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Table A.2

Best-fit parameters of the baseline applied model.

Slice kTa Nbmcb Γc Npexd NHe ξf Fg χ2/d.o.f.

1 3.62 916.63/908
2 3.35 947.22/848
3 4.34 998.94/924
4 6.89 1055.78/1020
5 7.32 1189.27/1109
6 6.78 1264.31/1115
7 5.74 1153.85/1069
8 6.71 1151.00/1105
9 6.77 1141.04/1118
10 6.36 1201.71/1140
11 6.29 1127.48/1085
12 3.78 1342.81/1234
21 3.11 984.13/959
22 2.86 903.21/814
23 3.32 981.42/952
24 2.46 902.52/913
25 2.27 757.83/740
26 3.08 815.43/747
27 2.89 773.01/758
28 3.24 743.77/755
29 3.63 709.54/764
30 4.10 1054.23/1051
31 3.24 1021.00/996
32 2.61 710.66/706
33 2.92 1206.77/1192
34 4.40 608.27/661
35 3.46 1127.82/1150
36 4.26 935.55/923
37 4.08 943.91/948
38 4.42 994.43/956
39 4.48 974.43/902
40 4.65 977.13/915
41 3.40 879.46/809
42 4.26 985.30/1000
43 3.91 955.51/959
44 3.75 1170.01/1163
45 3.10 1055.64/1045
46 2.32 824.40/800
48 2.31 591.83/567
49 2.83 948.39/901
50 3.80 812.27/830

Notes. The missing time intervals (13–20, 47) refer to the occultation episodes which have been neglected.

(a)

BB colour temperature in units of 10-2 keV.

(b)

Normalisation of the BMC component in units of .

(c)

Intrinsic photon index.

(d)

Normalisation of the PEXRAV component in units of 10-2 photons keV-1 cm-2 s-1 at 1 keV.

(e)

Column density of the ZXIPCF component in units of 1022 cm-2.

(f)

Ionisation degree of the ZXIPCF component in units of erg cm s-1.

(g)

0.2–10 keV flux in units of 10-11 erg s-1 cm-2.

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