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Table 3.
Best-fit parameters for the continuum model of the extracted spectra.
| OBSID | Orbital phase | NH | Γ | Flux | Luminosity | χ2/d.o.f. |
|---|---|---|---|---|---|---|
| (1022 cm−2) | – | (10−12 erg s−1 cm−2) | (1036 erg s−1) | – | ||
| 76 | −0.376 ± 0.019 | 5.48 |
0.55 |
95.5 |
1.76 |
1.39/174 |
| 77 | −0.155 ± 0.016 | 36.06 |
0.27 |
55.0 |
1.01 |
1.03/97 |
| 74a | 0.074 ± 0.018 | 0.17 |
0.02 |
1.0 |
0.019 |
1.19/23 |
| 74b | 0.109 ± 0.018 | 14.70 |
0.66 |
54.5 |
1.00 |
1.13/61 |
| 74c | 0.144 ± 0.018 | 5.99 |
0.86 |
61.1 |
1.13 |
1.10/135 |
| 26 | 0.188 ± 0.009 | 8.0 |
0.76 |
65.7 |
1.21 |
1.09/82 |
| 78 | 0.237 ± 0.008 | 0.99 |
1.01 |
75.7 |
1.39 |
0.90/155 |
| 75 | 0.377 ± 0.018 | 2.25 |
0.79 |
57.4 |
1.06 |
1.09/168 |
Notes. Both unabsorbed NTHCOMP flux and luminosity were calculated between 0.5–12 keV. A luminosity distance of 12.4 kpc is adopted (Torrejón et al. 2010).
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