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Table A.5

Coordinates, redshifts, detection significances, count rates, column densities, and luminosities of the Narrow Lines Seyfert 1s 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]

1H 0323+342 03 24 41.2 +34 10 45.9 0.063 5.9 0.20 ± 0.03 0.1a 43.97
Mrk 110 09 25 12.9 +52 17 10.5 0.035 5.0 0.86 ± 0.17 0.019a 44.09
NGC 4051 12 03 09.6 +44 31 53.2 0.002 13.6 0.47 ± 0.03  < 0.02b 41.34
Mrk 766 12 18 26.6 +29 48 45.6 0.013 7.7 0.26 ± 0.03 0.8c 42.71
NGC 4748 12 52 12.0  −13 25 48.0 0.014 5.2 0.16 ± 0.03  ≃ 0d 42.57
Mrk 783 13 02 58.8 +16 24 27.5 0.067 7.3 0.25 ± 0.03 0.046a 44.12
NGC 5506 14 13 14.9  −03 12 27.0 0.007 47.2 2.7 ± 0.06 3.4b 43.19
IGR J14552−5133 14 55 17.9  −51 34 13.3 0.016 12.5 0.25 ± 0.02 0.1a 42.88
IRAS 15091−2107 15 11 54.0  −21 21 21.6 0.044 5.3 0.22 ± 0.04 0.7e 43.70
IGR J16185−5928 16 18 26.4  −59 28 45.3 0.035 10.7 0.23 ± 0.02  < 0.1f 43.52
IGR J16385−2057 16 38 31.1  −20 55 25.0 0.027 7.7 0.26 ± 0.03 0.21g 43.35
IGR J19378−0617 19 37 33.1  −06 13 04.0 0.010 11.2 0.32 ± 0.03  ≃ 0h 42.58
ESO 399−20 20 06 57.2  −34 32 54.0 0.025 6.5 0.23 ± 0.04 0.048a 43.23
IGR J21277+5656 21 27 45.9 +56 56 34.4 0.014 24.2 0.52 ± 0.02 0.1a 43.08

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)

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

(b)

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

(c)

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

(d)

Grupe et al. (1998);

(e)

Jiménez-Bailón et al. (2008);

(f)

Malizia et al. (2008);

(g)

Rodriguez et al. (2008);

(h)

Malizia et al. (2008).

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