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Table 3.

Best-fit values of the spectral models for XMM-Newton data.

Component Model 1 Model 3 Model 4
Edge
EO VIII (keV) 0.871 (fixed) 0.871 (fixed) 0.871 (fixed)
τO VIII 0.7 ± 0.1 0.7 ± 0.1 0.7 ± 0.1

Edge
EFe XXVI (keV) 8.828 (fixed) 8.828 (fixed) 8.828 (fixed)
τFe XXVI 0.05 ± 0.01 0.04 ± 0.01 0.04 ± 0.01

phabs
nH(1022) 2.44 ± 0.04 2.40 ± 0.02 2.42 ± 0.04

diskbb
kTin (keV)
Rdisc (km)
Fbb
(10−9 erg cm−2 s1) 1.3

nthComp
Γ
kTe (keV)
kTseed (keV) 0.7 ± 0.1
Norm 0.08 ± 0.02
FCompt
(10−9 erg cm−2 s1) 2.4

diskline
betor
θ (deg) 35 ± 3
Rin (km)

diskline
EAr XVIII (keV) 3.32 (fixed)
NAr XVIII (×10−4) 4.1 ± 1.2

diskline
ECa XIX (keV) 3.90 (fixed)
NCa XIX (×10−4)

diskline
EFe XXV (keV) 6.81 ± 0.07
NFe XXV (×10−4) 5.7 ± 1.1

rdblur
Betor10 −2.8 (fixed) −2.5 (fixed)
Rin (km)
θ (deg)

gauss
EAr XVIII (keV) 3.32 (fixed) 3.32 (fixed)
NAr XVIII (×10−4)

gauss
ECa XIX (keV) 3.90 (fixed) 3.90 (fixed)
NCa XIX (×10−4)

rfxconv
rel_refl
logξ
χ2(d.o.f.) 2559(2245) 2523(2244) 2550(2245)

Notes. Uncertainties are reported at 90% confidence level. The spectral parameters are defined as in XSPEC. The units of the line normalisations are in photons/cm2 s−1. Fbb and FCompt represent the unabsorbed fluxes in the (0.1–100) keV energy range associated with the accretion disc and the Comptonisation component, respectively.

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