J/MNRAS/509/831ivo://CDS.VizieR/J/MNRAS/509/831doi:10.26093/cds/vizier.75090831CDSLakicevic M.Kovacevic-Dojcinovic J.Popovic L.C.2025-02-12T20:12:09Z2024-10-23T09:33:33ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleispectroscopyvisible-astronomyh-beta-photometryinfrared-sourcesThe differences between Narrow Line Seyfert 1 galaxies (NLS1s) and Broad Line AGNs (BLAGNs) are not completely understood; it is thought that they may have different inclinations and/or physical characteristics. The FWHM(H{beta})-luminosities correlations are found for NLS1s and their origin is the matter of debate. Here we investigated the spectroscopic parameters and their correlations considering a dusty, cone model of AGN. We apply a simple conical dust distribution (spreading out of broad line region, BLR), assuming that the observed surface of the model is in a good correlation with MIR emission. The dusty cone model in combination with a BLR provides the possibility to estimate luminosity dependence on the cone inclination. The FWHM(H{beta})-luminosities correlations obtained from model in comparison with observational data show similarities which may indicate the influence of AGN inclination and structure to this correlation. An alternative explanation for FWHM(H{beta})-luminosities correlations is the selection effect by the black hole mass. These FWHM(H{beta})-luminosities correlations may be related to the starburst in AGNs, as well. The distinction between spectral properties of the NLS1s and BLAGNs could be caused by multiple effects: beside physical differences between NLS1s and BLAGNs (NLS1s have lighter black hole mass than BLAGNs), inclination of the conical AGN geometry may have important role as well, where NLS1s may be seen in lower inclination angles.2022MNRAS.509..831Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/509/831CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/509/831https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/509/831http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/509/831https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/509/831https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/509/831http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/509/831GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/509/831/tablea1 (Name of object, coordinates, and redshifts, FWHM(H{beta}) and equivalent width of PAH at 7.7um)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/509/831/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/509/831/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/509/831/tablea1?GETtext/xml+votable180.050000true1.5813388920.202913890.0055555555555555566/1277 4215 4439 4488 5091 5367 5500 6028 6977 7246 7642 7921 8299 8922 9194 9750 10039 10265 10321 10912 10927 11206 11354 11490 11668 11898 13414 16301 16671 17727 18683 19283 19433 19567 19730 19767 19797 19883 22890 23233 23323 25054 26148 26292 26310 26859 27191 27293 27862 28517 30021 34881 36775 38268 43877 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/509/831?format=asciiOpticalInfrareddefaultJ/MNRAS/509/831/tablea1Name of object, coordinates, and redshifts, FWHM(H{beta}) and equivalent width of PAH at 7.7umrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of objectmeta.id;meta.maincharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatFWHMHbH{beta} FWHMkm/sphys.angSizeintr_FWHMHbReference for FWHMHb (G1)meta.ref;pos.framechardFWHMHbH{beta} FWHM dispersionkm/sinstr.dispersion;spect.linefloatr_dFWHMHbReference for dFWHMHb (G1)meta.ref;pos.framecharEW7.7? Equivalent width of PAH at 7.7umnmspect.line.eqWidth;em.IR.4-8umfloatnullablee_EW7.7? Equivalent width of PAH at 7.7um errornmstat.errordoublenullableSimbadNameSimbad column added by the CDSmeta.idcharnullableJ/MNRAS/509/831/tablea2Name of object, PAH fraction, L6, L12 and log(MBH)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of objectmeta.id;meta.maincharRPAHPAH fractionphys.mass;arith.ratiodoublee_RPAHPAH fraction errorstat.errordoublenuLnu6? Luminosity at 6um1e-07Wphys.luminosity;em.IRdoublenullablee_nuLnu6? Luminosity at 6um error1e-07Wstat.errordoublenullablenuLnu12Luminosity at 12um1e-07Wphys.luminosity;em.IR.8-15umdoublee_nuLnu12Luminosity at 12um error1e-07Wstat.errordoublelog(MBH)Black hole masslog(solMass)phys.massfloate_log(MBH)Black hole mass errorlog(solMass)stat.errordoubler_log(MBH)Reference for log(MBH) (G1)meta.ref;pos.framecharJ/MNRAS/509/831/tablea3Name of object, RBLR, {delta}RBLR, calculated inclination and luminosity at the peak of the 7.7um featurer_TypeReference for Typemeta.notecharlog(nuL7.7)? Luminosity at the peak of the 7.7um featurelog(1e-07W)phys.luminosity;em.IRdoublenullablee_log(nuL7.7)? Luminosity at the peak of the 7.7um feature errorlog(1e-07W)stat.errordoublenullableNameName of objectmeta.id;meta.maincharr_RblrReference for Rblr (G1)meta.ref;pos.framecharr_dRblrReference for dRblr (G1)meta.ref;pos.framecharTypeTypesrc.classchariInclinationdegsrc.orbital.inclinationdoublee_iInclination errordegstat.errordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRblrBLR radius (in day light unit)phys.size.radiusfloatdRblrBLR radius error (in day light unit)stat.errorfloat