J/MNRAS/536/1166ivo://CDS.VizieR/J/MNRAS/536/1166doi:10.26093/cds/vizier.75361166CDSEscott E.L.Morabito L.K.Scholtz J.Hickox R.C.Harrison C.M.,Alexander D.M.Arnaudova M.I.Smith D.J.B.Duncan K.J.Petley J.,Kondapally R.Calistro Rivera G.Kolwa S.2025-08-05T20:11:24Z2025-05-30T14:39:10ZCDS support team

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

cds-question@unistra.frradio-galaxiesactive-galactic-nucleimillimeter-astronomyphotometrysubmillimeter-astronomySome Active Galactic Nuclei (AGN) host outflows which have the potential to alter the host galaxy's evolution (AGN feedback). These outflows have been linked to enhanced radio emission. Here we investigate the connection between low-frequency radio emission using the International LOFAR Telescope and [OIII] {lambda}5007 ionised gas outflows using the Sloan Digital Sky Survey. Using the LOFAR Two-metre Sky Survey (LoTSS) Deep Fields, we select 198 AGN with optical spectra, 115 of which are detected at 144 MHz, and investigate their low-frequency radio emission properties. The majority of our sample do not show a radio excess when considering radio luminosity - SFR relationship, and are therefore not driven by powerful jets. We extract the [OIII] {lambda}5007 kinematics and remove AGN luminosity dependencies by matching the radio detected and non-detected AGN in L6um and redshift. Using both spectral fitting and W80 measurements, we find radio detected AGN have a higher outflow rate (67.2+/-3.4 percent) than the radio non-detected AGN (44.6+/-2.7 percent), indicating a connection between ionised outflows and the presence of radio emission. For spectra where there are two components of the [OIII] emission line present, we normalise all spectra by the narrow component and find that the average broad component in radio detected AGN is enhanced compared to the radio non-detected AGN. This could be a sign of higher gas content, which is suggestive of a spatial relationship between [OIII] outflows and radio emission in the form of either low-powered jets or shocks from AGN winds.2025MNRAS.536.1166Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/536/1166CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/648/A3 : LOFAR Two-metre Sky Survey Deep Fields DR1 (Kondapally+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/536/1166https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/536/1166http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/536/1166https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/536/1166https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/536/1166http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/536/1166GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/536/1166/target (Target Catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/536/1166/target?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/536/1166/target?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/536/1166/target?GETtext/xml+votable180.050000true157.66507658.1032140.0055555555555555565/1517 1519 2538 6/6046-6047 6073 6075 6090-6091 6112 6114 6120 9145-9147 9150-9151 9194 10147 10150 10156 10158 10501 10512-10513 10515-10518 10521 10524 11520-11521 11524https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/536/1166?format=asciiMillimeterRadiodefaultJ/MNRAS/536/1166/targetTarget CataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSDSSUnique object identifier for SDSS, HHMMSS.ss+DDMMSS.s (SDSS_NAME)meta.id;meta.mainchare_FSWIRE2c? Recommended SWIRE ch2 (4.5um) flux error (aperture and extinction corrected from 4" aperture) (ch2_swire_fluxerr_corr)uJystat.errordoublenullableFSWIRE3c? Recommended SWIRE ch3 (5.8um) flux (aperture and extinction corrected from 4" aperture) (ch3_swire_flux_corr)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSWIRE3c? Recommended SWIRE ch3 (5.8um) flux error (aperture and extinction corrected from 4" aperture) (ch3_swire_fluxerr_corr)uJystat.errordoublenullableRAJ2000Right Ascension (J2000) for SDSS positions (RA_SDSS)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) for SDSS positions (DEC_SDSS)degpos.eq.dec;meta.mainzRedshift from SDSS (Z)src.redshiftdoublePlateUnique spectroscopic plate number (PLATE)meta.id;instr.plateintMJDJulian date of spectroscopic observation (MJD)time.epochintFiberIDFiber ID (FIBERID)meta.idintLoTSSUnique LoTSS source name (Source_Name)meta.idcharRAOdeg? Optically defined Right Ascension (J2000) (optRA)degpos.eq.ranullableDEOdeg? Optically defined Declination (J2000) (optDec)degpos.eq.decnullableRALdeg? Right Ascension defined by LoTSS (J2000) (RA_LoTSS)degpos.eq.ranullableDELdeg? Declination defined by LoTSS (J2000) (DEC_LoTSS)degpos.eq.decnullableFtot? The total, integrated Stokes I flux density of the source at the reference frequency (Total_flux)Jyphot.flux.density;em.radiodoublenullablee_Ftot? The 1-sigma on the total flux density of the source (E_Total_flux)Jystat.errordoublenullableFpeak? The peak Stokes I flux density per beam of the source (Peak_flux)Jy/beamphot.flux.density;em.opt.Idoublenullablee_Fpeak? The 1-sigma error on the peak flux density per beam of the source (E_Peak_flux)Jy/beamstat.errordoublenullableIslrms? The average background rms value of the island (Isl_rms)Jy/beaminstr.det.noisedoublenullableFSDWFS1c? Recommended SDWFS Spitzer ch1 (3.6um) flux (aperture and extinction corrected from 4" aperture) (ch1_flux_corr)uJyphot.mag;em.IR.3-4umdoublenullablee_FSDWFS1c? Recommended SDWFS Spitzer ch1 (3.6um) flux error (aperture and extinction corrected from 4" aperture) (ch1_fluxerr_corr)uJystat.errordoublenullableDetWhether a source has a detection in LoTSS (Radio) or noT (Non-Radio) (Detection)meta.codecharFSDWFS2c? Recommended SDWFS Spitzer ch2 (4.5um) flux (aperture and extinction corrected from 4" aperture) (ch2_flux_corr)uJyphot.mag;em.IR.4-8umdoublenullablee_FSDWFS2c? Recommended SDWFS Spitzer ch2 (4.5um) flux error (aperture and extinction corrected from 4" aperture) (ch2_fluxerr_corr)uJystat.errordoublenullableFSDWFS3c? Recommended SDWFS Spitzer ch3 (5.8um) flux (aperture and extinction corrected from 4" aperture) (ch3_flux_corr)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSDWFS3c? Recommended SDWFS Spitzer ch3 (5.8um) flux error (aperture and extinction corrected from 4" aperture) (ch3_fluxerr_corr)uJystat.errordoublenullableFSDWFS4c? Recommended SDWFS Spitzer ch4 (8.0um) flux (aperture and extinction corrected from 4" aperture) (ch4_flux_corr)uJyphot.flux.density;em.IR.8-15umdoublenullablee_FSDWFS4c? Recommended SDWFS Spitzer ch4 (8.0um) flux error (aperture and extinction corrected from 4" aperture) (ch4_fluxerr_corr)uJystat.errordoublenullableFieldWhich LoTSS Deep Field the source is located in (Field)meta.id;obs.fieldcharFSWIRE1c? Recommended SWIRE ch1 (3.6um) flux (aperture and extinction corrected from 4" aperture) (ch1_swire_flux_corr)uJyphot.mag;em.IR.3-4umdoublenullablee_FSWIRE1c? Recommended SWIRE ch1 (3.6um) flux error (aperture and extinction corrected from 4" aperture) (ch1_swire_fluxerr_corr)uJystat.errordoublenullableFSWIRE2c? Recommended SWIRE ch2 (4.5um) flux (aperture and extinction corrected from 4" aperture) (ch2_swire_flux_corr)uJyphot.mag;em.IR.4-8umdoublenullableFSWIRE4c? Recommended SWIRE ch4 (8.0um) flux (aperture and extinction corrected from 4" aperture) (ch4_swire_flux_corr)uJyphot.flux.density;em.IR.8-15umdoublenullablee_FSWIRE4c? Recommended SWIRE ch4 (8.0um) flux error (aperture and extinction corrected from 4" aperture (ch4_swire_fluxerr_corr)uJystat.errordoublenullableL6umSix-micron Luminosity calculated using either swire or SDWFS Spitzer (L6um)1e-07Wphys.luminositydoublee_L6umError on six-micron luminosity (L6um_err)1e-07Wstat.errordoubleLradio? 144 MHz luminosity using Total_Flux (radio_lum)1e-07Wphot.flux.density;em.radiodoublenullablee_Lradio? Error of 144 MHz luminosity (radio_lum_err)1e-07Wstat.errordoublenullableLOIIIOIII luminosity (OIII_lum)1e-07Wphys.luminositydoublee_LOIIIError of OIII luminosity (OIII_lum_err)1e-07Wstat.errordoublezbest? Source redshift (Best et al., 2023MNRAS.523.1729B) (z_best)src.redshift;pos.heliocentricdoublenullableSFRcons? Consensus star formation rates from SEDs (Best et al., 2023MNRAS.523.1729B) (SFR_cons)log(solMass.yr**-1)meta.idfloatnullableMasscons? Consensus stellar mass from SEDs (Best et al., 2023MNRAS.523.1729B) (Mass_cons)log(solMass)phys.massfloatnullableSpInteractive spectrum from SDSS-DR14meta.ref.urlcharSimbadNameSimbad column added by the CDSmeta.idcharnullable