacs, supporting the unification model that FR-Is are regarded as the misaligned BL Lacs with smaller Doppler factors; (2) We propose that different regions of FR-Is in the plot of the {gamma|-ray luminosity against the photon spectral index logL_{gamma}-{alpha}_ph_ may indicate the different beaming effects; (3) The average Doppler factor of the 6 TeV FR-Is is similar to that of the 24 non-TeV FR-Is, which implies that the difference between the TeV and GeV emissions is not driven by the beaming effect in the Fermi-LAT-detected FR-I samples.</description><source format="bibcode">2023PASP..135a4101Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASP/135/A4101</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)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/866/137">J/ApJ/866/137 : Bright blazars variability brightness temp. 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