VizieR Online Data Catalog: IR photometry and SEDs of hard X-ray AGNs (Kilerci+, 2020)

The Swift observatory (Gehrels et al. 2004ApJ...611.1005G) scans the whole sky at 14-195 keV with the wide-field BAT (Barthelmy et al. 2005SSRv..120..143B). With its continuous all-sky survey, Swift/BAT identified several hard-X-ray selected AGNs in the local Universe (e.g. Tueller et al. 2008ApJ...681..113T, Cat. J/ApJ/681/113; Baumgartner et al. 2013ApJS..207...19B, Cat. J/ApJS/207/19; Ricci et al. 2017ApJS..233...17R, Cat. J/ApJS/233/17; Oh et al. 2018ApJS..235....4O, Cat. J/ApJS/235/4). The most recent data release of Swift/BAT includes 947 hard X-ray selected non-beamed AGNs. We cross-match these hard X-ray selected AGNs based on their optical counterpart coordinates within the AKARI/FIS all-sky survey bright source catalogue version 2 (Yamamura et al. 2018cwla.conf..227Y) within a radius of 20arcsec. We find the AKARI 90-μm detection for 378 AGNs, which is near the peak of the FIR dust emission near 100μm.

The Swift/BAT Spectroscopic Survey (BASS; Koss et al. 2017ApJ...850...74K, Cat. J/ApJ/850/74) data release 1 provides multiwavelength data of 836 local AGNs from the Swift/BAT 70-month catalogue (Baumgartner et al. 2013ApJS..207...19B, Cat. J/ApJS/207/19). The broad-band X-ray (between 0.3-150keV) spectral analysis of the BASS AGN sample is completed by Ricci et al. (2017ApJS..233...17R, Cat. J/ApJS/233/17). BASS includes 311 of the AGNs in our AKARI AGN sample, so for these sources we adopt the N_H values from BASS; except for ESO244-IG030 and ESO317-G041 for which we adopt the revised N_H measurements from Marchesi et al. (2019ApJ...882..162M). For 19 AGNs in our AKARI AGN sample, we take published N_H values from the literature. In total, 338 AGNs in our sample have N_H measurements (see Table 1).

(1 data file).