J/ApJ/763/111ivo://CDS.VizieR/J/ApJ/763/111doi:10.26093/cds/vizier.17630111CDSVasudevan R.V.Brandt W.N.Mushotzky R.F.Winter L.M.Baumgartner W.H.,Shimizu T.T.Schneider D.P.Nousek J.2017-11-10T11:16:12Z2014-11-05T08:46:50ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleix-ray-sourcessurveysredshiftedWe present a detailed X-ray spectral analysis of the non-beamed, hard X-ray selected active galactic nuclei (AGNs) in the northern Galactic cap of the 58 month Swift Burst Alert Telescope (Swift/BAT) catalog, consisting of 100 AGNs with b>50{deg}. This sky area has excellent potential for further dedicated study due to a wide range of multi-wavelength data that are already available, and we propose it as a low-redshift analog to the "deep field" observations of AGNs at higher redshifts (e.g., CDFN/S, COSMOS, Lockman Hole). We present distributions of luminosity, absorbing column density, and other key quantities for the catalog. We use a consistent approach to fit new and archival X-ray data gathered from XMM-Newton, Swift/XRT, ASCA, and Swift/BAT. We probe to deeper redshifts than the 9 month BAT catalog (<z>=0.043 compared to <z>=0.03 for the 9 month catalog), and uncover a broader absorbing column density distribution. The fraction of obscured (logN_H_>=22) objects in the sample is ~60%, and 43%-56% of the sample exhibits "complex" 0.4-10keV spectra. We present the average 1-10keV spectrum for the sample, which reproduces the 1-10keV X-ray background slope as found for the brighter 9 month BAT AGN sample.2013ApJ...763..111Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/763/111CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012)VI/117 : Observation Log from ASCA (PLAIN Center, 2001)J/ApJS/207/19 : Swift-BAT 2004-2010 hard X-ray survey (Baumgartner+, 2013)J/ApJ/754/45 : IR properties of Swift/BAT X-ray AGNs (Ichikawa+, 2012)J/ApJ/753/104 : AGN identifications from AKARI and Swift (Matsuta+, 2012)J/ApJ/749/21 : AGNs detected by 60 month Swift/BAT survey (Ajello+, 2012)J/A+A/530/A42 : X-ray properties of AGNs in XBS (Corral+, 2011)J/A+A/529/A135 : AGN Opt/IR properties in Lockman Hole (Rovilos+, 2011)J/ApJ/739/57 : Ultra hard X-ray AGNs in the Swift/BAT survey (Koss+, 2011)J/ApJ/728/58 : Swift-BAT survey of AGNs (Burlon+, 2011)J/MNRAS/413/1206 : XMM survey of 12um selected galaxies (Brightman+, 2011)J/ApJS/186/378 : Hard X-ray survey from Swift-BAT 2004-2006 (Tueller+, 2010)J/A+A/510/A48 : Palermo Swift-BAT Hard X-ray Catalogue (Cusumano+, 2010)J/A+A/505/417 : Second INTEGRAL AGN catalogue (Beckmann+, 2009)J/ApJ/699/603 : Evolution of Swift/BAT blazars (Ajello+, 2009)J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008)J/ApJ/678/102 : BAT X-ray survey. I. (Ajello+, 2008)J/ApJ/633/L77 : SWIFT/BAT detections of AGN (Markwardt+, 2005)J/AJ/126/2237 : Radio-excess IR galaxies PMN/FSC sample (Drake+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/763/111https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/763/111http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/763/111https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/763/111https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/763/111http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/763/111GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/763/111/table1 (Table of observations used for each object)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/763/111/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/763/111/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/763/111/table1?GETtext/xml+votable180.050000true150.45728.7850.0055555555555555566/4439 5149 5284 5423 5514 5576 5970 5975 5989 5996 6014 6097 6113 8216 8299 8426 8812 8845 8868 8870 8921 8922 9005 9894 10348 10454 10475 10538 10630 10662 10707 10788 10847 10912 10925 10927 10977 10984 10991 11006 11071 11158 11191 11232 11392 11408 11416 11490 25553 25572 25580 25585 25735 25742 25773 25790 25907 25965 26041 26071 26148 26300 26375 26393 26493 26509 26515 26547 27477 27486 27501 27504 27699 27721 27722 27767 27795 27803 27815 27914 27976 28060 28075 28259 28275 28278 28350 28471 28517 28518 28535 28563 28593 28609 28626 28639 28654https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/763/111?format=asciiX-rayOpticaldefaultJ/ApJ/763/111/table1Table of observations used for each objectSimbadNameSimbad column added by the CDSmeta.idcharNameAGN namemeta.id;meta.maincharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFitNumber of different fits for this AGNmeta.ref.urlintnullablen_Name[n] n: new observationmeta.notecharz[0.001/0.2] AGN redshiftsrc.redshiftfloatRAJ2000Right ascension in decimal degrees (J2000) (1)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000) (1)degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLAT[50.2/82.3] Galactic latitudedegpos.galactic.latfloatInstInstrument (ASCA, XMM, XRT)meta.id;instrcharObsIDObservation identification numbermeta.idlongDateObservation date (UT)time.epoch;obsnullableCts[3/1875711] Total number of counts in the source region at energies 0.4-10keV (2)ctphot.count;em.X-rayintTime[0.3/96] Observation timekstime.epochfloatf_Time[*] *: pile-up correction (3)meta.codecharUse[0/100]? Usable % of obs. (4)%stat.fit.paramintnullableTypeOptical typesrc.classcharFgam[4.3/533.1] BAT flux (14-195keV), in units of 10^-12^erg/s/cm^2^fW.m**-2phot.flux.density;em.gamma.hardfloatSNR[4.8/275] Signal-to-noise ratio of the BAT detectionstat.snrfloatSwiftCross-match within 2.5' with Ajellos et al. 2012 (J/ApJ/749/21) and Baumgartner et al. 2013 (J/ApJS/207/19)meta.ref.urlintnullableNEDSimbad column added by the CDSmeta.ref.urlcharJ/ApJ/763/111/table3Basic fit results for 95 AGNsl_RLLimit flag on RLmeta.code.errorcharl_NHLimit flag on NHmeta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAGN namemeta.id;meta.maincharModelBest fitting model (1)stat.param;meta.modelledcharchi2[3.2/11118] Model {chi}^2^stat.param;meta.modelleddoubledof[5/2780] Number of degrees of freedommeta.numberintProb[0/1] null-hypothesis probabilitystat.probabilityfloatNHg[0.6/4.1] Galactic neutral hydrogen column density1e+20cm**-2phys.columnDensityfloatNH[19.9/25.4]? Intrinsic column density (N_H_) (2)1e+20cm**-2phys.columnDensityfloatnullableE_NH[0/1]? Positive uncertainty on NH1e+20cm**-2stat.error;stat.maxfloatnullablee_NH[0/2]? Negative uncertainty on NH1e+20cm**-2stat.errorfloatnullableCF[0.1/1]? Covering fraction if partial-covering model is usedstatfloatnullablef_CF[*] *: the covering fraction was poorly constrainedmeta.codecharE_CF[0/0.9]? Positive error on CF (3)stat.error;stat.maxfloatnullablee_CF[0/1]? Negative error on CF (3)stat.errorfloatnullableGamma[1.5/2.2] Photon index {Gamma} (4)meta.code;spect.indexfloatf_Gamma[*] *: {Gamma} was frozen in the fitmeta.codecharE_Gamma[0/0.7]? Positive uncertainty on Gammastat.error;stat.maxfloatnullablee_Gamma[0/1.8]? Negative uncertainty on Gammastat.errorfloatnullableF0.5-2[0/256.5] 0.5-2keV flux in units of 10^-13^erg/s/cm^2^1e-16W.m**-2phot.flux;em.X-rayfloatF2-10[5/668.5] 2-10keV flux in units of 10^-13^erg/s/cm^2^1e-16W.m**-2phot.flux;em.X-rayfloatL0.5-2[39.9/44.7] Absorption-corrected 0.5-2keV luminosity (log erg/s)log(1e-07W)phys.luminosity;em.X-rayfloatL2-10[40.3/44.7] Absorption-corrected 2-10keV luminosity (log erg/s)log(1e-07W)phys.luminosity;em.X-rayfloatE_L2-10[0/0.9] Positive uncertainty on L2-10log(1e-07W)stat.error;stat.maxfloate_L2-10[0/44.44] Negative uncertainty on L2-10log(1e-07W)stat.errorfloatLgam[40.8/45]? Swift/BAT 14-195keV luminositylog(1e-07W)phot.flux.density;em.gamma.hardfloatnullableLgam2? Second value of 14-195keV luminositylog(1e-07W)phot.flux.density;em.gamma.hardfloatnullablef_Lgam2[d] Unexplained {dagger} flag on Lgammeta.codecharRL[-6/-2.5] Logarithm of radio-loudness (5)phys.luminosity;arith.ratiofloat