J/A+A/530/A42ivo://CDS.VizieR/J/A+A/530/A42doi:10.26093/cds/vizier.35300042CDSCorral A.Della Ceca R.Caccianiga A.Severgnini P.Brunner H.,Carrera F.J.Page M.J.Schwope A.D.2017-07-12T15:39:33Z2011-10-10T13:29:34ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleix-ray-sourcesX-ray surveys are a key instrument in the study of active galactic nuclei (AGN). Thanks to their penetrating ability, X-rays are able to map the innermost regions close to the central super massive black hole (SMBH) as well as to detect and characterize its emission up to high redshift. We present here a detailed X-ray spectral analysis of the AGN belonging to the XMM-Newton bright survey (XBS). The XBS is composed of two flux-limited samples selected in the complementary 0.5-4.5 and 4.5-7.5keV energy bands and comprising more than 300 AGN up to redshift ~2.4. We performed an X-ray analysis following two different approaches: by analyzing individually each AGN X-ray spectrum and by constructing average spectra for different AGN types.2011A&A...530A..42Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/530/A42CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/41 : XMM-Newton Serendipitous Source Catalogue 2XMMi-DR3 (XMM-SSC, 2010)J/A+A/428/383 : XMM-Newton Bright Serendipitous Survey (Della Ceca+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/530/A42https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/530/A42http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/530/A42https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/530/A42https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/530/A42http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/530/A42GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/530/A42/sample (Summary of XMM-Newton observations used and power law fit results (tables 2 and 3 of paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/530/A42/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/530/A42/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/530/A42/sample?GETtext/xml+votable180.050000true0.1154167-25.07861110.0055555555555555566/2340 2704 3934 4438 4448 4567 4750 4838 4992-4993 5091 5241 5313 5569 5687 5715 5731 5975 6027 6035 6040 6056-6057 6069 6977 7242 7310 7374 7409 7424 7426 7761 7871 7921 8066-8067 8258 8299 8339 8707 8922 8944 8952 9490 9512 10169 10255 10265 10465 10604 10938 11204 11206 11252-11253 11424 11787 11790 11856 11936 11938 12025 12111 12122 12644 16591 16755 16890 17022 17074 17221 17457 17553 17598 17683 17689-17690 17749 17752 17754 17817 17819 18184 18385 18387 18524 18590-18591 18912 19020 19022 19298 19402 19569 19797 19846 19848 19883 19978 20000 20460 21016 21245 22964 23210 24896 25084 25188 25245 25682 25906 26037 26080 26125 26292 26310 27009 27041 27136 27191 27246 27428 27860 28167 28173 28334 28356 28583 28589 28647 30021 30029 31389 31391 31504 31536 31628 31630 31669 31712 32298 32858 32961 33067 33378 33635 33713 33716 34104 34271 34443 34535 34653 34845 34975 35585 35935 35950 36005 36129 36131 36526 38268 38916 38973 43872 44094 44894 45421 45587 45590 46079 46130 46399 46484 46726 46737 46740 47017 47058 47682-47683 48262-48263 48423 48478 48610 48614 48907 48950-48951 49125https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/530/A42?format=asciiX-raydefaultJ/A+A/530/A42/sampleSummary of XMM-Newton observations used and power law fit results (tables 2 and 3 of paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintXBSSource name (JHHMMSS.s+DDMMSS)meta.id;meta.maincharn_XBS[p] low-confidence fit (1)meta.notecharTypeClassification (AGN1, AGN2 or BL Lac)src.classcharn_Type[be ] Note (1)meta.notecharzRedshiftsrc.redshiftfloatn_z[b] New optical identification (1)meta.notecharGammaPhoton index {Gamma}meta.code;spect.indexfloatn_Gamma[f] Fixed value of {Gamma} (1)meta.notecharl_NHLimit flag on NHmeta.code.errorcharNHIntrinsic column density1e+22cm**-2phys.columnDensityfloatFXObserved flux in the 2-10keV band, de-absorbed by our Galaxy (2)mW.m**-2phot.flux;em.X-rayfloatLXIntrinsic luminosity in the 2-10keV band (2)log(1e-07W)phys.luminosity;em.X-rayfloatchi2Chi^2^ valuestat.fit.chi2floatdofDegrees of freedomstat.fit.dofintProbNull hypothesis probability%statdoubleSampleSample the source belongs to (G1)src.samplecharPLWhether the simple power law is considered as our best fit (Y) or not (N) (3)meta.id;stat.fitcharSimbadSimbad column added by the CDSmeta.ref.urlcharObsIDObservation identifiermeta.id;obs.param;obscharpnFilter in use during the observation for pn camerameta.notecharMOS1Filter in use during the observation for MOS1 camerameta.notecharMOS2Filter in use during the observation for MOS2 camerameta.notecharNHXGalactic column density toward the used XMM-Newton pointing1e+20cm**-2phys.columnDensity;pos.galacticfloatExpTpn? pn resulting exposure time after removing high-background intervalskstime.duration;obs.exposurefloatnullableExpT1? MOS1 resulting exposure time after removing high-background intervalskstime.duration;obs.exposurefloatnullableExpT2? MOS2 resulting exposure time after removing high-background intervalskstime.duration;obs.exposurefloatnullableCountTotal EPIC counts (pn+MOS1+MOS2)ctphot.count;em.X-rayint_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.main