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Table 2.

Results of the fit of the time-averaged EPIC spectra.

Model pl + bb + 3 Gaussian pl + bb + apec + 2 Gaussian pl + bb + apec + 2 Gaussian
parameter (fixed abundance) (free abundance)
(10−21 cm−2) 1.16 ± 0.13
Γ 0.76 ± 0.01 0.76 ± 0.02
FluxPL (0.2–12 keV, ×10−11erg cm−2 s−1) 7.78 ± 0.06 7.78 ± 0.06
kTBB (eV)
RBB (km)
FluxBB (0.2–12 keV, ×10−12erg cm−2 s−1) 3.0 ± 0.3 2.8 ± 0.3
kTAPEC (keV)
Abundance (apec) 0.2 (fixed)
NAPEC (×10−3 cm−5)
FluxAPEC (0.2–12 keV, ×10−13erg cm−2 s−1)
Emission lines
Eline1 (keV) 0.97 ± 0.03
σline1 (keV)
Fluxline1 (×10−5 ph cm−2 s−1)
EWline1 (eV)
Eline2 (keV)
σline2 (keV) <0.04 0 (fixed) 0 (fixed)
Fluxline2 (×10−5 ph cm−2 s−1)
EWline2 (eV) 5 ± 3
Eline3 (keV)
σline3 (keV) 0 (fixed) 0 (fixed) 0 (fixed)
Fluxline3 (×10−5 ph cm−2 s−1) 1.3 ± 0.7 1.2 ± 0.7
EWline3 (eV) 18 ± 11 18 ± 11 18 ± 9
FluxBB/FluxTOT (0.01–12 keV) 3.8% 3.5% 3.6%
FluxAPEC/FluxTOT (0.01–12 keV) 1.4% 1.3%
Unabsorbed flux (0.2–12 keV, ×10−11erg cm−2 s−1)
Luminosity (0.2–12 keV, ×10−37erg s−1)
/d.o.f. 1.05/1204 1.05/1206 1.06/1205

Notes. The double-component continuum consists of a power-law and a black-body model, while the broad feature at 0.9–1 keV is described with either a broad Gaussian line or an APEC model. Both a fixed and a free value of the metal abundance are considered in the second case. In addition, two narrow Gaussian lines are needed to account for the positive residuals in the spectrum.

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