J/MNRAS/398/1165ivo://CDS.VizieR/J/MNRAS/398/1165doi:10.26093/cds/vizier.73981165CDSGoulding A.D.Alexander D.M.2024-07-09T20:15:37Z2010-03-26T07:12:13ZCDS support team

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

cds-question@unistra.frgalaxiesactive-galactic-nucleiinfrared-astronomyspectroscopyUsing Spitzer-infrared spectrograph (IRS) spectroscopy, we investigate the ubiquity of active galactic nuclei (AGN) in a complete (~94%), volume-limited sample of the most bolometrically luminous galaxies [L_IR,8-1000um_>=(0.3-20)x10^10^L_{sun}_] to D<15Mpc. Our analyses are based on the detection of the high-excitation emission line [NeV]({lambda}14.32{mu}m) (97.1eV) to unambiguously identify AGN activity. We find that 17 of the 64 infrared (IR) bright galaxies in our sample host AGN activity (~27^+8^_6_%), >=50t of which are not identified as AGN using optical spectroscopy.2009MNRAS.398.1165Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/398/1165CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/114/2353 : AGNs and QSOs behind nearby galaxies (Crampton+, 1997)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/398/1165https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/398/1165http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/398/1165https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/398/1165https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/398/1165http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/398/1165GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/398/1165/galaxies (Catalogue of sources, derived quantities, and mid-IR spectral emission lines)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/398/1165/galaxies?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/398/1165/galaxies?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/398/1165/galaxies?GETtext/xml+votable180.050000true91.872917-61.8077780.0055555555555555566/2409 2687 3389 3506 4511 5469 5492 5572 5581 5589 5715 5751 5995 7225 7606 10475 10761 10841 10856 10905 10927 10991 11000 11027 11375 13522 15592 16655 17754-17755 18387 18398 21362 23566 25135 25772 26271 26304 27030 27512 27514 28167 28184 28496 33228 33242 34272-34273 34361 35691 36990 38273 38390 38814 38946 39201 42016 43233 43262 43339 43881 45748https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/398/1165?format=asciiInfrareddefaultJ/MNRAS/398/1165/galaxiesCatalogue of sources, derived quantities, and mid-IR spectral emission linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyCommon galaxy namemeta.id;meta.maincharRAJ2000Right ascension (J2000) (1)pos.eq.ra;meta.mainDEJ2000Declination (J2000) (1)pos.eq.dec;meta.mainDistLuminosity distance to source from the RBGS (Sanders et al., 2003, Cat. <J/AJ/126/1607>)Mpcpos.distance;pos.heliocentricfloatSH1Projected spectral aperture in short-high (4)kpcpos.distancefloatSH2Projected spectral aperture in short-high (4)kpcpos.distancefloatLH1Projected spectral aperture in long-high (4)kpcpos.distancefloatLH2Projected spectral aperture in long-high (4)kpcpos.distancefloatMTypeMorphological classification from RC3 (de Vaucouleurs et al., 1991, Cat. <VII/155>)src.morphcharlogLIRlogarithm of IR luminosity (8-1000um) from RBGS (Cat. <J/AJ/126/1607>)log(solLum)phys.luminosity;em.IRfloatClassOptical spectral class from BPT diagnostics (2)src.classcharl_Ha/HbLimit flag on Ha/Hbmeta.code.error;phys.abundcharHa/Hb? Halpha-to-Hbeta optical emission line ratiospect.dopplerVeloc.opt;em.opt;arith.ratiofloatnullablel_[OIII]/HbLimit flag on [OIII]/Hbmeta.code.errorchar[OIII]/Hb? [OIII]-to-Hbeta optical emission line ratiospect.dopplerVeloc.opt;em.line.OIII;arith.ratiofloatnullable[SII]/Ha? [SII]-to-Halpha optical emission line ratiospect.dopplerVeloc.opt;em.opt;arith.ratiofloatnullable[NII]/Ha? [NII]-to-Halpha optical emission line ratiospect.dopplerVeloc.opt;em.opt;arith.ratiofloatnullablel_F[OIII]Limit flag on F[OIII]meta.code.errorcharF[OIII]? Observed [O III] flux (10^-15^erg/cm^2^/s)aW.m**-2phot.fluxdoublenullableRef? References for published optical data (3)meta.refintnullableEWPAHEquivalent widths the 11.3um PAH featureumspect.line.eqWidthfloatF[NeII]Flux of [NeII] 12.81um, 21.6eV (6)1e-17W.m**-2phot.fluxfloate_F[NeII]? rms uncertainty on e_F[NeII] (6)1e-17W.m**-2stat.errorfloatnullablel_F[NeV]Limit flag on F[NeV] (5)meta.code.errorcharF[NeV]Flux at [NeV] 14.32um, 97.1eV (6)1e-17W.m**-2phot.fluxfloate_F[NeV]? rms uncertainty on F[NeV] (6)1e-17W.m**-2stat.errorfloatnullablel_F[NeIII]Limit flag on F[NeIII] (5)meta.code.errorcharF[NeIII]Flux at [NeIII] 15.56um, 41.0eV (6)1e-17W.m**-2phot.fluxfloate_F[NeIII]? rms uncertainty on F[NeIII] (6)1e-17W.m**-2stat.errorfloatnullablel_F[NeV]2Limit flag on F[NeV]2 (5)meta.code.errorcharF[NeV]2Flux at [NeV] 24.32um, 97.1eV (6)1e-17W.m**-2phot.fluxfloate_F[NeV]2? rms uncertainty on F[NeV]2 (6)1e-17W.m**-2stat.errorfloatnullablel_F[OIV]Limit flag on [OIV] (5)meta.code.errorcharF[OIV]Flux at [O IV] 25.89um, 54.9eV (6)1e-17W.m**-2phot.fluxfloate_F[OIV]? rms uncertainty on F[OIV] (6)1e-17W.m**-2stat.errorfloatnullablel_F[FeII]Limit flag on F[FeII] (5)meta.code.errorcharF[FeII]Flux at [Fe II] 25.99um, 7.9eV (6)1e-17W.m**-2phot.fluxfloate_F[FeII]? rms uncertainty on [FeII] (6)1e-17W.m**-2stat.errorfloatnullablel_F[SIII]Limit flag on F[SIII] (5)meta.code.errorcharF[SIII]Flux at [S III] 33.48um. 23.3eV (6)1e-17W.m**-2phot.fluxfloate_F[SIII]? rms uncertainty on F[SIII] (6)1e-17W.m**-2stat.errorfloatnullableF[SIII]2Flux at [S III] 34.82um, 8.2eV (6)1e-17W.m**-2phot.fluxfloate_F[SIII]2? rms uncertainty on F[SIII]2 (6)1e-17W.m**-2stat.errorfloatnullableIRAGN?[Y] Mid-IR AGN? on the basis of [NeV] 14.32um emissionmeta.codecharSimbadSimbad column added by the CDScharNEDSimbad column added by the CDSchar