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Table 3

Best fit results of the summed EPIC-pn spectrum of the 10 XMM-Newton observations performed during the 2009 campaign.

2009 campaign – summed spectrum – 2 components of the Fe K α  line
  Narrow Fe Kα Resolved Fe Kα Diskline

Model Γ E Fe   Kα N Fe   KαN E W Fe   KαN σ Fe   KαR N Fe   KαR E W Fe   KαR σ ion. N ion. E W ion. χ2/d.o.f.
(keV) (ph cm-2 s-1) (eV) (keV) (ph cm-2 s-1) (eV) (keV) (ph cm-2 s-1) (eV)
(7) 1.67 ± 0.01 6.416 ± 0.011 1.5 27 1203.5/1192
rin Ndisk E Wion. χ2/d.o.f.
(rg) (ph cm-2 s-1) (eV)
(8) 1.67 ± 0.01 6.425 ± 0.013 1.5 27 1204.7/1192

Notes. Model (7) Broad ionised GaussiaNFeXXVI + Double Fe Kα: Power law + GausFe KαN + GausFe KαR + GausFe KβN + GausFe KβR + GausFeXXV + GausFeXXVI – AbsGaus. Model (8) Ionised-disc-lineFeXXVI + Double Fe Kα: Power law + GausFe KαN + GausFe KαR + GausFe KβN + GausFe KβR + GausFeXXV + GausFeXXVI – AbsGaus.

(†)

In units of 10-5 ph cm-2 s-1.

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