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Table 2.

Fit parameters of the most relevant fits to the phase-averaged spectrum.

Parameter WOF TS X TS Y TS Z
NH, 1 [1022 cm−2] 30.0 ± 1.3 24 . 8 5.4 + 1.6 $ 24.8^{+1.6}_{-5.4} $ 41 ± 4 25 . 8 1.6 + 2.0 $ 25.8^{+2.0}_{-1.6} $
NH, 2 [1024 cm−2] 2 . 94 0.34 + 0.28 $ 2.94^{+0.28}_{-0.34} $ 2 . 59 0.74 + 0.30 $ 2.59^{+0.30}_{-0.74} $ 1 . 93 0.26 + 0.32 $ 1.93^{+0.32}_{-0.26} $ 2 . 69 0.19 + 0.22 $ 2.69^{+0.22}_{-0.19} $
fpcf 0 . 514 0.029 + 0.028 $ 0.514^{+0.028}_{-0.029} $ 0 . 64 0.05 + 0.14 $ 0.64^{+0.14}_{-0.05} $ 0 . 543 0.030 + 0.034 $ 0.543^{+0.034}_{-0.030} $ 0 . 46 0.05 + 0.04 $ 0.46^{+0.04}_{-0.05} $
F1 [keV s−1 cm−2] (a) 11.7 ± 0.6 7 . 0 0.7 + 0.5 $ 7.0^{+0.5}_{-0.7} $ 10 . 6 0.4 + 0.6 $ 10.6^{+0.6}_{-0.4} $ 16 . 8 0.9 + 1.6 $ 16.8^{+1.6}_{-0.9} $
Γ 0 . 28 0.16 + 0.15 $ 0.28^{+0.15}_{-0.16} $ 0 . 94 0.19 + 0.08 $ 0.94^{+0.08}_{-0.19} $ 0.35 ± 0.09 0 . 59 0.12 + 0.13 $ 0.59^{+0.13}_{-0.12} $
Efold [keV] 6 . 50 0.18 + 0.20 $ 6.50^{+0.20}_{-0.18} $ 7 . 0 1.7 + 0.5 $ 7.0^{+0.5}_{-1.7} $ 6 . 1 0.7 + 0.4 $ 6.1^{+0.4}_{-0.7} $ 6 . 39 0.29 + 0.38 $ 6.39^{+0.38}_{-0.29} $
Ecutoff [keV] 14 . 2 2.6 + 2.5 $ 14.2^{+2.5}_{-2.6} $ 22 . 2 2.2 + 10.7 $ 22.2^{+10.7}_{-2.2} $ 20 . 1 2.9 + 5.1 $ 20.1^{+5.1}_{-2.9} $ 16 . 8 1.7 + 2.1 $ 16.8^{+2.1}_{-1.7} $
NBB(b) 1 . 19 0.24 + 0.30 $ 1.19^{+0.30}_{-0.24} $ 8 5 + 93 $ 8^{+93}_{-5} $ 67 29 + 34 $ 67^{+34}_{-29} $ 1 . 7 0.8 + 1.5 $ 1.7^{+1.5}_{-0.8} $
TBB [keV] 0 . 439 0.033 + 0.028 $ 0.439^{+0.028}_{-0.033} $ 0 . 25 0.06 + 0.04 $ 0.25^{+0.04}_{-0.06} $ 0 . 264 0.016 + 0.022 $ 0.264^{+0.022}_{-0.016} $ 0 . 341 0.030 + 0.050 $ 0.341^{+0.050}_{-0.030} $
AFe Kα [10−3 ph s−1 cm−2] 9.78 ± 0.12 6 . 2 0.4 + 0.7 $ 6.2^{+0.7}_{-0.4} $ 10.32 ± 0.19 12 . 4 0.6 + 0.4 $ 12.4^{+0.4}_{-0.6} $
AFe Kβ [10−3 ph s−1 cm−2] 0.84 ± 0.10 0 . 62 0.15 + 0.17 $ 0.62^{+0.17}_{-0.15} $ 0.96 ± 0.14 1 . 41 0.29 + 0.20 $ 1.41^{+0.20}_{-0.29} $
ASE [10−3 ph s−1 cm−2] 8 . 0 1.2 + 1.0 $ 8.0^{+1.0}_{-1.2} $ 2 . 0 1.0 + 2.9 $ 2.0^{+2.9}_{-1.0} $ 6 . 4 0.8 + 0.7 $ 6.4^{+0.7}_{-0.8} $ 5 . 8 2.3 + 1.9 $ 5.8^{+1.9}_{-2.3} $
ESE [keV] 6.289 ± 0.021 6 . 16 0.13 + 0.10 $ 6.16^{+0.10}_{-0.13} $ 6.310 ± 0.027 6 . 28 0.06 + 0.05 $ 6.28^{+0.05}_{-0.06} $
σSE [keV] 0 . 61 0.06 + 0.05 $ 0.61^{+0.05}_{-0.06} $ 0 . 23 0.14 + 0.20 $ 0.23^{+0.20}_{-0.14} $ 0 . 51 0.04 + 0.05 $ 0.51^{+0.05}_{-0.04} $ 0 . 42 0.17 + 0.13 $ 0.42^{+0.13}_{-0.17} $
ECRSF1 [keV] 37 . 4 1.0 + 1.1 $ 37.4^{+1.1}_{-1.0} $ 37 . 9 1.5 + 1.8 $ 37.9^{+1.8}_{-1.5} $ 38 . 0 2.2 + 1.4 $ 38.0^{+1.4}_{-2.2} $ 37 . 3 1.5 + 1.7 $ 37.3^{+1.7}_{-1.5} $
σCRSF1 [keV] 6 . 6 0.9 + 1.3 $ 6.6^{+1.3}_{-0.9} $ 7 . 3 1.9 + 4.2 $ 7.3^{+4.2}_{-1.9} $ 10 . 0 2.5 + 3.1 $ 10.0^{+3.1}_{-2.5} $ 6 . 9 1.5 + 2.2 $ 6.9^{+2.2}_{-1.5} $
dCRSF1 [keV] 5 . 5 1.5 + 2.4 $ 5.5^{+2.4}_{-1.5} $ 5 . 2 2.6 + 24.9 $ 5.2^{+24.9}_{-2.6} $ 14 8 + 17 $ 14^{+17}_{-8} $ 5 . 8 2.7 + 5.3 $ 5.8^{+5.3}_{-2.7} $
ECRSF2 [keV] 51 . 5 1.0 + 1.1 $ 51.5^{+1.1}_{-1.0} $ 50 . 8 1.0 + 1.3 $ 50.8^{+1.3}_{-1.0} $ 52 . 5 1.6 + 2.1 $ 52.5^{+2.1}_{-1.6} $ 51 . 3 2.4 + 2.3 $ 51.3^{+2.3}_{-2.4} $
σCRSF2 [keV] 5 . 1 0.8 + 1.0 $ 5.1^{+1.0}_{-0.8} $ 3 . 6 1.0 + 1.5 $ 3.6^{+1.5}_{-1.0} $ 5 . 0 1.2 + 1.8 $ 5.0^{+1.8}_{-1.2} $ 4 . 9 1.6 + 1.9 $ 4.9^{+1.9}_{-1.6} $
dCRSF2 [keV] 7 . 7 2.2 + 3.2 $ 7.7^{+3.2}_{-2.2} $ 5 . 2 2.0 + 3.8 $ 5.2^{+3.8}_{-2.0} $ 6 . 9 3.0 + 6.4 $ 6.9^{+6.4}_{-3.0} $ 6 4 + 6 $ 6^{+6}_{-4} $
CFPMB 1.0035 ± 0.0011 1.0006 ± 0.0023 1.0030 ± 0.0020 1.0036 ± 0.0017
gFPMA [eV] −32.2 ± 2.0 18 14 + 8 $ -18^{+8}_{-14} $ −32.1 ± 2.9 28 5 + 7 $ -28^{+7}_{-5} $
gFPMB [eV] −61.2 ± 2.0 48 14 + 8 $ -48^{+8}_{-14} $ −59.1 ± 2.9 59 5 + 7 $ -59^{+7}_{-5} $

37(c) 2 . 83 0.13 + 0.14 $ 2.83^{+0.14}_{-0.13} $ 1 . 69 0.17 + 0.11 $ 1.69^{+0.11}_{-0.17} $ 2 . 55 0.10 + 0.13 $ 2.55^{+0.13}_{-0.10} $ 4 . 06 0.21 + 0.38 $ 4.06^{+0.38}_{-0.21} $
χ2/d.o.f. 720/477 445/437 588/445 494/451
χ red 2 $ \chi^2_\mathrm{red} $ 1.51 1.02 1.32 1.10

Notes. We show the parameters of the fit to the whole observation and the three time segments.

(a)

Unabsorbed flux of the continuum and blackbody in the energy range of 5–50 keV.

(b)

Relative norm of the blackbody component with respect to the powerlaw component.

(c)

Luminosity in units of 1037erg s−1 in the energy range of 5–50 keV and observer’s frame.

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