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Table A.4

Coordinates, redshifts, detection significances, count rates, column densities, and luminosities of the Compton-thick Seyfert 2s used for the stacking analysis.

Name RA Dec z Det. significance Count rate N   H log L17−80   keV
[h m s] [° ′ ″] [σ] [ct   s-1] [1022   cm-2] [erg   s-1]

NGC 1068 02 42 40.8  −00 00 48.4 0.003 14.0 0.45 ± 0.03 150a 41.91
SWIFT J0601.9−8636 06 05 39.1  −86 37 52.0 0.006 7.3 0.40 ± 0.06 101b 42.40
Mrk 3 06 15 36.3 +71 02 14.9 0.014 31.3 1.43 ± 0.05 110c 43.70
NGC 3281 10 31 52.1  −34 51 13.3 0.011 12.0 0.78 ± 0.07 151d 43.26
IGR J13091+1137 13 09 05.6 +11 38 02.9 0.025 14.8 0.51 ± 0.03 90c 43.73
NGC 5643 14 32 41.3  −44 10 24.0 0.003 9.2 0.20 ± 0.02 60−100e 41.50
Mrk 477 14 40 38.1 +53 30 15.9 0.037 5.8 0.44 ± 0.07  >100f 44.09
NGC 5728 14 42 23.3  −17 16 51.6 0.009 13.6 0.80 ± 0.06 210a 43.12
IGR J16351−5806 16 35 13.2  −58 04 49.7 0.009 12.9 0.28 ± 0.02  >150g 42.69
NGC 7582 23 18 23.5  −42 22 14.1 0.005 5.5 1.20 ± 0.20 160a 42.77

Notes. Detection significances, count rates, and luminosities are in the 17–80 keV band. The flux of the Crab in the 17–80 keV band is of 278   ct   s-1.

References. 

(a)

Della Ceca et al. (2008) and ref. therein;

(b)

Ueda et al. (2007);

(c)

Beckmann et al. (2006) and ref. therein;

(d)

Bodaghee et al. (2007) and ref. therein;

(e)

Guainazzi et al. (2004);

(f)

Bassani et al. (1999);

(g)

Malizia et al. (2009).

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