J/MNRAS/414/3084ivo://CDS.VizieR/J/MNRAS/414/3084doi:10.26093/cds/vizier.74143084CDSBrightman M.Nandra K.2024-07-14T20:15:06Z2012-03-21T12:48:47ZCDS support team

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

cds-question@unistra.frx-ray-sourcesmillimeter-astronomysubmillimeter-astronomygalaxiesinfrared-sourcesWe present a multi-waveband analysis of a 126-galaxy sub-sample of the 12um galaxy sample (12MGS), for which we have carried out a detailed X-ray spectral analysis in a previous paper. We determine the activity class of the galaxies by way of optical-line ratio diagnostics and characterize the optical classes by their X-ray, 12um and [OIII] luminosities and X-ray spectral properties.2011MNRAS.414.3084Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/414/3084CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/413/1206 : XMM survey of 12um selected galaxies (Brightman+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/414/3084https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/414/3084http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/414/3084https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/414/3084https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/414/3084http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/414/3084GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/414/3084/sample (Optical line ratio data compiled from the literature, nuclear activity classification, and multi-wavelength data for our sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/414/3084/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/414/3084/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/414/3084/sample?GETtext/xml+votable180.050000true1.581591720.20293890.0055555555555555566/700 2251 2564 4314 4439 4488 5202 5469 5975 6034 6098 6977 7214 7241 7424 7550 7552 7606 7642 7659 7777 7921 8085 8225 8845 8922 9895 10210 10265 10761 10817 10841 10905 10911-10912 10927 11027 11029 11101 11206 12060 16042 16479 17061 17183 17529 17748 17754 18212 18387 18683 18809 19283 19619 19730 19883 19954 20000 20060-20061 20489 21016 22632 22654 22721 23171 23323 24896 25083 25344 25603 25610 25907 26148 26175 26292 27704 27767 27861 27914 27937 27945 28035 28123 28167 28496 28517 28529 28631 31158 31259 33193 33920 34273 34294 34471 34493 34531 34534 35447 35623 36194 36668 36785 36861 40410 43806 43874 43877 43881 44448 45587 45816 45914 46079 46130 46399 46615 46890 46987 47047 47078 47415 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/414/3084?format=asciiX-rayInfraredRadiodefaultJ/MNRAS/414/3084/sampleOptical line ratio data compiled from the literature, nuclear activity classification, and multi-wavelength data for our samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy namemeta.id;meta.mainchar[OIII]/Hb? Emission-line flux ratio [OIII]/H{beta}phot.flux;em.line.OIII;arith.ratiofloatnullable[OI]/Ha? Emission-line flux ratio [OI]/H{alpha}spect.line.intensity;arith.ratiofloatnullable[NII]/Ha? Emission-line flux ratio [NII]/H{alpha}phot.flux;arith.ratiofloatnullable[SII]/Ha? Emission-line flux ratio [SII]/H{alpha}phot.flux;arith.ratiofloatnullableFobs? Observed flux of the [OIII]{lambda}5007 line (in 10^-16^erg/s/cm2)1e-19W.m**-2phot.flux;em.line.OIII;spect.lineintnullableHa/Hb? Balmer decrement H{alpha}/H{beta}phot.flux;arith.ratiofloatnullableFcor? Flux of the [OIII] line corrected for absorption using the Balmer decrement1e-19W.m**-2phot.flux;em.line.OIII;spect.lineintnullableRefReference for the line ratio data (1)meta.ref;pos.framecharClass1Activity classification based on diagram 1src.classcharClass2Activity classification based on diagram 2src.classcharClass3Activity classification based on diagram 3src.classcharClassAdopted activity classificationsrc.classcharBLR[HIB] Broad-line region information taken from Veron-Cetty & Veron (2006, Cat. VII/248) (2)src.classcharlogLXObserved 2-10keV luminositylog(1e-07W)phys.luminosity;em.X-rayfloatlogL1212um luminositylog(1e-07W)phys.luminosity;em.IR.8-15umfloatlogL[O3]? Absorption-corrected [OIII] luminositylog(1e-07W)phys.luminosityfloatnullablelogNHMeasured hydrogen column densitylog(cm**-2)phys.columnDensityfloatlogT? T=F(2-10keV)/F([OIII]) where F(2-10keV) is the observed X-ray flux, and F([OIII]) the absorption-corrected [OIII] fluxphot.flux;arith.ratiofloatnullableSimbadDetails from the SIMBAD databasemeta.ref.urlcharNEDSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainSimbadNameSimbad column added by the CDSmeta.idchar