Table C.1
Flux-limited sample: relevant best-fit-model parameters corresponding to the neutral reflection run and 6.4 keV relativistic Fe Kα line.
| Source | Power Law | Warm Absorber | Compton Reflection | EW Narrow Fe Kα Emission Lines | ||||
| Γ | NH | ξ | R | Norm | FeI 6.4 keV | FeXXV 6.7 keV | FeXXVI 6.96 keV | |
| (1022 cm-2) | (erg cm-1 s-1) | (10-3 keV-1 cm-2 s-1) | (eV) | (eV) | (eV) | |||
|
|
||||||||
| AKN564 | 2.82 |
0.76 |
– | 2.22 |
18.38 |
< 18 | 13 |
< 4 |
| NGC526A | 1.52 |
1.24 |
< 0.47 | < 0.77 | 4.46 |
42 |
< 26 | < 22 |
| MCG-6-30-15 | 2.05 |
0.80 |
6.30 |
0.51 |
17.38 |
44 |
< 5 | < 7 |
| MRK766 | 2.10 |
0.40 |
10.37 |
0.78 |
> 6.87 | 32 |
< 21 | 20 |
| NGC5548 | 1.64 |
< 0.42 | – | 0.20 |
8.57 |
67 |
< 4 | < 7 |
| MCG+8-11-11 | 1.78 |
< 6.24 | – | 1.37 |
11.78 |
97 |
< 10 | < 17 |
| MRK704 | 1.72 |
9.67 |
105.42 |
< 3.33 | 3.37 |
< 83 | < 42 | < 45 |
| NGC3516 | 1.61 |
4.48 |
77.03 |
1.99 |
4.02 |
140 |
< 7 | < 5 |
| MCG-5-23-16 | 1.65 |
1.20 |
< 0.02 | 1.15 |
19.37 |
32 |
< 5 | < 5 |
| NGC3227 | 1.52 |
0.09 |
< 25.38 | 0.15 |
6.70 |
59 |
< 5 | 8 |
| H0557-385 | 1.86 |
1.22 |
5.67 |
< 3.28 | 13.63 |
< 31 | < 14 | < 26 |
| NGC4593 | 1.84 |
< 4.07 | – | 1.24 |
11.88 |
39 |
< 10 | 14 |
| NGC7469 | > 1.97 | < 0.53 | – | 1.79 |
10.07 |
73 |
< 3 | < 9 |
| NGC3783 | 1.70 |
1.64 |
54.21 |
0.51 |
13.44 |
90 |
< 1 | 23 |
| ESO511-G030 | 1.93 |
< 1.38 | – | 2.10 |
6.31 |
11 |
< 14 | < 12 |
| IRAS05078+1626 | 1.72 |
4.94 |
– | 1.70 |
5.96 |
38 |
11 |
< 11 |
| MRK279 | 1.83 |
< 0.51 | – | 1.16 |
7.79 |
55 |
< 3 | 7 |
| MRK509 | > 1.96 | < 0.2 | – | 2.49 |
12.88 |
34 |
< 4 | < 3 |
| NGC7314 | 2.09 |
1.35 |
4.86 |
1.16 |
18.22 |
< 56 | 14 |
27 |
| NGC7213 | 1.76 |
< 7.67 | – | < 0.77 | 5.80 |
82 |
22 |
17 |
| IC4329A | 1.79 |
0.33 |
< 0.47 | 0.93 |
26.85 |
34 |
< 4 | 8 |
| MR2251-178 | 1.32 |
< 0.61 | – | 0.54 |
3.06 |
23 |
< 5 | < 2 |
| H1846-786 | 1.87 |
< 8.95 | – | > 0 | 1.98 |
78 |
< 35 | 104 |
| FAIRALL9 | 1.90 |
< 2.67 | – | 1.70 |
3.56 |
107 |
< 21 | < 29 |
| UGC3973 | 1.78 |
< 37.79 | – | > 0 | 3.06 |
156 |
< 87 | < 38 |
| MCG-2-58-22 | 1.69 |
< 2.93 | – | < 3.32 | 7.65 |
< 51 | < 20 | 21 |
| NGC4051 | 2.02 |
2.21 |
– | < 1.49 | 9.48 |
63 |
17 |
< 17 |
| MRK590 | 1.61 |
< 3.39 | – | 0.59 |
1.46 |
113 |
< 31 | 41 |
| ARK120 | 2.12 |
< 0.52 | – | 2.14 |
15.95 |
65 |
15 |
9 |
| MRK110 | 1.88 |
< 1.21 | – | 1.47 |
8.58 |
33 |
< 6 | < 3 |
| ESO198-G24 | 1.79 |
< 2.57 | – | 1.79 |
2.7 |
60 |
< 8 | < 8 |
|
|
||||||||
Notes. Errors are given at the 90% confidence level. Upper limits to the relevant parameters are also given at the 90% confidence level. Sources with a significant broad Fe Kα line detection are marked in bold (as listed in Table 2).
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.