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.
Rodriguez et al. (2010);
Winter et al. (2008) and references therein;
Beckmann et al. (2009) and ref. therein;
Bodaghee et al. (2007) and ref. therein;
Ricci et al. (2010);
Winter et al. (2009);
Tomsick et al. (2008);
Malizia et al. (2007);
Paltani et al. (2008) and ref. therein;
Beckmann et al. (2006) and ref. therein;
Jiménez-Bailón et al. (2008);
Panessa et al. (2008);
Landi et al. (2007a).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.