Table E.1
Summary of the results of the self-consistent reflection model.
| Source | Distant reflection | Disc reflection | Disc ionisation | θ | a | β | χ2/d.o.f. |
| (erg cm s-1) | (°) | ||||||
|
|
|||||||
| IC 4329A | 0.5 ± 0.2 | 0.3 ± 0.2 |
|
|
≥ 0 |
|
197.2/163 |
| MCG-5-23-16 | 0.3 ± 0.1 | 0.5 ± 0.3 | ≤ 70 |
|
≥ 0 |
|
247.3/164 |
| ESO511-G030 | 0.7 ± 0.2 | 0.8 ± 0.4 | 70 ± 50 |
|
≥ 0 |
|
185.0/162 |
| MCG-6-30-15 | 0.2 ± 0.1 | 2.4 ± 0.8 |
|
39 ± 5 | ≥ 0.8 | 3.4 |
192.1/164 |
| NGC 4051 | 0.9 ± 0.3 | 1.0 ± 0.5 |
|
|
≥ 0.3 | 2.5 |
172.0/162 |
| NGC 3516 | 1.5 ± 0.3 | 1.8 ± 0.5 | ≤ 70 |
|
≥ 0.3 | 2.7 ± 0.4 | 212.7/161 |
| NGC 3783 | 0.8 ± 0.2 | 0.8 ± 0.4 | ≤ 90 |
|
≥ 0.2 | 3.1 |
221.4/163 |
| NGC 3227 | 0.6 ± 0.2 | 0.5 ± 0.3 |
|
26 ± 9 | ≥ 0 | 2.3 |
226.5/162 |
| MRK 509 | 0.3 ± 0.1 | 1.0 ± 0.6 |
|
≥ 45 | ≥ 0.4 | 2.8 |
244.2/160 |
| MRK 766 | 0.3 ± 0.1 | 0.8 ± 0.4 |
|
28 ± 8 | ≥ 0.3 | 2.6 |
262.5/162 |
| ARK 120 | 1.0 ± 0.3 | 0.7 ± 0.4 |
|
45 ± 10 | ≥ 0.1 | 2.7 |
188.7/160 |
Notes. All sources for which a detection of a relativistic line component is claimed in the paper have been described with two self-consistent reflection models, one for distant reflection (the PEXMON model), the other for disc reflection (the REFLION model). The relevant parameters and fitting statistics are reported in this table.
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