TY - JOUR
T1 - THE COMPLETE INFRARED VIEW of ACTIVE GALACTIC NUCLEI from the 70 MONTH SWIFT/BAT CATALOG
AU - Ichikawa, Kohei
AU - Ricci, Claudio
AU - Ueda, Yoshihiro
AU - Matsuoka, Kenta
AU - Toba, Yoshiki
AU - Kawamuro, Taiki
AU - Trakhtenbrot, Benny
AU - Koss, Michael J.
N1 - Funding Information:
C.R. acknowledge financial support from the CONICYT-Chile grants EMBIGGEN Anillo ACT1101, FONDECYT 1141218, and Basal-CATA PFB-06/2007. Part of this was financially supported by the Grant-in-Aid for JSPS fellow for young researchers (PD; KI. KM; DC1; TK.).
PY - 2017/1/20
Y1 - 2017/1/20
N2 - We systematically investigate the near- to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert Telescope (BAT) all-sky ultra-hard X-ray (14-195 keV) survey. Out of 606 non-blazar AGNs in the Swift/BAT 70 month catalog at high galactic latitudes of(b) > 10° , we obtain IR photometric data of 604 objects by cross-matching the AGN positions with catalogs from the WISE, AKARI, IRAS, and Herschel infrared observatories. We find a good correlation between the ultra-hard X-ray and mid-IR luminosities over five orders of magnitude (41 < log L14-195 < 46). Informed by previous measurements of the intrinsic spectral energy distribution of AGNs, we find FIR pure-AGN candidates whose FIR emission is thought to be AGN-dominated with low star-formation activity. We demonstrate that the dust covering factor decreases with the bolometric AGN luminosity, confirming the luminosity-dependent unified scheme. We also show that the completeness of the WISE color-color cut in selecting Swift/BAT AGNs increases strongly with 14-195 keV luminosity.
AB - We systematically investigate the near- to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert Telescope (BAT) all-sky ultra-hard X-ray (14-195 keV) survey. Out of 606 non-blazar AGNs in the Swift/BAT 70 month catalog at high galactic latitudes of(b) > 10° , we obtain IR photometric data of 604 objects by cross-matching the AGN positions with catalogs from the WISE, AKARI, IRAS, and Herschel infrared observatories. We find a good correlation between the ultra-hard X-ray and mid-IR luminosities over five orders of magnitude (41 < log L14-195 < 46). Informed by previous measurements of the intrinsic spectral energy distribution of AGNs, we find FIR pure-AGN candidates whose FIR emission is thought to be AGN-dominated with low star-formation activity. We demonstrate that the dust covering factor decreases with the bolometric AGN luminosity, confirming the luminosity-dependent unified scheme. We also show that the completeness of the WISE color-color cut in selecting Swift/BAT AGNs increases strongly with 14-195 keV luminosity.
KW - X-rays: galaxies
KW - galaxies: active
KW - galaxies: nuclei
KW - infrared: galaxies
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U2 - 10.3847/1538-4357/835/1/74
DO - 10.3847/1538-4357/835/1/74
M3 - Article
AN - SCOPUS:85011416595
VL - 835
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 1
M1 - 74
ER -