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Table A.1

Coordinates, redshifts, detection significances, count rates, column densities, and luminosities of the Seyfert 1s used for the stacking analysis.

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

IGR J02086−1742 02 08 31.4  −17 43 04.8 0.129 7.3 0.31 ± 0.04  < 0.017a 44.78
IGR J02097+5222 02 09 37.7  + 52 26 43.6 0.049 13.5 0.56 ± 0.04 0.03b 44.20
Mrk 590 02 14 33.6  −00 46 00.3 0.027 5.0 0.13 ± 0.03 0.03c 43.05
Mrk 1040 02 28 14.6 +31 18 39.4 0.016 8.4 0.72 ± 0.09 0.067d 43.33
RBS 345 02 42 16.0 +05 31 48.0 0.069 5.1 0.23 ±  0.04 44.11
ESO 548−01 03 41 54.7  −21 15 28.8 0.014 6.1 0.64 ± 0.11 43.17
UGC 3142 04 43 46.9 +28 58 19.0 0.022 13.8 0.58 ± 0.04 1.4e 43.52
LEDA 168563 04 52 04.7 +49 32 45.0 0.029 11.6 0.51 ± 0.04  < 0.22b 43.70
Ark 120 05 16 11.5  −00 09 00.6 0.033 29.3 0.77 ± 0.03  < 0.1c 43.99
EXO 055620−3820.2 05 58 02.0  −38 20 01.0 0.034 5.6 0.31 ± 0.06 2.57f 43.62
IRAS 05589+2828 06 02 09.7 +28 28 17.0 0.033 17.5 0.61 ± 0.03  < 0.04b 43.89
SWIFT J0640.4−2554 06 40 10.8  −25 49 48.0 0.026 5.0 0.39 ± 0.08 0.33f 43.49
IGR J07597−3842 07 59 41.7  −38 43 57.4 0.040 21.8 0.60 ± 0.03 0.05d 44.05
PG 0804+761 08 10 58.7 +76 02 42.5 0.100 5.0 0.20 ± 0.04 0.023d 44.37
Fairall 1146 08 38 30.7  −35 59 35.0 0.032 14.0 0.34 ± 0.02 0.1d 43.61
IGR J09026−4812 09 02 37.3  −48 13 34.1 0.039 21.6 0.37 ± 0.02 0.9g 43.82
SWIFT J0917.2−6221 09 16 09.4  −62 19 29.5 0.057 12.1 0.34 ± 0.03 0.5h 44.11
4U 0937−12 09 45 42.1  −14 19 35.0 0.008 17.1 0.99 ± 0.06 1.19f 42.87
SWIFT J1038.8−4942 10 38 45.0  −49 46 55.0 0.060 9.3 0.25 ± 0.03 1.55f 44.02
IGR J11457−1827 11 45 41.0  −18 27 29.0 0.033 6.8 0.87 ± 0.13  ≃ 0f 44.05
IGR J12107+3822 12 10 43.4 +38 22 51.6 0.023 5.3 0.17 ± 0.03 43.02
IGR J12136−0527 12 13 37.0  −05 26 53.0 0.066 5.3 0.16 ± 0.03 2.0i 43.91
IGR J12172+0710 12 17 09.0 +07 09 33.0 0.007 8.3 0.22 ± 0.03 0.15i 42.10
Mrk 50 12 23 24.1 +02 40 44.8 0.023 8.9 0.22 ± 0.02 0.018d 43.14
NGC 4593 12 39 39.4  −05 20 39.3 0.009 39.7 1.03 ± 0.03 0.02j 42.99
ESO 323−77 13 06 26.6  −40 24 50.0 0.015 16.6 0.50 ± 0.03 6.0k 43.12
IGR J13109−5552 13 10 43.1  −55 52 11.7 0.104 15.2 0.31 ± 0.02  < 0.1c 44.60
Mrk 279 13 53 03.5 +69 18 29.2 0.031 5.0 0.64 ± 0.13 0.02f 43.86
RHS 39 14 19 22.2  −26 38 41.0 0.022 10.4 0.46 ± 0.04  < 0.05c 43.42
IGR J14471−6414 14 46 28.3  −64 16 24.1 0.053 9.7 0.19 ± 0.02  < 0.1c 43.80
IGR J16119−6036 16 11 51.4  −60 37 53.1 0.016 14.8 0.33 ± 0.02 0.1d 43.00
IGR J16482−3036 16 48 14.9  −30 35 06.1 0.031 29.9 0.62 ± 0.02 0.13c 43.85
IGR J16558−5203 16 56 05.7  −52 03 41.2 0.054 23.9 0.47 ± 0.02 0.011c 44.21
IGR J17418−1212 17 41 55.3  −12 11 57.5 0.037 19.4 0.43 ± 0.02 0.1d 43.84
IGR J18027−1455 18 02 48.0  −14 54 54.8 0.035 23.6 0.42 ± 0.02 0.41l 43.78
IGR J18259−0706 18 25 57.6  −07 10 22.8 0.037 13.2 0.24 ± 0.02 0.6c 43.58
ESO 140-43 18 44 54.0  −62 21 52.9 0.014 11.8 0.52 ± 0.04 1.8e 43.08
IGR J18559+1535 18 56 00.6 +15 37 58.0 0.084 18.3 0.35 ± 0.02 0.7a 44.46
ESO 141-55 19 21 14.2  −58 40 15.0 0.037 12.7 0.64 ± 0.05 0.004c 44.01
SWIFT J1933.9+3258 19 33 47.3 +32 54 25.0 0.056 7.0 0.22 ± 0.03  < 0.04m 43.91
IGR J19405−3016 19 40 15.2  −30 15 48.5 0.052 9.0 0.29 ± 0.03  < 0.1c 43.97
RX J2135.9+4728 21 35 54.4 +47 28 28.3 0.025 14.1 0.28 ± 0.02 0.4c 43.31
IGR J22292+6647 22 29 13.5 +66 46 51.8 0.113 9.7 0.22 ± 0.02 0.2c 44.52
IGR J23206+6431 23 20 36.8 +64 30 42.8 0.072 9.0 0.15 ± 0.02 0.6c 43.96

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.

(a)

Rodriguez et al. (2010);

(b)

Winter et al. (2008) and references therein;

(c)

Beckmann et al. (2009) and ref. therein;

(d)

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

(e)

Ricci et al. (2010);

(f)

Winter et al. (2009);

(g)

Tomsick et al. (2008);

(h)

Malizia et al. (2007);

(i)

Paltani et al. (2008) and ref. therein;

(j)

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

(k)

Jiménez-Bailón et al. (2008);

(l)

Panessa et al. (2008);

(m)

Landi et al. (2007a).

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