Table D.1.
Results from fitting different models to the pn spectra.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|---|---|---|---|---|---|---|---|
| Object | Time | nH | kT | Γ | C-stat (d.o.f.) | Fabs | Funabs |
| selection | (×1022 at. cm−2) | (keV) | (10−13 erg cm−2 s−1) | ||||
| 6 J015709.1+373739 | A | < 0.12 | 0.16  |
... | 19.79 (19) | 0.16  |
0.26  |
| < 1.14 | ... | 2.95  |
14.83 (19) | 0.20  |
0.41  |
||
| 8 J174610.8−290021 | A | 22.71  |
1.92  |
... | 88.88 (90) | 1.81  |
4.10  |
30.38  |
... | 1.74  |
88.69 (90) | 1.86  |
9.17  |
||
| 25 J113407.5+005223 | A | < 0.18 | 0.30  |
... | 36.30 (20) | 0.15  |
0.17  |
0.31  |
... | 3.55  |
35.56 (20) | 1.89  |
0.18  |
||
| M 31-1 J004307.5+412019 | B | < 0.50 | 0.32  |
... | 1.72 (2) | 0.83  |
1.15  |
| < 0.12 | ... | 1.91  |
0.68 (2) | 1.91  |
2.68  |
||
| P | < 0.16 | 0.22  |
... | 73.23 (51) | 0.23  |
0.39  |
|
0.23  |
... | 3.31  |
56.71 (51) | 0.32  |
2.03  |
||
| M 31-3 J004215.6+411720 | B | < 0.39 | 0.68  |
... | 2.72 (3) | 1.33  |
1.47  |
| < 0.54 | ... | 0.74  |
0.48 (3) | 3.55  |
3.60  |
||
| P | < 0.19 | 0.65  |
... | 50.42 (50) | 0.56  |
0.61  |
|
0.25  |
... | 1.64  |
36.78 (50) | 0.96  |
1.32  |
||
| M 31-6 J004210.9+411248 | B | < 3.86 | 0.71  |
... | 7.23 (2) | 3.22  |
3.50  |
| < 3.55 | ... | 1.15  |
5.87 (2) | 5.18  |
5.18  |
||
| P | 0.12( * ) | 0.23  |
... | 18.59 (23) | 0.13  |
0.23  |
|
| 0.12( * ) | ... | 2.38  |
21.39 (23) | 0.25  |
0.47  |
||
| M 31-8 J004212.1+411758 | B | 0.12( * ) | 0.43  |
... | 0.28 (2) | 1.75  |
2.15  |
| 0.32( * ) | ... | 2.34  |
1.18 (2) | 2.51  |
6.15  |
||
| P | < 0.19 | 0.73  |
... | 31.21 (23) | 1.37  |
1.48  |
|
0.32  |
... | 1.55  |
24.69 (23) | 2.27  |
3.06  |
||
Notes. Column (1) gives the name of the object in this paper and in 3XMM, (2) time selection of the fit refers to all photons of the observation (A), the burst (B) or persistent (P) emission. Column (3) gives the interstellar absorption; Cols. (4) and (5) give the black-body temperature (kT) or the power law index (Γ) respectively; Col. (6) the goodness of fit measured using the C-statistic and the number of degrees of freedom; Cols. (7) and (8) give an estimate of the absorbed (Fabs) and unabsorbed (Funabs) fluxes in the 0.2–10.0 keV band, respectively. All the errors are given for 90% confidence for one interesting parameter. For the fluxes, the errors are at 68% confidence. ( * ) Values frozen for the fit.
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