J/MNRAS/426/2522ivo://CDS.VizieR/J/MNRAS/426/2522doi:10.26093/cds/vizier.74262522CDSPatrick A.R.Reeves J.N.Porquet D.Markowitz A.G.Braito V.,Lobban A.P.2024-07-19T20:16:35Z2013-08-28T14:36:14ZCDS support team

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

cds-question@unistra.frsurveysseyfert-galaxiesactive-galactic-nucleispectroscopyWe construct full broad-band models in an analysis of Suzaku observations of nearby Seyfert 1 active galactic nuclei (AGN) (z<=0.2) with exposures >50ks and with greater than 30000 counts in order to study their iron line profiles. This results in a sample of 46 objects and 84 observations. After a full modelling of the broad-band Suzaku and Swift-Burst Alert Telescope data (0.6-100keV), we find complex warm absorption is present in 59 per cent of the objects in this sample which has a significant bearing upon the derived FeK region parameters. Meanwhile 35 per cent of the 46 objects require some degree of high column density partial coverer in order to fully model the hard X-ray spectrum. We also find that a large number of the objects in the sample (22 per cent) require high velocity, high ionization outflows in the FeK region resulting from FeXXV and FeXXVI. A further four AGN feature highly ionized FeK absorbers consistent with zero outflow velocity, making a total of 14/46 (30%) AGN in this sample showing evidence for statistically significant absorption in the FeK region.2012MNRAS.426.2522Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/426/2522CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/207/19 : Hard X-ray survey from Swift-BAT 2004-2010 (Baumgartner+ 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/426/2522https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/426/2522http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/426/2522https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/426/2522https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/426/2522http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/426/2522GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/426/2522/table1 (The Suzaku Seyfert sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/426/2522/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/426/2522/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/426/2522/table1?GETtext/xml+votable180.050000true66.5033333-57.20011110.005555555555555556Suzaku6/1263 1405 4439 6977 7246 7642 7659 8299 8922 10912 10927 11898 12002 12025 13414 14858 15481 16184 16301 16671 17075 18524 18683 19283 19797 19883 21245 22890 23323 25907 26148 27862 28517 29398 33930 34531 34881 38268 38653 40410 43787 43806 43877 46615 47047 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/426/2522?format=asciiOpticaldefaultJ/MNRAS/426/2522/table1The Suzaku Seyfert sampleSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectSource namemeta.id;meta.maincharprimaryRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatNHGalactic H column density1e+22cm**-2phys.columnDensity;pos.galacticfloatJ/MNRAS/426/2522/table3Broad Gaussian parametrisation of FeK region in addition to the baseline modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectSource name ["Mrk 355" was corrected into into "Mrk 335" at CDS]meta.id;meta.maincharn_Object[b] Multiple observations (1)meta.notecharlineE? Line energy (2)keVphys.energy;spect.linefloatnullableE_lineE? Error on lineE (upper value)keVstat.error;stat.maxfloatnullablee_lineE? Error on lineE (lower value)keVstat.errorfloatnullablel_sigmaBLimit flag on signaBmeta.code.errorcharsigmaB? Broad line width ({sigma})keVspect.line.widthfloatnullableE_sigmaB? Error on sigmaB (upper value)keVstat.error;stat.maxfloatnullablee_sigmaB? Error on sigmaB (lower value)keVstat.errorfloatnullablel_EWBLimit flag on EWBmeta.code.errorcharEWB? Broad line equivalent widtheVspect.line.eqWidthintnullableE_EWB? Error on EWB (upper value)eVstat.error;stat.maxintnullablee_EWB? Error on EWB (lower value)eVstat.errorintnullablel_FluxLimit flag on Fluxmeta.code.error;phot.fluxcharFlux? Flux1e-05cm**-2.s**-1phot.flux;em.X-rayfloatnullableE_Flux? Error on Flux (upper value)1e-05cm**-2.s**-1stat.error;stat.maxfloatnullablee_Flux? Error on Flux (lower value)1e-05cm**-2.s**-1stat.error;phot.fluxfloatnullableDchi2? {Delta}{chi}^2^ valuestat.fit.chi2intnullableFe25[X] Flag for FeXXV emissionmeta.codecharFe26[X] Flag for FeXXVI emissionmeta.codecharJ/MNRAS/426/2522/table4Summary of RELLINE fits to objects in which some statistical improvement is made. Line energy fixed at 6.4keVrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectNamemeta.id;meta.maincharn_Object[c] Note on Object (1)meta.notecharl_EWLimit flag on EWmeta.code.error;spect.line.eqWidthcharEW? Equivalent width (lineE=6.4keV)eVspect.line.eqWidthintnullableE_EW? Error on EW (upper value)eVstat.error;stat.maxintnullablee_EW? Error on EW (lower value)eVstat.error;spect.line.eqWidthintnullablel_qLimit flag on qmeta.code.errorcharq? Average emissivity index of the accretion disk (lineE=6.4keV)phys.emissivityfloatnullableE_q? Error on q (upper value)stat.error;stat.maxfloatnullablee_q? Error on q (lower value)stat.errorfloatnullablen_q[*d ] Note on q (1)meta.notecharl_aLimit flag on ameta.code.errorchara? Black home spin parameter a (lineE=6.4keV)phys.atmolfloatnullableE_a? Error on a (upper value)stat.error;stat.maxfloatnullablee_a? Error on a (lower value)stat.errorfloatnullablel_iLimit flag on imeta.code.errorchari? Inclination of the accretion disk (lineE=6.4keV)degsrc.orbital.inclinationintnullableE_i? Error on i (upper value)degstat.error;stat.maxintnullablee_i? Error on i (lower value)degstat.errorintnullablel_FluxLimit flag on Fluxmeta.code.error;phot.fluxcharFlux? Flux, if spin is frozen at maximal (a=0.998) and the inner radius is allowed to vary away from R_ISCO_ (innermost stable circular orbit of the accretion disk)1e-05cm**-2.s**-1phot.flux;em.X-rayfloatnullableE_Flux? Error on Flux (upper value)1e-05cm**-2.s**-1stat.error;stat.maxfloatnullablee_Flux? Error on Flux (lower value)1e-05cm**-2.s**-1stat.error;phot.fluxfloatnullablel_RinLimit flag on Rinmeta.code.errorcharRin? Inner radius of emission quoted as an alternative to the spin parameter, in units of R_g_phys.atmolintnullableE_Rin? Error on Rin (upper value)stat.error;stat.maxintnullablee_Rin? Error on Rin (lower value)stat.errorintnullableFe25[X] Flag for FeXXV emissionmeta.codecharFe26[X] Flag for FeXXVI emissionmeta.codecharDchi2? {Delta}{chi}^2^ value (a negative value indicates a fit improvement)stat.fit.chi2intnullablechi2? {chi}^2^ valuestat.fit.chi2floatnullablechi2b? Second value of {chi}^2^stat.fit.chi2intnullableJ/MNRAS/426/2522/tableb1Summary of observations for the objects in the samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintObjectNamemeta.id;meta.maincharMissMission namemeta.id;obscharInstInstrument (1)meta.id;instrcharDateObservation datetime.epoch;obsnullableExp? Exposure timestime.duration;obs.exposureintnullableCRCount rate (1)ct/sphot.count;em.X-raydoublee_CRrms uncertainty on CRct/sstat.errordoubleFluxX-ray flux, in 10^-11^erg/cm^2^/s (1)1e-14W.m**-2phot.flux;em.X-rayfloatObsID? ObsIDmeta.notelongnullableNct? Number of countsctphot.count;em.X-rayintnullable