Table 2.
Summary of the results obtained from the fits to the average spectra from the XMM-Newton observation of each considered source.
| OBSID | 0823990401 | 0823990501 | 0823990601 | 0823990801 | 0823990901 | 0823991001 | 0844100701 |
|---|---|---|---|---|---|---|---|
| nH | 9.0 ± 0.5 | 3.3 ± 0.6 | 18 ± 5 | 27 ± 6 | 19 ± 1 | 3.5 ± 0.8 | 4.0 ± 0.4 |
| nH, pc | 21 ± 1 | 7.5 ± 1.9 | 36 ± 3 | – | – | 9.2 ± 0.9 | 13 ± 2 |
| Cov. frac. | 0.71 ± 0.03 | 0.77 ± 0.09 | 0.90 ± 0.06 | – | – | 0.90 |
0.74 ± 0.03 |
| Γ | 1.27 ± 0.04 | 2.4 ± 0.2 | 1.4 ± 0.1 | 2.4 |
1.5 ± 0.1 | 1.88 ± 0.10 | 1.96 ± 0.10 |
| Flux (1−10 keV) | 90 ± 3 | 2.0 |
46 ± 5 | 1.1 |
6.7 ± 0.5 | 5.9 ± 0.4 | 8.2 ± 0.7 |
| Cstat/d.o.f. | 305/272 | 264/242 | 241/218 | 326/234 | 165/135 | 254/244 | 302/253 |
Notes. In the table, nH is the absorption column density in the direction of the source, nH, pc is the absorption column density of the partial covering component, Cov. frac. is the corresponding covering fraction, and Γ is the photon index of the power-law component. We also provide the flux measured in the 1−10 keV energy band (in units of 1 × 10−10 erg cm−2 s−1 not corrected for absorption) and the value of the C-statistics together with the degree of freedom of each spectrum.
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