J/MNRAS/369/156ivo://CDS.VizieR/J/MNRAS/369/156doi:10.26093/cds/vizier.73690156CDSPage M.J.Loaring N.S.Dwelly T.Mason K.O.McHardy I.Gunn K.,Moss D.Sasseen T.Cordova F.Kennea J.Seymour N.2024-07-02T20:17:36Z2007-02-09T16:34:18ZCDS support team

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

cds-question@unistra.frsurveysx-ray-sourcesspectroscopyWe present the X-ray spectra of 86 optically identified sources in the 13^H^ XMM-Newton/Chandra deep field which have >70 X-ray counts. The majority of these sources have 2-10keV fluxes between 10-15 and 5x10^-14^erg/cm^2^/s. The sample consists of 50 broad-line active galactic nuclei (BLAGN), 25 narrow emission-line galaxies (NELGs), six absorption-line galaxies and five Galactic stars. The majority (42/50) of the BLAGN have X-ray spectra which are consistent with a power-law shape.2006MNRAS.369..156Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/369/156CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/362/1371 : XMM-Newton 13^H^ deep field (Loaring+, 2005)J/MNRAS/342/802 : Chandra survey of 13-h XMM/ROSAT survey (McHardy+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/369/156https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/369/156http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/369/156https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/369/156https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/369/156http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/369/156GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/369/156/table1 (Power-law fits to the XMM-Newton spectra)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/369/156/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/369/156/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/369/156/table1?GETtext/xml+votable180.050000true203.3944166737.819633330.0055555555555555566/10484https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/369/156?format=asciiX-rayOpticaldefaultJ/MNRAS/369/156/table1Power-law fits to the XMM-Newton spectra_RAPosition (as computed from Loaring et al., J/MNRAS/362/1371 (right ascension part)degpos.eq.ra;meta.main_DEPosition (as computed from Loaring et al., J/MNRAS/362/1371 (declination part)degpos.eq.dec;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTypeType of object (BLAGN, NELGs, galaxies or stars)src.classchar[LDP2005]Sequential numbermeta.recordintz? Redshiftsrc.redshiftfloatnullableGAMMAPhoton index GAMMA (1)spect.indexfloatE_GAMMAError on GAMMA (upper limit)stat.error;stat.maxfloate_GAMMAError on GAMMA (lower limit)stat.errorfloatalphaPower-law normalization at 1keV in 10^-6^ph/cm^2^/s/keV1e-06ph.cm**-2.s**-1.keV**-1stat.fit.paramfloatE_alphaError on alpha (upper limit)1e-06ph.cm**-2.s**-1.keV**-1stat.error;stat.maxfloate_alphaError on alpha (upper limit)1e-06ph.cm**-2.s**-1.keV**-1stat.error;pos.eq.rafloatchi2chi^2^ value of the fitstat.fit.chi2;stat.fit.param;meta.modelledintnuDegrees of freedom of the chi2 (nu)stat.fit.dofintl_PrLimit flag on Pmeta.code.errorcharPrNull hypothesis probability corresponding to chi^2^/nustat.fit.goodnessdouble