J/A+A/298/375ivo://CDS.VizieR/J/A+A/298/375doi:10.26093/cds/vizier.32980375CDSFALCKE H.MALKAN M.A.BIERMANN P.L.1999-02-26T14:00:35Z1999-02-26T15:00:27ZCDS support team

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

cds-question@unistra.frquasarsradio-galaxiesWe investigate the correlation between the accretion disk (UV) luminosity and the radio core emission of a quasar sample, containing all PG quasars, also deriving empirical conversion factors from emission line luminosities to disk luminosities. This method allows us to investigate the radio properties of AGN on the absolute scale set by the accretion power. The tables contain the quasar (and radio galaxy) sample discussed in this paper (including the complete PG quasars sample) and give the derived `disk luminosities' of the UV-bump and 5GHz radio luminosities.1995A&A...298..375Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/298/375CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/298/375https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/298/375http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/298/375https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/298/375https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/298/375http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/298/375GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/A+A/298/375/table1The quasar sample used in this paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintQuasar[1-131]+ Quasar ID number (1)meta.idintprimaryindexedNameQuasar IAU namemeta.id;meta.maincharzRedshiftsrc.redshiftfloatClassClass (2)src.classcharlog(Ldisk)Logarithm of average disk luminositylog(1e-07W)phys.luminosityfloatlog(LdiskUV)[]? Logarithm of disk luminosity derived from UV-bump fitslog(1e-07W)phys.luminosityfloatnullablelog(LdiskMb)[]? Logarithm of disk luminosity derived from absolute blue magnitudelog(1e-07W)phys.luminosityfloatnullablelog(LdiskMv)[]? Logarithm of disk luminosity derived from absolute magnitude of the continuum at 5500 Alog(1e-07W)phys.luminosityfloatnullablelog(LdiskeL)[]? Logarithm of disk luminosity derived from emission lines seen in the optical spectrumlog(1e-07W)phys.luminosityfloatnullablel_log(nu*L_nu_)Limit flag on radio luminositymeta.code.errorcharlog(nu*L_nu_)Logarithm of Radio luminosity of the core at 5GHz rest framelog(1e-07W)phys.luminosity;em.radiofloatl_f(c)Limit flag on ratio f(c)meta.code.errorcharf(c)Radio of core flux to total flux at 5GHz rest frame%phot.flux;arith.ratiofloatalphaDifferential spectral index of fitted spectrum at 5GHz rest framespect.indexfloatJ/A+A/298/375/table2The FR II sample used in this paperNameQuasar IAU namemeta.id;meta.maincharzRedshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintQuasar[132-170]+ Quasar ID numbermeta.idintprimaryindexedLdiskLogarithm of the disk luminosity derived by multiplying the lobe power calculated by Rawlings and Saunders (1991)log(1e-07W)phys.luminosityfloatl_log(nu*L_nu_)Limit flag on radio luminositymeta.code.errorcharlog(nu*L_nu_)Logarithm of radio luminosity of the core at 5GHz rest framelog(1e-07W)phys.luminosity;em.radiofloatl_f(c)Limit flag on ratio f(c)meta.code.errorcharf(c)Radio of core flux to total flux at 5GHz rest frame%phot.flux;arith.ratiofloatalphaDifferential spectral index of fitted spectrum at 5GHz rest framespect.indexfloat