J/MNRAS/478/4068ivo://CDS.VizieR/J/MNRAS/478/4068doi:10.26093/cds/vizier.74784068CDSLakicevic M.Popovic L.C.Kovacevic-Dojcinovic J.2024-08-18T20:20:05Z2021-12-10T13:53:19ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiquasarsinfrared-sourcesx-ray-sourcesvisible-astronomyinvestigated narrow-line Seyfert 1 galaxies (NLS1s) at optical, mid-infrared (MIR), and X-ray wavelengths, comparing them to the broad-line active galactic nuclei (BLAGNs). We found that black hole mass, coronal line luminosities, X-ray hardness ratio and X-ray, and optical and MIR luminosities are higher for the BLAGNs than for NLS1s, while policyclic aromatic hydrocarbon (PAH) contribution and the accretion rates are higher for NLS1s. Furthermore, we found some trends among spectral parameters that NLS1s have and BLAGNs do not have. The evolution of FWHM(H{beta}) with the luminosities of MIR and coronal lines, continuum luminosities, PAH contribution, H{beta} broad line luminosity, FWHM[OIII], and EW(H{beta}NLR) are important trends found for NLS1s. That may contribute to the insight that NLS1s are developing AGNs, growing their black holes, while their luminosities and FWHM(H{beta}) consequently grow, and that BLAGNs are mature, larger objects of slower and/or different evolution. Black hole mass is related to PAH contribution only for NLS1s, which may suggest that PAHs are more efficiently destroyed in NLS1s.2018MNRAS.478.4068Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/478/4068CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/478/4068https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/478/4068http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/478/4068https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/478/4068https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/478/4068http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/478/4068GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/478/4068/table1 (The MIR and optical data for 99 BLAGNs and 64 NLS1s)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/478/4068/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/478/4068/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/478/4068/table1?GETtext/xml+votable180.050000true20.940736-58.8057840.0055555555555555566/1277 2622 4215 4405 4506 4545 5091 5244 5367 5437 5481 5500 5576 5597 5687 5711 5971 6028 6112 6252 6391 6535 6593 7246 7277 7298 7466 7484 7777 7998 8071 8528 8597 8612 8636 8641 8881 8893 8906 8941 8943 9018-9019 9072 9194 9196 9217 9262 9643 9750 9796 10156 10162 10190-10191 10265 10269 10472 10487 10578 10653 10691 10694 10709 10927 11071 11206 11217 11354 11382 11388 11406 11504 11520 11524 11615 11668 11875 11898 11924 12380 12632 13414 17691 17727 17814 17819 18207 18601 18769 18918 19416 19433 19567 19730 19738 19741 19746 19797 19883 19932 23211 23233 23323 25403 25965 26041 26070 26096 26148 26178 26183 26260 26310 26509 26859 26902 27005 27023 27025 27191 27227 27293 27349 27580 27862 27955 28060 28083 28113 28138 28152 28164 28356 28471 28517 30021 31258 31422 31650-31651 34065 34881 36775 39118 43634 43787 43806 43877 44785 44988 48561 48865https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/478/4068?format=asciiX-rayOpticalInfrareddefaultJ/MNRAS/478/4068/table1The MIR and optical data for 99 BLAGNs and 64 NLS1sSimbadNameSimbad column added by the CDSmeta.idcharnullablezRedshiftsrc.redshiftdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSample[BLAGN NLS1] BLAGN or NLS1 samplesrc.samplecharNameSource namemeta.id;meta.maincharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainRAGN? Fractional contributions of AGN component to the integrated MIR luminosity (1)phys.luminosity;arith.rationullableRPAH? Fractional contributions of PAH component to the integrated MIR luminosity (1)phys.luminosity;arith.ratiodoublenullableRSTR? Fractional contributions of stellar component to the integrated MIR luminosity (1)phys.luminosity;arith.ratiodoublenullableSSIL? Silicate strengthspect.line.intensityfloatnullablealpha? Spectral index of the AGN componentspect.indexfloatnullableL6A? L6A parameterstat.fit.paramdoublenullableL12A? L12A parameterstat.fit.paramdoublenullableL12S? L12S parameterstat.fit.paramdoublenullablenuLnu6? Monochromatic luminosity of the source at 6um1e-07Wphys.luminosity;em.IR.4-8umdoublenullablenuLnu12? Monochromatic luminosity of the source at 12um1e-07Wphys.luminosity;em.IR.8-15umdoublenullableLDLuminosity distanceMpcpos.distancefloatFWHM(Hb)FWHM of broad H{beta} componentkm/sspect.line.widthdoubleLogL5100? logarithm of AGN luminosity at 5100{AA}, multiplied with 51001e-07Wphys.luminosity;em.optdoublenullablelogMBH? logarithm of black hole masslog(solMass)phys.massdoublenullableacr? acr parameterstat.fit.paramdoublenullableRefoptReference for the optical data (2)meta.bibcharlog(LHb)? Luminosity of H{bata} broad line (3)1e-07Wphys.luminositydoublenullableJ/MNRAS/478/4068/table2HRs and the luminosities at 0.2-12keV for 33 BLS1s and 33 NLS1srecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSample[BLAGN NLS1] BLAGN or NLS1 samplesrc.samplecharNameSource namemeta.id;meta.maincharzRedshiftsrc.redshiftfloatIAUnameIAU name (JHHMMSS.s+DDMMSS)meta.idcharHR1Hardness ratio 1 (0.2-0.5keV, 0.5-1.0keV)phot.flux;arith.ratiofloatHR2Hardness ratio 2 (0.5-1.0keV, 1.0-2.0keV)phot.flux;arith.ratiofloatHR3Hardness ratio 3 (1.0-2.0keV, 2.0-4.5keV)phot.flux;arith.ratiofloatHR4Hardness ratio 4 (2.0-4.5keV, 4.5-12.0keV)phot.flux;arith.ratiofloatL0.2-12keV0.2-12keV band luminosity1e-07Wphys.luminosity;em.X-raydoubleJ/MNRAS/478/4068/table3The luminosities of MIR lines for both NLS1 and BLAGN samplesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource namemeta.id;meta.maincharL25um? Luminosity of MIR line [OIV] at 25.89um1e-07Wphys.luminosity;em.IRdoublenullableL14um? Luminosity of MIR line [NeV] at 14.32um1e-07Wphys.luminosity;em.IRdoublenullableL15um? Luminosity of MIR line [NeIII] at 15.55um1e-07Wphys.luminosity;em.IRdoublenullable