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Table 4.

LP observations best-fit spectral parameters during peak/no-peak phases.

Observation nH(a) kTsoft Norm. kThard Norm. Flux (b) Lum. (c) χ2/d.o.f. n.h.p.
(1020 cm−2) (keV) (keV) (10−4) (10−13 erg cm−2 s−1) (1039 erg s−1)
B
peak 10.0−4.7+5.8 0.31−0.05+0.07 1.1−0.7+2.0 2.7−0.3+0.4 7.0−2.7+3.6 7.4 ± 0.2 7.4 ± 0.2 159.28/162 0.546
no-peak 7.8−3.1+3.5 0.34−0.04+0.05 0.5−0.3+0.5 2.8 ± 0.3 4.0−1.3+1.7 4.67 ± 0.09 4.61 ± 0.09 288.73/255 0.072
C
peak 10.8−4.3+5.1 0.30−0.04+0.05 1.4−0.8+1.9 2.9−0.3+0.4 5.7−2.1+2.8 7.30 ± 0.18 7.46 ± 0.18 175.12/180 0.589
no-peak 5.8−2.6+3.0 0.36−0.04+0.05 0.32−0.15+0.28 2.8−0.2+0.3 4.0−1.1+1.4 4.62 ± 0.08 4.45 ± 0.08 277.37/277 0.482

B+C
peak 10.5−3.2+3.7 0.31−0.03+0.04 1.3−0.6+1.2 2.8−0.2+0.3 6.2−1.7+2.1 7.35 ± 0.13 7.45 ± 0.13 337.69/347 0.63
no-peak 6.6−2.0+2.2 0.35−0.03+0.04 0.39−0.14+0.23 2.76−0.17+0.20 4.0−0.8+1.0 4.64 ± 0.06 4.52 ± 0.06 567.63/537 0.174

Notes. Best-fit parameters of the spectra during the peaks and the minima (no-peak) of the modulation of the latest XMM-Newton observations. For our fits, we considered the same double-disk model as before.

(a)

The Galactic absorption component was fixed to nH, gal = 3.3 × 1020 cm−2 (HI4PI Collaboration 2016).

(b)

Observed flux in the 0.3–10 keV band.

(c)

Unabsorbed luminosity in the 0.3–10 keV band.

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