J/A+A/686/A43ivo://CDS.VizieR/J/A+A/686/A43doi:10.26093/cds/vizier.36860043CDSIgo Z.Merloni A.Hoang D.Buchner J.Liu T.Salvato M.Arcodia R.,Bellstedt S.Bruggen M.Croston J.H.de Gasperin F.Georgakakis A.,Hardcastle M.J.Nandra K.Ni Q.Pasini T.Shimwell T.Wolf J.2024-11-21T20:01:23Z2024-05-28T11:02:16ZCDS support team

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

cds-question@unistra.frx-ray-sourcesvisible-astronomysloan-photometryinfrared-photometryRadio jets are present in a diverse sample of AGN. However, the mechanisms of jet powering are not fully understood, and it remains unclear to what extent they obey mass-invariant scaling relations similar to those found for the triggering and fuelling of X-ray-selected AGN. We use the multi-wavelength data in the eFEDS field observed by eROSITA/Spectrum-Roentgen-Gamma (SRG) and LOFAR to study the incidence of X-ray and radio AGN as a function of several stellar mass (M*)-normalised AGN power indicators. From the LOFAR-eFEDS survey, we defined a new sample of radio AGN, with optical counterparts from Legacy Survey DR9, according to a radio-excess relative to their host star formation rate. We further divided the sample into compact and complex radio morphologies. In this work, we used the subset matching to the well-characterised, highly complete spectroscopic GAMA09 galaxies (0<z<0.4). We release this value-added LOFAR-eFEDS catalogue. We calculated the fraction of GAMA09 galaxies hosting radio, X-ray, and both radio and X-ray AGN as functions of the specific black hole kinetic (lambda_Jet_) and radiative (lambda_Edd_) power. Despite the soft-X-ray eROSITA-selected sample, the incidence of X-ray AGN as a function of lambda_Edd_ shows the same mass-invariance and power law slope (-0.65) as that found in previous studies once corrected for completeness. Across the M* range probed, the incidence of compact radio AGN as a function of lambda_Jet_ is described by a power law with constant slope, showing that it is not only high mass galaxies hosting high power jets and vice versa. This slope is steeper than that of the X-ray incidence, which has a value of around ~1.5. Furthermore, higher-mass galaxies are more likely to host radio AGN across the lambda_Jet_ range, indicating some residual mass dependence of jet powering. Upon adding complex radio morphologies, including 34 FRIIs, three of which are giant radio galaxies, the incidence not only shows a larger mass dependence but also a jet power dependence, being clearly boosted at high lambda_Jet_ values. Importantly, the latter effect cannot be explained by such radio AGN residing in more dense environments (or more massive dark matter haloes). The similarity in the incidence of quiescent and star-forming radio AGN reveals that radio AGN are not only found in "red and dead" galaxies. Overall, our incidence analysis reveals some fundamental statistical properties of radio AGN samples, but highlights open questions regarding the use of a single radio luminosity-jet power conversion. We explore how different mass and accretion rate dependencies of the incidence can explain the observed results for varying disk-jet coupling models.2024A&A...686A..43Ihttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/686/A43CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/474/3875 : Galaxy And Mass Assembly (GAMA): DR3 (Baldry+, 2018)J/A+A/598/A104 : LOFAR Two-metre Sky Survey (Shimwell+, 2017)J/A+A/622/A1 : LOFAR Two-metre Sky Survey DR1 source catalogJ/A+A/648/A2 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Sabater+, 2021)J/A+A/648/A3 : LOFAR Two-metre Sky Survey Deep Fields DR1J/A+A/659/A1 : LOFAR Two-metre Sky Survey (LoTSS) DR2 (Shimwell+, 2022)J/A+A/674/A119 : LoTTS Deep Fields ELAIS-N1 (Snidaric+, 2023)J/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/686/A43https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/686/A43http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/686/A43https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/686/A43https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/686/A43http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/686/A43GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/686/A43/catalog (LOFAR-eFEDS value-added catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/686/A43/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/686/A43/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/686/A43/catalog?GETtext/xml+votable180.050000true132.49657-0.566490.0055555555555555564/256 1365 1367 1706-1707 5/1028-1030 1032-1034 5457 5459 5465 6819-6820 6822-6823 6840 6842 10239 6/4124 4126 4140-4141 4144 4160-4161 4224 4226 21833 21835 21856-21857 21859 21868-21869 21969 21972-21973 21975 27183 27194 27269-27272 27274-27275 27286-27287 27336 27338-27339 27342 27364 27366 27372 40947 40949-40951 40953-40955https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/686/A43?format=asciiX-rayOpticalInfrareddefaultJ/A+A/686/A43/catalogLOFAR-eFEDS value-added cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLOFARLOFAR unique number that identifies the source (LOFAR_Source_id)meta.id;meta.mainintRAJ2000LOFAR Right ascension of the source (J2000) (for the equinox of the image) (LOFAR_RA)degpos.eq.ra;meta.mainindexedDEJ2000LOFAR Declination of the source (J2000) (for the equinox of the image) (LOFAR_DEC)degpos.eq.dec;meta.mainindexedFtotLOFAR Total, integrated Stokes I flux density of the source at the reference frequency 144MHz (LOFAR_Total_flux)Jyphot.flux.density;em.radio.100-200MHzdoublee_Ftot1{sigma} error on the total flux density of the source (LOFAR_E_Total_flux)Jystat.errordoubleFpeak? LOFAR Peak Stokes I flux density per beam of the source at 144MHz (LOFAR_Peak_flux)Jy/beamphot.flux.density;em.radio.100-200MHzdoublenullablee_Fpeak? 1{sigma} error on the peak flux density per beam of the source (LOFAR_E_Peak_flux)Jy/beamstat.errordoublenullableMajLOFAR FWHM of the major axis of the source (LOFAR_Maj)degphys.angSizedoubleeposLOFAR Positional error (LOFAR_pos_err)arcsecstat.error;posdoublescodeS[0/1] LOFAR Morphology Flag (LOFAR_scodeS_flag) (1)meta.codeintFluxratio[0/1] LOFAR Morphology Flag (LOFAR_fluxratio_flag) (2)meta.codeintf_Maj[0/1] LOFAR Morphology Flag (LOFAR_maj_flag) (3)meta.codeintIsolated[0/1] LOFAR Morphology Flag (LOFAR_isolated_flag) (4)meta.codeintCompact[0/1] LOFAR Morphology Flag (LOFAR_compact_flag) (5)meta.codeintLS9TypeLS9 Morphological model (LS9_TYPE)src.classcharRALdeg? LS9 Right ascension (J2000) (LS9_RA)degpos.eq.ranullableDELdeg? LS9 Declination (J2000) (LS9_DEC)degpos.eq.decnullableePosL? LS9 Positional error (LS9_pos_err)arcsecstat.error;posdoublenullableg0mag? LS9 De-reddened g-band magnitude (LS9_mag_g_dered)magphot.mag;em.opt.Bdoublenullabler0mag? LS9 De-reddened r-band magnitude (LS9_mag_r_dered)magphot.mag;em.opt.Rdoublenullablez0mag? LS9 De-reddened z-band magnitude (LS9_mag_z_dered)magphot.mag;em.opt.IdoublenullableW10mag? LS9 De-reddened W1-band magnitude (LS9_mag_W1_dered)magphot.mag;em.IR.3-4umdoublenullableW20mag? LS9 De-reddened W2-band magnitude (LS9_mag_W2_dered)magphot.mag;em.IR.4-8umdoublenullableW30mag? LS9 De-reddened W2-band magnitude (LS9_mag_W3_dered)magphot.flux.density;em.IR.8-15umdoublenullableRAcdeg? Right Ascension of flux-weighted centre (ICRS) (RAcen)degpos.eq.ranullableDEcdeg? Declination of flux-weighted centre (ICRS) (Deccen)degpos.eq.decnullableW40mag? LS9 De-reddened W4-band magnitude (LS9_mag_W4_dered)magphot.flux.density;em.IR.15-30umdoublenullableSep? Separation between LOFAR source and best-match LS9 counterpart (CTP_Separation)arcsecpos.angDistancedoublenullablepi[0/1]? Probability for the counterpart to be the correct one (p_i)stat.fit.goodnessdoublenullablepany[0/1]? Probability for a source to have any counterpart in the search region, optimal: pany>0.06 (p_any)stat.fit.goodnessdoublenullableGAMAID? GAMA09 Unique GAMA ID of object, (uberID)meta.idnullableCATAID? GAMA09 Unique numeric GAMA object identifier (CATAID)meta.idintnullablezsp? Spectroscopic redshift (Z)src.redshiftdoublenullableMass50? Median stellar mass from MCMC chain (StellarMass_50)solMassphys.massdoublenullableMass16? 16th percentile stellar mass from MCMC chain (StellarMass_16)solMassstat.errordoublenullableMass84? 84th percentile stellar mass from MCMC chain (StellarMass_84)solMassstat.errordoublenullableSFR50? Median SFR from MCMC chain (SFR_50)solMass/yrphys.SFRfloatnullableSFR16? 16th percentile SFR from MCMC chain (SFR_16)solMass/yrstat.errorfloatnullableSFR84? 84th percentile SFR from MCMC chain (SFR_84)solMass/yrstat.errorfloatnullableSC[6/8]? Science sample class SC>=6 is used her (SC)meta.codeintnullableRadioAGN[0/1] 1 if LOFAR source (with SNR>5, pany>0.06) fulfils radio-excess criterion (radioAGN_flag)meta.codeintvisInsp[0/1] 1 if source has been visually inspected (vis_inspected)meta.codeintG9radioAGN[0/1] Final sample of mass-complete G9 radio AGN, with visual inspection results applied (G9_radioAGN)meta.codeintFRII[0/1] 1, 0.5, 0: secure, likely, unlikely FRII-morphology, respectively (FRII_flag)meta.codefloatGRG[0/1] Giant radio galaxy flag (largest linear size >0.7Mpc (GRG_flag)meta.codeintG9RXr[0/1] 1 if the LOFAR source has an X-ray match in eROSITA eFEDS (G9_radioXray_sources)meta.codeintSpecial[0/1] 1 if source required special cross-matching and/or property estimation (special_flag)meta.codeintLS9Legacy Survey DR9 Unique source identifier, NNNNNN_NNNN (LS9_UNIQUE_OBJID)meta.idchar