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Table 2
Best-fit parameters of the total spectrum and the different observations using the Comptonization model compps for the primary continuum and nthcomp for the UV-soft X-rays.
| Obs. | Γwc | k Twc | τwc | k Thc | yhc | τhc | Tbb,wc | Tbb,hc | Npexmon | χ2/d.o.f. | |
| (keV) | (keV) | (eV) | (eV) | ( × 10-3) | |||||||
|
|
|||||||||||
| Total | 2.595 |
0.56 |
18.4 |
123 |
0.63 |
0.65 |
3.4 |
100 |
2.9 | 1387/690 | |
| Obs. 1 | 2.56 |
0.48 |
20.3 |
102 |
0.63 |
0.89 |
2.6 |
97 |
(f) | 396/415 | |
| Obs. 2 | 2.55 |
0.54 |
19.3 |
122 |
0.63 |
0.66 |
2.7 |
95 |
(f) | 510/415 | |
| Obs. 3 | 2.53 |
0.54 |
19.3 |
120 |
0.60 |
0.65 |
2.9 |
108 |
(f) | 501/415 | |
| Obs. 4 | 2.60 |
0.56 |
17.1 |
164 |
0.54 |
0.42 |
3.2 |
102 |
(f) | 500/415 | |
| Obs. 5 | 2.57 |
0.50 |
19.8 |
141 |
0.51 |
0.46 |
3.3 |
105 |
(f) | 467/415 | |
| Obs. 6 | 2.54 |
0.59 |
18.5 |
108 |
0.66 |
0.78 |
2.9 |
116 |
(f) | 518/415 | |
| Obs. 7 | 2.54 |
0.54 |
19.0 |
119 |
0.60 |
0.67 |
2.9 |
104 |
(f) | 513/415 | |
| Obs. 8 | 2.52 |
0.52 |
20.0 |
78 |
0.64 |
1.05 |
2.6 |
114 |
(f) | 494/415 | |
| Obs. 9 | 2.55 |
0.49 |
20.2 |
115 |
0.60 |
0.67 |
3.0 |
100 |
(f) | 450/415 | |
| Obs. 10 | 2.53 |
0.53 |
19.7 |
102 |
0.67 |
0.84 |
2.6 |
108 |
(f) | 409/415 | |
Notes. The optical depth τwc of the warm corona is estimated from eqpair fits (see Appendix A).
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