Table A.4.
Time-selected Swift/XRT spectroscopy: Results.
| tbabs * zpowerlw (2–10 keV) | |||||
| Γ2 − 10 | F2 − 10 | χ2/d.o.f. | |||
| total |
 |
6.23 | 42.40/48 | ||
| 1st year |
 |
6.55 | 28.15/31 | ||
| 2nd year |
 |
5.84 | 36.08/17 | ||
| pre0 |
 |
6.14 | 17.41/15 | ||
| pre1 |
 |
5.88 | 5.02/3 | ||
| flare |
 |
14.1 | 12.72/20 (70.48) | ||
| plateau |
 |
6.5 | 4.01/4 | ||
| post |
 |
7.15 | 3.49/4 | ||
| tbabs * zpowerlw (0.3–10 keV) | |||||
| Γ0.3 − 10 | F0.3 − 10 | χ2/d.o.f. | |||
| flare |
 |
17.2 | 32.98/37 (98.40) | ||
| tbabs * ztbabs * zpowerlw (0.3–10 keV) | |||||
| NH, z | Γ0.3 − 10 | F0.3 − 10 | χ2/d.o.f. | ||
| total |
 |
 |
8.64 | 142.83/117 | |
| 1st year |
 |
 |
9.00 | 87.05/79 | |
| 2nd year |
 |
 |
8.00 | 70.11/44 | |
| pre0 |
 |
 |
8.57 | 40.80/41 | |
| pre1 |
 |
 |
8.11 | 13.40/12 | |
| flare |
 |
 |
14.4 | 33.96/36 (98.17) | |
| v plateau |
 |
 |
9.95 | 20.99/17 | |
| post |
 |
 |
9.32 | 17.62/16 | |
| tbabs * absori * zpowerlw (0.3–10 keV) | |||||
| NH, z | Γ0.3 − 10 | ξ | F0.3 − 10 | χ2/d.o.f. | |
| total |
 |
 |
 |
8.45 | 128.51/116 |
| 1st year |
 |
 |
 |
8.80 | 83.11/78 |
| 2nd year |
 |
 |
 |
7.81 | 62.08/43 |
| pre0 |
 |
 |
 |
8.35 | 39.50/40 |
| pre1 |
 |
 |
 |
7.73 | 11.98/11 |
| plateau |
 |
 |
 |
9.60 | 19.52/16 |
| 1 post |
 |
 |
 |
8.78 | 14.43/15 |
| tbabs * zpcfabs * zpowerlw (0.3–10 keV) | |||||
| NH, z | f | Γ0.3 − 10 | F0.3 − 10 | χ2/d.o.f. | |
| total |
 |
 |
 |
8.45 | 124.47/116 |
| 1st year |
 |
 |
 |
8.82 | 82.25/78 |
| 2nd year |
 |
 |
 |
7.81 | 59.48/43 |
| pre0 |
 |
 |
 |
8.42 | 39.41/40 |
| pre1 |
 |
 |
 |
7.76 | 12.26/11 |
| plateau |
 |
 |
 |
9.56 | 19.19/16 |
| post |
 |
 |
 |
8.77 | 14.42/15 |
| 1st year |
 |
0.91 | 1.84 ± 0.15 | 8.82 | 82.26/79 |
| 2nd year |
 |
0.91 |
 |
7.84 | 59.50/44 |
| pre0 |
 |
0.91 |
 |
8.42 | 39.42/41 |
| pre1 |
 |
0.91 |
 |
7.65 | 12.38/12 |
| plateau |
 |
0.91 |
 |
9.41 | 19.69/17 |
| post |
 |
0.91 |
 |
8.69 | 14.45/16 |
Notes. The fits are for z = 0.16409 and a fixed 
cm−2 (TBABS). Absorption columns NH, z are in units of ×1021 cm−2, the ionisation parameter, ξ, in units of ×10−2, while the observed fuxes are in units of ×10−13 erg cm−2 s−1. For the flare spectrum, Cash statistics was used and the goodness of fit (g.o.f.) was calculated with 104 simulations. Uncertainties are given at 90 % c.l. for one interesting parameter.
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