Table A.2
Coordinates, redshifts, detection significances, count rates, column densities, and luminosities of the Seyfert 1.5s 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] | ||
|
|||||||
IGR J00335+6126 | 00 33 18.4 | +61 27 42.4 | 0.105 | 9.2 | 0.14 ± 0.02 | 0.5a | 44.26 |
Mrk 1152 | 01 13 50.1 | −14 50 44.1 | 0.052 | 5.0 | 0.47 ± 0.09 | 2.7b | 44.17 |
NGC 985 | 02 34 37.8 | −08 47 15.4 | 0.043 | 14.9 | 0.42 ± 0.03 | 0.6c | 43.96 |
IGR J03334+3718 | 03 33 18.8 | +37 18 11.4 | 0.055 | 5.0 | 0.18 ± 0.03 | – | 43.81 |
4U 0517+17 | 05 10 45.5 | +16 29 55.0 | 0.017 | 25.3 | 0.90 ± 0.04 | 0.1c | 43.40 |
SWIFT J0519.5−3140 | 05 19 35.7 | −32 39 25.0 | 0.013 | 14.9 | 0.67 ± 0.05 | 26.6e | 43.12 |
MCG+08−11−011 | 05 54 53.6 | +46 26 21.8 | 0.020 | 24.9 | 1.81 ± 0.07 | 0.18c | 43.93 |
Mrk 6 | 06 52 12.3 | +74 25 36.8 | 0.019 | 16.7 | 0.74 ± 0.04 | 10d | 43.50 |
ESO 209−12 | 08 01 57.6 | −49 46 42.0 | 0.040 | 15.8 | 0.34 ± 0.02 | 0.1c | 43.81 |
IGR J09253+6929 | 09 25 47.6 | +69 27 51.5 | 0.039 | 5.1 | 0.29 ± 0.06 | 8f | 43.72 |
NGC 3227 | 10 23 30.6 | +19 51 53.7 | 0.003 | 17.4 | 1.88 ± 0.11 | 6.8c | 42.30 |
NGC 3516 | 11 06 47.6 | +72 34 08.3 | 0.009 | 6.5 | 1.26 ± 0.19 | 4g | 43.08 |
NGC 3783 | 11 39 01.8 | −37 44 18.7 | 0.009 | 10.9 | 2.05 ± 0.19 | 0.08b | 43.29 |
IGR J12415−5750 | 12 41 25.4 | −57 50 04.0 | 0.024 | 16.2 | 0.33 ± 0.02 | <0.11c | 43.35 |
IGR J13133−1109 | 13 13 17.0 | −11 08 34.0 | 0.034 | 5.0 | 0.20 ± 0.04 | – | 43.43 |
MCG−06−30−015 | 13 35 53.8 | −34 17 44.0 | 0.008 | 23.2 | 0.74 ± 0.03 | 0.03c | 42.75 |
IGR J14080−3023 | 14 08 06.6 | −30 23 52.6 | 0.023 | 5.0 | 0.18 ± 0.04 | 0.03h | 43.05 |
NGC 5548 | 14 17 59.7 | +25 08 13.4 | 0.017 | 7.1 | 0.49 ± 0.07 | 0.51d | 43.22 |
QSO B1419+480 | 14 21 29.6 | +47 47 26.0 | 0.072 | 5.2 | 0.25 ± 0.05 | 0.5i | 44.18 |
PG 1501+106 | 15 04 01.2 | +10 26 16.2 | 0.036 | 7.2 | 0.49 ± 0.07 | 3.9j | 43.87 |
SWIFT J1930.5+3414 | 19 30 13.7 | +34 10 52.0 | 0.062 | 8.8 | 0.28 ± 0.03 | 27.5e | 44.10 |
NGC 6814 | 19 42 40.4 | −10 19 24.0 | 0.005 | 25.9 | 0.79 ± 0.03 | < 0.05d | 42.37 |
SWIFT J2009.0−6103 | 20 08 47.0 | −61 05 48.0 | 0.015 | 7.6 | 0.61 ± 0.08 | 4.53e | 43.21 |
Mrk 509 | 20 44 09.8 | −10 43 24.7 | 0.035 | 16.0 | 1.12 ± 0.07 | <0.01d | 44.21 |
1RXS J211928.4+333259 | 21 19 35.5 | +33 33 03.6 | 0.051 | 9.8 | 0.29 ± 0.03 | – | 43.95 |
1RXS J213944.3+595016 | 21 39 42.7 | +59 49 37.2 | 0.114 | 5.5 | 0.13 ± 0.02 | – | 44.30 |
1H 2251−179 | 22 54 05.9 | −17 34 55.3 | 0.064 | 9.5 | 1.12 ± 0.12 | < 0.19d | 44.73 |
NGC 7469 | 23 03 15.8 | +08 52 25.9 | 0.017 | 10.3 | 0.78 ± 0.08 | 0.061c | 43.42 |
MCG−02−58−022 | 23 04 43.5 | −08 41 08.6 | 0.047 | 8.2 | 0.71 ± 0.09 | < 0.08d | 44.27 |
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.
Beckmann et al. (2009) and ref. therein;
Fiore et al. (1997);
Bodaghee et al. (2007) and ref. therein;
Beckmann et al. (2006) and ref. therein;
Winter et al. (2009) and ref. therein;
Rodriguez et al. (2008);
Guainazzi et al. (2002);
Landi et al. (2010);
Barcons et al. (2003);
Longinotti et al. (2010).
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