Table 2
X-ray properties of the high-τ 9.7 μm AGN in the 12 μm sample.
Name | z | N H | log [Lx] | X-ray Ref. | Mission | Comment |
(1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
||||||
Mrk 938 | 0.020 | 40 | 42.30 | 1, 16 | XMM | – |
NGC 1125 | 0.011 | – | 41.97 | 2 | Swift | – |
I 08572+3915 | 0.058 | – | 41.30 | 3 | Chandra | – |
UGC 5101 | 0.039 | 140 | 41.67 | 4, 6, 7, 8, 11, 16 | Chandra/XMM | a |
NGC 3079 | 0.004 | 200 | 40.25 | 5, 16 | XMM | a |
Mrk 266 | 0.028 | >160 | 41.7 | 1, 6 | XMM/Chandra | a |
Mrk 273 | 0.038 | 40 | 42.40 | 10, 16 | Chandra | – |
Arp 220 | 0.018 | >100 | 40.96 | 7, 12, 14 | XMM | b,c |
I 19254-7245 | 0.062 | >100 | 42.57 | 7, 8, 13 | BeppoSAX | a |
NGC 7172 | 0.009 | 8 | 42.20 | 9 | BeppoSAX | – |
NGC 7582 | 0.005 | 160 | 42.00 | 9, 15, 17 | BeppoSAX | a |
Notes. The columns are: (1) Name. (2) Redshift. (3) X-ray column density in units of 1022 cm-2. (4) Logarithm of the obscured X-ray luminosity in the 2−10 keV band in units of erg s-1. (5) X-ray spectroscopy reference: 1) Guainazzi et al. (2005); 2) Cusumano et al. (2010); 3) Iwasawa et al. (2009); 4) Imanishi et al. (2003); 5) Akylas & Georgantopoulos (2009); 6) Brassington et al. (2007); 7) Iwasawa et al. (2005); 8) Braito et al. (2003); 9) Dadina (2008); 10) Iwasawa et al. (2011); 11) González-Martin et al. (2009); 12) Ptak et al. (2003); 13) Georgantopoulos et al. (2010); 14) Clements et al. (2002); 15) Bianchi et al. (2009); 16) Brightman & Nandra (2011). (6) X-ray mission. (7) X-ray criterion on which the source is classified as Compton-thick: a. detection of the absorption turnover b. high-equivalent width FeKα line c. Flat spectrum (see text for details).
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