J/ApJ/850/74ivo://CDS.VizieR/J/ApJ/850/74doi:10.26093/cds/vizier.18500074CDSKoss M.Trakhtenbrot B.Ricci C.Lamperti I.Oh K.Berney S.,Schawinski K.Balokovic M.Baronchelli L.Crenshaw D.M.Fischer T.,Gehrels N.Harrison F.Hashimoto Y.Hogg D.Ichikawa K.Masetti N.,Mushotzky R.Sartori L.Stern D.Treister E.Ueda Y.Veilleux S.,Winter L.2018-05-16T06:56:14Z2018-02-27T14:25:35ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleivisible-astronomyspectroscopygamma-ray-astronomyredshiftedgalaxy-kinematicsline-intensitiesWe present the first catalog and data release of the Swift-BAT AGN Spectroscopic Survey. We analyze optical spectra of the majority of the detected AGNs (77%, 642/836) based on their 14-195keV emission in the 70-month Swift-BAT all-sky catalog. This includes redshift determination, absorption and emission-line measurements, and black hole mass and accretion rate estimates for the majority of obscured and unobscured AGNs (74%, 473/642), with 340 measured for the first time. With ~90% of sources at z<0.2, the survey represents a significant advance in the census of hard X-ray-selected AGNs in the local universe. In this first catalog paper, we describe the spectroscopic observations and data sets, and our initial spectral analysis. The FWHMs of the emission lines show broad agreement with the X-ray obscuration (~94%), such that Sy 1-1.8 have N_H_<10^21.9^cm^-2^, and Seyfert 2 have N_H_>10^21.9^cm^-2^. Seyfert 1.9, however, show a range of column densities. Compared to narrow-line AGNs in the SDSS, the X-ray-selected AGNs have a larger fraction of dusty host galaxies (H{alpha}/H{beta}>5), suggesting that these types of AGN are missed in optical surveys. Using the [OIII]{lambda}5007/H{beta} and [NII]{lambda}6583/H{alpha} emission-line diagnostic, about half of the sources are classified as Seyferts; ~15% reside in dusty galaxies that lack an H{beta} detection, but for which the upper limits on line emission imply either a Seyfert or LINER, ~15% are in galaxies with weak or no emission lines despite high-quality spectra, and a few percent each are LINERS, composite galaxies, H II regions, or in known beamed AGNs.2017ApJ...850...74Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/850/74CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)J/ApJS/129/547 : RBSC-NVSS sample. I. (Bauer+, 2000)J/ApJS/132/37 : Spectroscopy of Southern warm IR galaxies (Kewley+, 2001)J/ApJS/145/199 : Opt. spec. atlas of low-redshift AGN (Marziani+, 2003)J/A+A/424/519 : Naked active galactic nuclei (Hawkins+, 2004)J/ApJ/633/L77 : SWIFT/BAT detections of AGN (Markwardt+, 2005)J/ApJ/667/131 : Mass function of active black holes (Greene+, 2007)J/ApJS/183/1 : Cat. of central stellar velocity dispersions (Ho+, 2009)J/A+A/495/691 : Multifreq. catalog of blazars, Roma-BZCAT (Massaro+, 2009)J/ApJ/727/20 : The Megamaser Cosmology Project (MCP). III. (Kuo+, 2011)J/MNRAS/417/2651 : AT20G-optical catalogue (Mahony+, 2011)J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)J/ApJ/733/60 : Accretion rate of AGNs from COSMOS surveys (Trump+, 2011)J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011)J/ApJ/746/L22 : Dual AGNs in the nearby Universe (Koss+, 2012)J/A+A/545/A101 : Spectra of Swift/BAT optical counterparts (Parisi+, 2012)J/MNRAS/421/1043 : Emission-line galaxies from SDSS DR7 (Shirazi+, 2012)J/other/RMxAA/48.9 : Optical spectrosc. atlas of MOJAVE AGNs (Torrealba+, 2012)J/ApJS/207/19 : X-ray survey from Swift-BAT 70mth (Baumgartner+, 2013)J/A+A/561/A67 : Spectra of Swift/BAT optical counterparts (Parisi, 2014)J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)J/ApJ/815/L13 : Compton-thick AGNs from 70-mth Swift/BAT (Ricci+, 2015)J/ApJS/218/10 : HET Massive Galaxy Survey (HETMGS) (van den Bosch+, 2015)J/MNRAS/460/19 : Update of INTEGRAL/IBIS AGN catalogue (Malizia+, 2016)J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)J/ApJ/817/172 : X-ray Observations of Stripe 82 (LaMassa+, 2016)http://swift.gsfc.nasa.gov/results/bs70mon/ : Swift BAT 70-month hard X-rayhttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/850/74https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/850/74http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/850/74https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/850/74https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/850/74http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/850/74GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/850/74/agns (Optical spectra, stellar velocity dispersion measurements, and strong emission line classification (tables 2, 4, 8))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/850/74/agns?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/850/74/agns?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/850/74/agns?GETtext/xml+votable180.050000true0.261-7.1230.0055555555555555566/43 815 941 953 1093 1120 1121 1263 1358 1405 1526 1546 1566 1583 1701 1702 1841 2004 2153 2206 2221 2251 2464 2512 2531 2549 2551 2564 2846 3056 3103 3105 3219 3222 3309 3502 3762 3771 3886 4114 4215 4231 4329 4369 4439 4488 4535 4540 4558 4589 4784 4834 5018 5099 5149 5284 5395 5423 5463 5514 5597 5762 5964 5972 5975 5976 5989 5996 6014 6021 6097 6113 6167 6212 6241 6376 6458 6466 6502 6583 6665 6752 6923 6928 6977 7157 7166 7177 7184 7246 7277 7361 7386 7422 7424 7502 7518 7552 7560 7606 7628 7642 7660 7713 7728 7741 7869 7921 7952 7959 7969 8029 8030 8071 8085 8216 8299 8426 8641 8658 8670 8812 8845 8870 8921 8922 8945 9005 9093 9231 9375 9468 9490 9502 9612 9633 9707 9821 9894 9942 10118 10348 10454 10475 10538 10605 10630 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49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/850/74?format=asciiOpticalGamma-raydefaultJ/ApJ/850/74/agnsOptical spectra, stellar velocity dispersion measurements, and strong emission line classification (tables 2, 4, 8)SWIFTSwift/BAT identifiermeta.idcharSimbadNameSimbad column added by the CDSmeta.idcharRefReference(s) (4)meta.ref;pos.framecharExp[60/27097] Exposure timestime.duration;obs.exposureintSlit[0/276]? Slit widthkpcspect.line.widthfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/1209] Swift-BAT 70-month hard X-ray survey ID (G1)meta.id;meta.mainintprimaryCNameCounterpart source namemeta.idcharSourceSource of optical spectrum (G2)meta.id;obscharz[OIII][-0/3.3] Redshift measured from [OIII]5007src.redshift;pos.heliocentricfloatDist[3.6/28370]? DistanceMpcpos.distance;pos.heliocentricdoublenullablelogLx[40.4/48.7]? Log Swift-BAT 14-195keV X-ray luminositylog(1e-07W)phys.luminosity;em.X-rayfloatnullablelogLbol[41.3/49.6]? Log 14-195keV bolometric luminosity (1)log(1e-07W)phys.luminosityfloatnullableDateDate(s) taken optical spectra; dd/mm/yyyytime.epochcharType[1/2]? AGN classification following Osterbrock 1981ApJ...249..462Osrc.classfloatnullableBeamBeamed AGN identifier (1 = beamed AGN)meta.codeintnHObscuration identifier (2)meta.noteBDisplay the properties derived from spectral decomposition of broad Hbeta and broad Halpha sources (table 9)meta.ref.urlcharhighzDisplay the properties derived from spectral decomposition for this high redshift source (table 10)meta.ref.urlintnullableEmLDisplay the emission line measurements for this source (tables 5-7)meta.ref.urlcharSource2Source of optical spectrum (G2)meta.id;obscharz[0.001/1.3]? Redshift measured from stellar templatesrc.redshiftdoublenullablesigma[85/577]? Stellar velocity dispersionkm/sphys.veloc.dispersionintnullablee_sigma? Formal uncertainty in sigmakm/sstat.errorintnullablelogMbh[6.9/10]? Log of the Black Hole masslog(solMass)phys.massfloatnullablee_logMbh? Formal uncertainty in logMbhlog(solMass)stat.errorfloatnullablef_sigma[1/9] Fitting quality flag on sigma (3)meta.codeintCaHK[1]? 1= line is fittedmeta.codeintnullableMgb[1]? 1= line is fittedmeta.codeintnullablesigmaCaT[68/205]? Stellar velocity dispersion measured from CaTkm/sphys.veloc.dispersionintnullablee_sigmaCaT? Formal uncertainty in sigmaCaTkm/sstat.errorintnullablef_sigmaCaT[1/9]? Fitting quality flag for sigmaCaT (3)meta.codeintnullablesigmalit[30/462]? Literature stellar velocity dispersionkm/sphys.veloc.dispersionintnullablee_sigmalit? Formal uncertainty in sigmalitkm/sstat.errorintnullablelogMbhlit[6.3/9.5]? Log literature Black Hole masslog(solMass)phys.massfloatnullablee_logMbhlit? Lower formal uncertainty in logMbhlitlog(solMass)stat.errorfloatnullableE_logMbhlit? Upper format uncertainty in logMbhlitlog(solMass)stat.error;stat.maxfloatnullablef_CName(B): broad-line sourcemeta.codecharN2/O3The [NII]/Halpha vs. [OIII]/Hbeta diagnostic classification (5)phot.flux;arith.ratiocharS2/O3The [SII]/Halpha vs. [OIII]/Hbeta diagnostic classification (5)phot.flux;arith.ratiocharO1/O3The [OI]/Halpha vs. [OIII]/Hbeta diagnostic classification (5)phot.flux;arith.ratiocharHe2/N2The [HeII]/Hbeta vs. [NII]/Halpha diagnostic classification (5)phot.flux;arith.ratiocharO3/O1The [OIII]/[OII] vs. [OI]/Halpha diagnostic classification (5)phot.flux;arith.ratiocharPapVDisplay the x-ray data from Paper V (Ricci+, 2017, J/ApJS/233/17)phot.flux;arith.ratiocharNEDNED column added by the CDSmeta.ref.urlchar_RAPositions from the Swift-BAT 70 month catalog (Baumgartner+, 2013, J/ApJS/207/19) (right ascension part)degpos.eq.ra;meta.main_DEPositions from the Swift-BAT 70 month catalog (Baumgartner+, 2013, J/ApJS/207/19) (declination part)degpos.eq.dec;meta.mainJ/ApJ/850/74/emlinesEmission line measurements: [OII]3727 spectral region, narrow Hbeta spectral region and narrow Halpha spectral region (tables 5-7)FitHaSpectral fitting quality flag (G4)meta.code.qualcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/1209] Swift-BAT 70-month hard X-ray survey ID (G1)meta.id;meta.mainintFWHMO2[205/4134]? Full-width at half-maximum measured from the [OII]3727{AA} linekm/sspect.line.widthintnullablee_FWHMO2? Formal uncertainty of FWHMO2km/sstat.errorintnullablel_F[NeV]3346The 3{sigma} limit flag on F[NeV]3346meta.code.errorcharF[NeV]3346? Flux of [NeV]3346{AA} line (G3)1e-15W.m**-2phot.flux;spect.linedoublenullablee_F[NeV]3346[0/]? Formal uncertainty of F[NeV]33461e-15W.m**-2stat.errordoublenullablel_F[NeV]3426The 3{sigma} limit flag on F[NeV]3426meta.code.errorcharF[NeV]3426? Flux of [NeV]3426{AA} line (G3)1e-15W.m**-2phot.flux;spect.linedoublenullablee_F[NeV]3426[0/2]? Formal uncertainty of F[NeV]34261e-15W.m**-2stat.errorfloatnullablel_F[OII]3727The 3{sigma} limit flag on F[OII]3727meta.code.errorcharF[OII]3727[0/3332]? Flux of [OII]3727{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[OII]3727[0/]? Formal uncertainty of F[OII]37271e-15W.m**-2stat.errordoublenullablel_F[NeIII]3869The 3{sigma} limit flag on F[NeIII]3869meta.code.errorcharF[NeIII]3869[0/26999]? Flux of [NeIII]3869{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[NeIII]3869[0/11472]? Formal uncertainty of F[NeIII]38691e-15W.m**-2stat.errorfloatnullablel_F[NeIII]3968The 3{sigma} limit flag F[NeIII]3968meta.code.errorcharF[NeIII]3968[0/15343]? Flux of [NeIII]3968{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[NeIII]3968? Formal uncertainty of F[NeIII]39681e-15W.m**-2stat.errordoublenullableFitO2Spectral fitting quality flag (G4)meta.code.qualcharFWHMHb[180/1781]? Full-width at half-maximum measured from narrow Hbetakm/sspect.line.widthintnullablee_FWHMHb[0/3866]? Formal uncertainty of FWHMHbkm/sstat.errorintnullablel_FHeII4686The 3{sigma} limit flag on l_FHeII4686meta.code.errorcharFHeII4686[0.1/1953]? Flux of HeII4686{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_FHeII4686[0/47]? Formal uncertainty of FHeII46861e-15W.m**-2stat.errorfloatnullablel_FHbThe 3{sigma} limit flag on FHbmeta.code.errorcharFHb[0/3409]? Flux of H{beta} line (G3)1e-15W.m**-2phot.flux;em.line.Hbetafloatnullablee_FHb[0/309]? Formal uncertainty of FHb1e-15W.m**-2stat.errorfloatnullablef_FHbHbeta flag (G5)meta.codecharF[OIII]5007[0.3/41159]? Flux of [OIII]5007{AA} line (G3)1e-15W.m**-2phot.flux;em.line.OIII;spect.linefloatnullablee_F[OIII]5007[0/180]? Formal uncertainty of F[OIII]50071e-15W.m**-2stat.errorfloatnullableFitHbSpectral fitting quality flag (G4)meta.code.qualcharFWHMHa[152/1436]? Full-width at half-maximum measured from narrow Halphakm/sspect.line.widthintnullablee_FWHMHa[0/426]? Formal uncertainty of FWHMHakm/sstat.errorintnullablel_F[OI]6300The 3{sigma} limit flag on F[OI]6300meta.code.errorcharF[OI]6300[0.1/882]? Flux of [OI]6300{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[OI]6300[0/24]? Formal uncertainty of F[OI]63001e-15W.m**-2stat.errorfloatnullablel_FHaThe 3{sigma} limit flag on FHameta.code.errorcharFHa[0/6498]? Flux of H{alpha} (G3)1e-15W.m**-2phot.flux;em.line.Halphafloatnullablee_FHa[0/45]? Formal uncertainty of FHa1e-15W.m**-2stat.errorfloatnullablef_FHaHalpha flag (G5)meta.codecharl_F[NII]6583The 3{sigma} limit flag on F[NII]6583meta.code.errorcharF[NII]6583[0/11935]? Flux of [NII]6583{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[NII]6583[0/39]? Formal uncertainty of F[NII]65831e-15W.m**-2stat.errorfloatnullablel_F[SII]6716The 3{sigma} limit flag on F[SII]6716meta.code.errorcharF[SII]6716[0/1149]? Flux of [SII]6716{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[SII]6716[0/22]? Formal uncertainty of F[SII]67161e-15W.m**-2stat.errorfloatnullablel_F[SII]6731The 3{sigma} limit flag on F[SII]6731meta.code.errorcharF[SII]6731[0/1594]? Flux of [SII]6731{AA} line (G3)1e-15W.m**-2phot.flux;spect.linefloatnullablee_F[SII]6731[0/28]? Formal uncertainty of F[SII]67311e-15W.m**-2stat.errorfloatnullableJ/ApJ/850/74/table9Properties derived from spectral decomposition of broad Hbeta and broad Halpha sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/1206] Swift-BAT 70-month hard X-ray survey ID (G1)meta.id;meta.mainintlogL5100[41.6/46.1]? Log monochromatic luminosity (1)log(1e-07W)phys.luminosity;em.optfloatnullablelogLbol[42.8/46.8]? Log bolometric luminosity (2)log(1e-07W)phys.luminosityfloatnullableFWHMbHb[1222/14999]? Full-width at half-maximum of broad Hbetakm/sspect.line.widthintnullableEWbHb[5/204]? Equivalent width of broad Hbeta0.1nmspect.line.eqWidth;em.line.HbetafloatnullablelogMbhTN12[5.3/9.6]? Log black hole mass with logLbol (2)log(solMass)phys.massfloatnullablelogEddTN12[-2.7/0.04]? Log Eddington ratio with logLbol (2)phys.luminosity;arith.ratiofloatnullablebHb? Fitting quality flag for broad Hbeta (G6)meta.code.qual;stat.fitintnullableFbHa[7.9/12449]? Flux of broad Halpha (G3)1e-15W.m**-2phot.fluxfloatnullablee_FbHa[0/123]? Formal uncertainty of FbHa1e-15W.m**-2stat.errorfloatnullableFWHMbHa[1010/12436]? Full-width at half-maximum of broad Halphakm/sspect.line.widthintnullablee_FWHMbHa[0/3245]? Formal uncertainty of FWHMbHakm/sstat.errorintnullableEWbHa[2.9/992]? Equivalent width of broad Halpha0.1nmspect.line.eqWidth;em.line.HalphafloatnullablelogMbhGH05[4.5/9.5]? Log of the black hole mass (3)log(solMass)phys.massfloatnullablebHa? Fitting quality flag for broad Halpha (G6)meta.code.qual;stat.fitintnullablelogEddBAT[-2/1.6]? Log Eddington ratio derived from 14-195keV Swift-BAT survey (4)phys.luminosity;arith.ratiofloatnullablelogMbhlit[5.4/9.2]? Log black hole mass from literature (5)log(solMass)phys.massfloatnullablee_logMbhlit? Lower formal uncertainty of logMbhlitlog(solMass)stat.errorfloatnullableE_logMbhlit[0/0.5]? Upper formal uncertainty of logMbhlitlog(solMass)stat.error;stat.maxfloatnullableJ/ApJ/850/74/table10Properties derived from spectral decomposition of high redshift sourcesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[120/1171] Swift-BAT 70-month hard X-ray survey ID (G1)meta.id;meta.mainintCNameCounterpart source namemeta.idcharz[0.5/3.3] Redshiftsrc.redshiftfloatLineBroad emission lines (MgII or CIV) (1)meta.id;spect.linecharlogLcont[45.1/46.8] Monochromatic luminosity (2)log(1e-07W)phys.luminosityfloatFlux[1.7/20.8] Emission line flux (G3)1e-15W.m**-2phot.flux;spect.linefloatEW[9.8/52.4] Equivalent width of the line0.1nmspect.line.eqWidthfloatFWHM[2009/8207] Full-width at half-maximum of the linekm/sspect.line.widthintlogMbh[8.3/9.9] Log black hole masslog(solMass)phys.massfloatlogEdd[-1.2/-0.1] Log Eddington ratiophys.luminosity;arith.ratiofloatFitSpectral fitting quality flag (G6)meta.code.qualint