J/other/RAA/20.2ivo://CDS.VizieR/J/other/RAA/20.25doi:10.26093/cds/vizier/dx/cakcfCDSPei Z.-Y.Fan J.-H.Bastieri D.Yang J.-H.Xiao H.-B.Yang W.-X.2026-02-10T20:07:50Z2021-10-01T13:41:10ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fractive-galactic-nucleiradio-sourcesActive galactic nuclei (AGNs) can be divided into two major classes, namely radio-loud and radio-quiet AGNs. A small subset of the radio-loud AGNs is called blazars, which are believed to be unified with Fanaroff-Riley type I and type II (FRI&II) radio galaxies. Following our previous work, we present a latest sample of 966 sources with measured radio flux densities of the core and extended components. The sample includes 83 BL Lacs, 473 flat spectrum radio quasars, 101 Seyferts, 245 galaxies, 52 FRIs&IIs and 12 unidentified sources. We then calculate the radio core-dominance parameters and spectral indices and study their relationship. Our analysis shows that the core-dominance parameters and spectral indices are quite different for different types of sources. We also confirm that the correlation between core-dominance parameter and radio spectral index extends over all the sources in a large sample presented.2020RAA....20...25Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/RAA/20.25CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/other/RAA/19.70 : Sample of 2400 AGNs (Pei+, 2019)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/RAA/20.25https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/RAA/20.25http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/RAA/20.25https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/other/RAA/20.25https://vizier.iucaa.in/viz-bin/votable?-source=J/other/RAA/20.25http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/other/RAA/20.25GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/other/RAA/20.25/table1for the whole sourcesNameSource namemeta.id;meta.maincharnu1[4/5]? First frequency for emissionGHzem.freqintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClassClassification (1)meta.code.classcharzRedshiftsrc.redshiftdoubleScoreCore-emission at nu1mJyphot.flux.density;em.radiofloatSext? Extended emission at nu1mJyphot.flux.density;em.radiodoublenullableSTotal1? Total emission at nu1mJyphot.flux.density;em.radiodoublenullabler_ScoreReference for Score, Sext and STotal1, in refs.dat filemeta.ref;pos.framecharlogRCore-dominance parameter at 5 GHzphot.flux;arith.ratiofloatnu2[0.85/4.85]? Second frequency (from NED)GHzem.freqfloatnullableSTotal2? Total emission at nu2 (from NED)mJyphot.flux.density;em.radiodoublenullablealpha? Radio spectral index, alpha_R_ (S_nu_ {prop.to} nu^-alphaR^ (from NED)spect.indexfloatnullableJ/other/RAA/20.25/refsReferencesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibCodeBibCodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorcharComCommentsmeta.notechar