Table 3
Same as Table 2 but for the orbital phase resolved spectral analysis.
| Parameter | Value | |||
|
|
||||
| (units) | Steady emission | Phase 0.0–0.2 | Phase 0.2–0.4 | Phase 0.4–0.6 |
|
|
||||
| NH (1022cm-2) |
|
5.6 ± 0.1 | 5.5 ± 0.2 |
|
| E1 (keV) |
|
|
|
|
| σ1 (keV) | 0.0 † | 0.0 † | 0.0 † | 0.0 † |
| EW1 (keV) |
|
−0.014 ± 0.08 |
|
−0.026 ± 0.008 |
| E2 (keV) |
|
2.52 ± 0.06 |
|
|
| σ2 (keV) |
|
|
|
|
| EW2 (keV) |
|
−0.048 ± 0.015 | −0.047 ± 0.013 |
|
| E3 (keV) |
|
– | 3.21 ± 0.06 |
|
| σ3 (keV) |
|
– |
|
0.0 † |
| EW3 (keV) |
|
– |
|
−0.011 ± 0.06 |
| E4 (keV) |
|
|
|
|
| σ4 (keV) |
|
0.0 † | 0.0 † | 0.0 † |
| EW4 (keV) |
|
−0.012 ± 0.05 | −0.014 ± 0.07 | −0.017 ± 0.007 |
| E5 (keV) |
|
– | – | – |
| σ5 (keV) |
|
– | – | – |
| EW5 (keV) |
|
– | – | – |
| E6 (keV) |
|
5.67 ± 0.04 |
|
5.92 ± 0.06 |
| σ6 (keV) | 0.0 † | 0.0 † | 0.0 † | 0.0 † |
| EW6 (keV) |
|
−0.021 ± 0.08 |
|
−0.022 ± 0.010 |
| E7 (keV) |
|
6.20 ± 0.06 | 6.18 ± 0.04 | – |
| σ7 (keV) |
|
0.0 † | 0.0 † | – |
| EW7 (keV) |
|
−0.022 ± 0.012 |
|
– |
| E8 (keV) | 6.72 ± 0.01 | 6.68 ± 0.02 | 6.71 ± 0.02 |
|
| σ8 (keV) | 0.0 † | 0.0 † | 0.0 † | 0.0 † |
| EW8 (keV) | −0.14 ± 0.03 | −0.12 ± 0.02 |
|
−0.11 ± 0.02 |
| E9 (keV) | 7.00 ± 0.03 | 6.96 ± 0.03 |
|
|
| σ9 (keV) | 0.0 † | 0.0 † | 0.0 † | 0.0 † |
| EW9 (keV) | −0.08 ± 0.02 | −0.11 ± 0.02 | −0.11 ± 0.02 | −0.064 ± 0.022 |
| E10 (keV) |
|
7.86 ± 0.05 | 7.89 ± 0.04 |
|
| σ10 (keV) | 0.0 † | 0.0 † | 0.0 † | 0.0 † |
| EW10 (keV) |
|
|
−0.10 ± 0.03 | −0.11 ± 0.03 |
| Egabs (keV) | 9.5 ± 0.2 |
|
|
|
| σgabs (keV) |
|
0.9 ± 0.2 |
|
|
| S gabs |
|
|
|
|
| kTdiskbb(keV) |
|
1.32 ± 0.02 |
|
1.26 ± 0.03 |
| N diskbb |
|
7.3 ± 0.6 |
|
|
F0.5−10 keV
( ) |
|
1.43 ± 0.01 |
|
1.55 ± 0.03 |
| χ2/ν (d.o.f) | 1.41 (101) | 1.27 (104) | 1.34 (103) | 1.34 (103) |
| Exposure time (s) | 16780 | 6564 | 6478 | 4943 |
Notes. We repeat here the first column in order to facilitate the comparison between the results of the averaged steady emission and those obtained from the phase resolved spectral analysis. We excluded from the orbital phase resolved spectral analysis the phases corresponding to the eclipses and the dips (see text for details).
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