Table 8
Results from automated fitting of the 770 ks stacked spectrum with Cloudy simulated spectra.
| Best fit Cloudy parameters | ||||||
| SED | Spectrum range | Absorptiona | C-statistic | log ξ | log vturb | log NH |
| Å | (d.o.f) | km s-1 | cm-2 | |||
|
|
||||||
| obscured | 5.7−38.2 | B, E | 2213 (1084) | 2.3 | 2.5 | 22.5 |
| obscured | 5.7−38.2 | A−C | 2178 (1084) | 2.3 | 2.5 | 22.5 |
| unobscured | 5.7−38.2 | B, E | 2298 (1084) | 1.5 | 2.0 | 23 |
| unobscured | 5.7−38.2 | A−C | 2272 (1084) | 1.5 | 2.0 | 22.5 |
|
|
||||||
| unobscured | 21.5−23 | B, E | 97 (49) | 1.7 | 2.5 | 23.25 |
| unobscured | 21.5−23 | A−C | 106 (49) | 1.7 | 2.0 | 22.25 |
|
|
||||||
| unobscured | 5.7 − 38.2 | B, E | 2273 (1084) | 1.45 | 2.25 | 22.9 |
| unobscured | 5.7 − 38.2 | A − C | 2243 (1084) | 1.45 | 2.25 | 22.9 |
Notes. For each fit the Cloudy spectra are given an outflow velocity of −300 km s-1, in order to match the O VII f line (the strongest in the spectrum). The emboldened rows show the best-fits to both absorption scenarios when using the fine grid of Cloudy models.
Letters refer to Kaastra et al. (2014) WA components.
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