J/A+A/672/A164ivo://CDS.VizieR/J/A+A/672/A164doi:10.26093/cds/vizier.36720164CDSPoitevineau R.Castignani G.Combes F.2024-11-28T20:02:53Z2023-04-19T08:36:13ZCDS support team

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

cds-question@unistra.frquasarsactive-galactic-nucleiradio-galaxiesredshiftedThe relation between the mass of the supermassive black hole (SMBH) in the center of galaxies and their bulge mass or central velocity dispersion is well known. This suggests a coevolution between the SMBHs and their galaxy hosts. Our aim is to study this relation, specifically, for radio loud galaxies, and as a function of redshift z. We selected a sample of 42 radio galaxies and active galactic nuclei (AGN) with broad emission lines and spectroscopic redshifts between z=0.3-4 by cross-matching the low radio frequency sources from Very Large Array (VLA) FIRST with spectroscopically confirmed galaxies from wide-field surveys, including Sloan Digital Sky Survey (SDSS) DR14 ugriz and Dark Energy Survey (DES) DR2 grzY in the optical, Wield Infrared Survey Explorer (WISE), and the Galaxy And Mass Assembly (GAMA) spectroscopic survey. We characterized the stellar mass (M_*_), star formation, and black hole properties (mass of the central SMBH, Eddington ratio {eta} , and jet power, Q_mjet_. The relation between SMBH mass, M_*_, {eta} , and z is placed into context by comparing them with scaling relations (M_mBH_-M_*_, M_mBH_/M_*_-z, M_mBH-Q_mjet_, and Q_mjet_-{eta} from the literature. On the basis of a multiwavelength spectral energy distribution modeling, our radio sources are broadly consistent with being on the star-forming main sequence. They have sub-Eddington accretion rates, {eta}~=1% on average, as typically found in type I AGN, while higher accretion rates favor more powerful jets to be launched by the central engine. We find overmassive SMBHs in (17+/-5% of our radio sources, similarly to previous studies on nearby early-type galaxies. Altogether, an evolutionary scenario in which radio-mode AGN feedback regulates the accretion onto the SMBHs and the stellar mass assembly of the radio sources is discussed, which may explain the observed phenomenology. This pilot study represents a benchmark for future studies using wide-field surveys such as Euclid and the Vera Rubin telescope.2023A&A...672A.164Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/672/A164CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/672/A164https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/672/A164http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/672/A164https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/672/A164https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/672/A164http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/672/A164GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/672/A164/tablea (Properties of the radio sources in our (tables 1 and 2)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/672/A164/tablea?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/672/A164/tablea?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/672/A164/tablea?GETtext/xml+votable180.050000true35.8955833-6.62305280.0055555555555555566/4097 17669 17683 17686 17688-17690 17692 17747 17750-17751 17753 17756-17757 21844 21850 21854 21873 25587 25935 25939 25964-25966 25971 25976 26053 26056 26255 26275 26277-26278 26970 27301https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/672/A164?format=asciiRadiodefaultJ/A+A/672/A164/tableaProperties of the radio sources in our (tables 1 and 2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDGalaxy ID numbermeta.idintRAJ2000Right ascension of center (J2000)pos.eq.ra;meta.mainDEJ2000Declination of center (J2000)pos.eq.dec;meta.mainzSpectroscopic redshiftsrc.redshiftdoublelogL1.4GHz1.4GHz rest-frame luminosity densitylog(1e-07W.Hz**-1)phys.luminosity;em.radio.750-1500MHzfloate_logL1.4GHzError on the 1.4GHz rest-frame luminosity densitylog(1e-07W.Hz**-1)stat.errorfloatlogLdustDust SED-based dust luminositylog(solLum)phys.luminosityfloatlogMstarStellar SED-based dust masslog(solMass)phys.massfloatl_SFRUpper limit flag on SFRmeta.code.error;phys.SFRcharSFRStar formation ratesolMass/yrphys.SFRfloatWISEWISE color-based classmeta.code.classcharTypeSource typemeta.code.classcharNameSource namemeta.id;meta.maincharLineBroad emission line usedmeta.id;spect.linecharFWHMFull Width Half Maximum of the line1000km/sspect.line.widthfloate_FWHMError on the Full Width Half Maximum1000km/sstat.error;phys.angSizefloatlogLlineLuminosity of the linelog(1e-07W)phys.luminosityfloate_logLlineError on the line luminositylog(1e-07W)stat.errorfloatMbhCentral Black Hole masslog(solMass)phys.massfloate_MbhStatistical error on the black hole masslog(solMass)stat.errorfloatlogQjetJet powerlog(1e-07W)phys.luminosityfloatlogLblrBroad line region luminositylog(1e-07W)phys.luminosityfloatlogetaLog of the Eddington ratiophys.luminosity;arith.ratiofloat