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<ri:Resource created="2024-06-03T11:33:05Z" 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>Broad emission line of 4FGL blazars</title><shortName>J/ApJS/271/20</shortName><identifier>ivo://CDS.VizieR/J/ApJS/271/20</identifier><altIdentifier>doi:10.26093/cds/vizier.22710020</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chen G.</name></creator><creator><name>Zheng Z.</name></creator><creator><name>Zeng X.</name></creator><creator><name>Zhang L.</name></creator><creator><name>Xiao H.</name></creator><creator><name>Liu X.</name></creator><creator><name>Cui L.</name></creator><creator><name>Fan J.</name></creator><date role="Updated">2024-11-06T20:31:03Z</date><date role="Created">2024-06-03T11:33:05Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>redshifted</subject><subject>bl-lacertae-objects</subject><subject>quasars</subject><description>In this work, we obtained a sample of 979 Fermi blazars with broad emission lines, including 701 objects collected from published works and 278 objects developed in this work. For the 278 objects, we made a crossmatch from three catalogs, the Fermi Large Area Telescope Fourth Source Catalog (4FGL), the Sloan Digital Sky Survey, and the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, and calculated the broad-line region (BLR) luminosity. Then, we estimated the Doppler factor and studied the correlations between the BLR luminosities and the {gamma}-ray luminosities, the synchrotron peak frequency ({nu}p), and Doppler factor ({delta}) for the whole sample. Our analyses and discussions came to the following main conclusions: For the 278 blazars, their BLR luminosity (log LBLR) ranges from 40.44 to 45.45erg/s, with a mean value of 43.39erg/s. The Doppler factor ranges from {delta}=0.45 to {delta}=88.52, with a mean value of 12.99 for the 979 Fermi blazars, which is consistent with the results in the literature. Both the BLR luminosity and the Doppler factor exhibit positive correlations with the {gamma}-ray luminosity. The BLR luminosity is anticorrelated with synchrotron peak frequency, implying a Compton cooling. A line of logL_BLR_=1.58log{nu}_p_-19.46 separating BL Lacertae objects and flat-spectrum radio quasars was obtained in the diagram of logL_BLR_ against log{nu}_p_ using a machine-learning method. Based on the analysis of the equivalent width and the Doppler factors, we proposed five changing-look blazar candidates.</description><source format="bibcode">2024ApJS..271...20C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/271/20</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/V/156">V/156 : LAMOST DR7 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/67">IX/67 : Incremental Fermi LAT 4th source cat. 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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. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sp</name><description>Display the emission line fluxes of this source (link to Table 2)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>4FGL</name><description>4FGL-DR4 catalog identifier (JHHMM.m+DDMM)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType><flag>primary</flag></column><column><name>Name</name><description>Other name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>z</name><description>[0.027/4.4] Spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>C1</name><description>4FGL-DR4 catalog classification (1)</description><ucd>meta.code.class;src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>C2</name><description>Yang+ 2022, J/ApJS/262/18 classification</description><ucd>meta.code.class;src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>lognu</name><description>[12.1/18.2]? Log peak frequency (2)</description><unit>log(Hz)</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F0.1-100</name><description>[5e-13/7.4e-10] The 0.1-100GeV gamma-ray flux; erg/cm^2^/sr</description><unit>mW.m**-2.sr**-1</unit><ucd>phot.flux;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>alpha</name><description>[1.4/3.3] 4FGL-DR4 catalog photon spectral index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLg</name><description>[42.8/48.9] Log 0.1-100GeV gamma-ray luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.gamma</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLBLR</name><description>[40.4/46.7] Log Broad-Line Region luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_logLBLR</name><description>Reference code for logLBLR (3)</description><ucd>meta.ref;phys.luminosity</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>delta</name><description>[0.45/88.6] Doppler factor from this work</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DR3</name><description>Display data from 4FGL-DR3 (IX/67)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Y22</name><description>Display data from Yang+ 2022, J/ApJS/262/18</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions from SIMBAD or from the 4FGL-DR4 (https://fermi.gsfc.nasa.gov/ssc/data/access/lat/14yr_catalog/gll_psc_v32.reg) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from SIMBAD or from the 4FGL-DR4 (https://fermi.gsfc.nasa.gov/ssc/data/access/lat/14yr_catalog/gll_psc_v32.reg) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJS/271/20/table2</name><description>The 278 Fermi blazars whose optical spectra exhibit at least one of the broad emission lines H{alpha}, H{beta}, MgII, and CIV</description><column><name>4FGL</name><description>4FGL-DR4 catalog identifier (JHHMM.m+DDMM)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>z</name><description>[0.04/4.1] Spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Class</name><description>Classification (1)</description><ucd>meta.code.class;src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>FHa</name><description>[8.7/62567]? Halpha emission line flux; 1e-17erg/s/cm^2^</description><unit>1e-20W.m**-2</unit><ucd>phot.flux;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FHa</name><description>[0/543]? Uncertainty in FHa</description><unit>1e-20W.m**-2</unit><ucd>stat.error;phot.flux;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FHb</name><description>[4.9/19028]? Hbeta emission line flux; 1e-17erg/s/cm^2^</description><unit>1e-20W.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_FHb</name><description>[3.8/1455]? Uncertainty in FHb</description><unit>1e-20W.m**-2</unit><ucd>stat.error;phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FMgII</name><description>[8.2/1745]? MgII emission line flux; 1e-17erg/s/cm^2^</description><unit>1e-20W.m**-2</unit><ucd>phot.flux;em.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FMgII</name><description>[4.9/153]? Uncertainty in FMgII</description><unit>1e-20W.m**-2</unit><ucd>stat.error;phot.flux;em.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FCIV</name><description>[7.6/4074]? CIV emission line flux; 1e-17erg/s/cm^2^</description><unit>1e-20W.m**-2</unit><ucd>phot.flux;em.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FCIV</name><description>[5.7/1416]? Uncertainty in FCIV</description><unit>1e-20W.m**-2</unit><ucd>stat.error;phot.flux;em.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLBLR</name><description>[40.44/45.45] Log Broad-line region luminosity; erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logLBLR</name><description>[0/0.5] Uncertainty in logLBLR</description><unit>log(1e-07W)</unit><ucd>stat.error;phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>