J/ApJ/870/31 BAT AGN spectroscopic survey. XI. IR photometry (Ichikawa+, 2019) ================================================================================ BAT AGN spectroscopic survey. XI. The covering factor of dust and gas in Swift/BAT active galactic nuclei. Ichikawa K., Ricci C., Ueda Y., Bauer F.E., Kawamuro T., Koss M.J., Oh K., Rosario D.J., Shimizu T.T., Stalevski M., Fuller L., Packham C., Trakhtenbrot B. =2019ApJ...870...31I (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Active gal. nuclei; Redshifts; Energy distributions; Photometry, infrared; Surveys Keywords: galaxies: active; galaxies: nuclei; infrared: galaxies Abstract: We quantify the luminosity contribution of active galactic nuclei (AGNs) to the 12{mu}m, mid-infrared (MIR; 5-38{mu}m), and total IR (5-1000{mu}m) emission in the local AGNs detected in the all-sky 70 month Swift/Burst Alert Telescope (BAT) ultrahard X-ray survey. We decompose the IR spectral energy distributions (SEDs) of 587 objects into the AGN and starburst components using templates for an AGN torus and a star-forming galaxy. This enables us to recover the emission from the AGN torus including the low-luminosity end, down to log(L_14-150_/erg/s)~41, which typically has significant host galaxy contamination. The sample demonstrates that the luminosity contribution of the AGN to the 12{mu}m, the MIR, and the total IR bands is an increasing function of the 14-150keV luminosity. We also find that for the most extreme cases, the IR pure-AGN emission from the torus can extend up to 90{mu}m. The total IR AGN luminosity obtained through the IR SED decomposition enables us to estimate the fraction of the sky obscured by dust, i.e., the dust covering factor. We demonstrate that the median dust covering factor is always smaller than the median X-ray obscuration fraction above an AGN bolometric luminosity of log(L_bol_^(AGN)^/erg/s)~42.5. Considering that the X-ray obscuration fraction is equivalent to the covering factor coming from both the dust and gas, this indicates that an additional neutral gas component, along with the dusty torus, is responsible for the absorption of X-ray emission. Description: Our initial sample is based on the sample of Ichikawa+ (2017, J/ApJ/835/74), which contains the 606 non-blazar AGNs from the Swift/BAT 70 month catalog (Baumgartner+ 2013, J/ApJS/207/19) at galactic latitudes (|b|>10{deg}) for which secure spectroscopic redshifts are available. In this study, we use the column density (N_H_) and the absorption-corrected 14-150keV luminosity (L_14-150_) tabulated in Ricci+ (2017, J/ApJS/233/17). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 415 606 The IR catalog of the Swift/BAT 70 month AGN survey -------------------------------------------------------------------------------- See also: B/swift : Swift Master Catalog (HEASARC, 2004-) II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) II/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989) II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010) II/298 : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010) VI/139 : Herschel Observation Log (Herschel Science Centre, 2013) II/328 : AllWISE Data Release (Cutri+ 2013) VIII/106 : Herschel/PACS Point Source Catalogs (Herschel team, 2017) J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006) J/ApJ/666/806 : SED of Spitzer quasars (QUEST) (Netzer+, 2007) J/ApJ/679/140 : IR measurement of quasar obscuration (Treister+, 2008) J/ApJ/681/113 : Swift BAT survey of AGNs (Tueller+, 2008) J/MNRAS/386/1252 : SWIRE/SDSS quasars (Hatziminaoglou+, 2008) J/A+A/505/417 : Second INTEGRAL AGN catalogue (Beckmann+, 2009) J/AJ/144/11 : IR, nuclear SEDs & Spitzer spectra of 22 AGNs (Mason+, 2012) J/ApJ/754/45 : IR properties of Swift/BAT X-ray AGNs (Ichikawa+, 2012) J/MNRAS/419/2095 : HMXBs in nearby galaxies (Mineo+, 2012) J/A+A/558/A149 : VLTI/MIDI AGN Large Program observations (Burtscher+, 2013) J/ApJS/207/19 : Hard X-ray survey Swift-BAT 2004-2010 (Baumgartner+, 2013) J/MNRAS/430/3445 : Covering factor of warm dust in quasars (Ma+, 2013) J/ApJ/794/152 : PACS observations of Herschel-BAT sample (Melendez+, 2014) J/MNRAS/439/1648 : Subarcsecond mid-infrared atlas of local AGN (Asmus+, 2014) J/ApJ/803/109 : Spitzer spectral decompositon AGN (Hernan-Caballero+,2015) J/ApJ/806/109 : Rest-frame optical spectra of 3 in Simbad). Note (2): References as follow: A = AKARI PSC; Murakami+ 2007PASJ...59S.369M P = Hershel/PACS; Griffin+ 2010A&A...518L...3G, Poglitsch+ 2010A&A...518L...2P W = WISE; Wright+ 2010AJ....140.1868W (see Cat. II/328) IF = IRAS Faint Source Catalog; Moshir+ 1989, II/156 IP = IRAS Point Source Catalog; IPAC 1986, II/125 -------------------------------------------------------------------------------- History: From electronic version of the journal References: Koss et al. Paper I. 2017ApJ...850...74K Cat. J/ApJ/850/74 Berney et al. Paper II. 2015MNRAS.454.3622B Oh et al. Paper III. 2017MNRAS.464.1466O Lamperti et al. Paper IV. 2017MNRAS.467..540L Cat. J/MNRAS/467/540 Ricci et al. Paper V. 2017ApJS..233...17R Cat. J/ApJS/233/17 Trakhtenbrot et al. Paper VI. 2017MNRAS.470..800T Ricci et al. Paper VII. 2017Natur.549..488R Shimizu et al. Paper VIII. 2018ApJ...856..154S Powell et al. Paper IX. 2018ApJ...858..110P Oh et al. Paper X. 2018ApJS..235....4O Cat. J/ApJS/235/4 Ichikawa et al. Paper XI. 2019ApJ...870...31I This catalog Ricci et al. Paper XII. 2018MNRAS.480.1819R Bar et al. Paper XIII. 2019MNRAS.489.3073B Paliya et al. Paper XVI. 2019ApJ...881..154P Cat. J/ApJ/881/154 Baek et al. Paper XVII. 2019MNRAS.488.4317B Liu et al. Paper XVIII. 2020ApJ...896..122L Rojas et al. Paper XIX. 2020MNRAS.491.5867R Koss et al. Paper XX. 2021ApJS..252...29K Cat. J/ApJS/252/29 Koss et al. Paper XXI. 2022ApJS..261....1K Koss et al. Paper XXII. 2022ApJS..261....2K Cat. J/ApJS/261/2 Pfeifle et al. Paper XXIII. 2022ApJS..261....3P Oh et al. Paper XXIV. 2022ApJS..261....4O Cat. J/ApJS/261/4 Mejia-Restrepo et al. Paper XXV. 2022ApJS..261....5M Cat. J/ApJS/261/5 Koss et al. Paper XXVI. 2022ApJS..261....6K Cat. J/ApJS/261/6 Gupta et al. Paper XXVII. 2021MNRAS.504..428G den Brok et al. Paper XXVIII. 2022ApJS..261....7D Cat. J/ApJS/261/7 Ricci et al. Paper XXIX. 2022ApJS..261....8R Cat. J/ApJS/261/8 Ananna et al. Paper XXX. 2022ApJS..261....9A Kakkad et al. Paper XXXI. 2022MNRAS.511.2105K Kawamuro et al. Paper XXXII. 2022ApJ...938...87K Marcotulli et al. Paper XXXIII. 2022ApJ...940...77M Cat. J/ApJ/940/77 Kawamuro et al. Paper XXXIV. 2023ApJS..269...24K Cat. J/ApJS/269/24 Caglar et al. Paper XXXV. 2023ApJ...956...60C Powell et al. Paper XXXVI. 2022ApJ...938...77P Ricci et al. Paper XXXVII. 2022ApJ...938...67R Ananna et al. Paper XXXVIII. 2022ApJ...939L..13A Temple et al. Paper XXXIX. 2023MNRAS.518.2938T Tortosa et al. Paper XL. 2023MNRAS.526.1687T Ricci et al. Paper XLII. 2023ApJ...959...27R ================================================================================ (End) Prepared by [AAS], Coralie Fix [CDS] 28-Jan-2020