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Table 2.

Parameters for the best-fit model including fully covering ionised absorption and Gaussian lines.

Component Parameter Obs. 1 Obs. 2
TBabs NH 0.056 0.056

power-law Γ 1.66 ± 0.04 2.05 ± 0.10
Norm (×10−3) 0.64 ± 0.1 1.4 ± 0.2

WA log ξ 2.00 ± 0.04 1.75 ± 0.15
NH 7.9 ± 0.9 5.4 ± 0.4
z 0.096
Δχ2/d.o.f. 642/2 1616/2

zgauss (Emi) E (keV) 0.56 ± 0.02 0.59 ± 0.02
z 0.096
Norm (×10−4) 1.4 ± 0.4 2.6 ± 1.0
EW (eV) 70 ± 30 45 ± 25
Δχ2/d.o.f. 18/2 31/2

zgauss (Emi) E (keV) 6.30 ± 0.8
z 0.096
Norm (×10−6) 5.0 ± 2.0
EW (eV) 130 ± 90 125 ± 80
Δχ2/d.o.f. 18/2

zgauss (Abs) E (keV) 6.80 ± 0.07
z 0.096
Norm (×10−6) −3.5 ± 1.2
EW (eV) −100 ± 50 −100 ± 50
Δχ2/d.o.f. 11/2

zgauss (Abs) E (keV) 8.2 ± 0.2
σ (eV) 200
z 0.096
Norm (×10−6) −5.4 ± 3.1
EW (eV) −220 ± 120
Δχ2/d.o.f. 8/2

Notes. The power law normalisation (normalised at 1 keV) is in units of photons keV−1 cm−2 s−1, while units for the column density and ionisation parameter are 1022 cm−2 and erg s−1 cm, respectively. The normalisation of emission and absorption lines are in photons cm−2 s−1. Finally, a is used to identify the parameters kept frozen during the fit while the specifies the component whose parameters were tied between the observations.

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