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Table 1

Results of the “averaged ratio flux spectrum” spectral fitting in the 3–10 keV.

Model Power law/pexrav Gaussian Diskline



Γ foldE RDist cosi EKα σKα EWKα EDisk Rin Rout β i EW χ2/d.o.f.
(keV) (Ω/2π) (keV) (keV) (eV) (keV) (Rg) (Rg) (deg) (eV)

Pow + Narrow 1.76 ± 0.02 ... ... ... 6.40* 0.01* 45 ± 13 ... ... ... ... ... ... 31.3/19
Pow + Broad 1.77 ± 0.02 ... ... ... 6.40* 75 ± 40 ... ... ... ... ... ... 25.6/18
Pow + Disk 1.78n ... ... ... ... ... ... 6.40* 6.0* 100.0*  −2.5* 35.3n 128 ± 41 41.6/18

Pow + Narrow + Broad 1.78 ± 0.02 ... ... ... 6.40* 0.01* 28 ± 20 ... ... ... ... ... ...
... ... ... ... 6.40* 73 ± 43 ... ... ... ... ... ... 22.8/17
Pow + Narrow + Disk 1.78 ± 0.02 ... ... ... 6.40* 0.01* 39 ± 14 6.40* 6.0* 100.0*  −2.5* 22.7/17
Pow + pexrav + Narrow + Broad 1.8* 200* 0.27 ± 0.17 0.9* 6.40* 0.01* 28 ± 20 ... ... ... ... ... ...
... ... ... ... 6.40*  < 105 ... ... ... ... ... ... 21.6/17
Pow + pexrav + Narrow + Disk 1.8* 200* 0.24 ± 0.17 0.9* 6.40* 0.01* 37 ± 14 6.40* 6.0* 100.0*  −2.5* 45.5 ± 3.5  <137 21.5/17

Notes. All errors and upper limits refer to the 68% confidence range for a single parameter. In all the spectral fits, the errors in the Fe lines EW are calculated using XSPEC eqw with err option.

(*)

Denotes fixed parameter.

(n)

Error calculation is not possible due to poor fit.

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