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.
Bodaghee et al. (2007) and ref. therein;
Beckmann et al. (2009) and ref. therein;
Beckmann et al. (2006) and ref. therein;
Grupe et al. (1998);
Jiménez-Bailón et al. (2008);
Malizia et al. (2008);
Rodriguez et al. (2008);
Malizia et al. (2008).
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