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Table 1

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

2009 campaign – summed spectrum – 1 component of the Fe K α  line
  Fe Kα Fe Kβ Fe xxv Fe xxvi

Model Γ EFe   Kα σFe   Kα NFe   Kα E WFe   Kα E WFe   Kβ NFe   xxv E WFe   xxv NFe   xxvi E WFe   xxvi χ2/d.o.f.
(keV) (keV) (ph cm-2 s-1) (eV) (eV) (ph cm-2 s-1) (eV) (ph cm-2 s-1) (eV)
(1) 1.66 ± 0.01 6.43 ± 0.01 0.14 ± 0.02 3.8 ± 0.3 70 ± 5   1311.7/1194
(2) 1.66 ± 0.01 6.43 ± 0.01 0.14 ± 0.02 3.8 ± 0.3 70 ± 5 20 ± 3 ⋄    1244.8/1193
(3) 1.66 ± 0.01 6.415 ± 0.012 0.092 ± 0.012 10.4‡ 9.8 6 1219.8/1192
  Fe Kα Fe Kβ Diskline

Γ EFe   Kα σFe   Kα NFe   Kα E WFe   Kα E WFe   Kβ Incl. Emissiv. Ndiskline E Wdiskline χ2/d.o.f.
(deg.) (ph cm-2 s-1) (eV)
(4) 1.67 ± 0.01 6.415 ± 0.011 0.084 ± 0.015 2.7 ± 0.2 50.0 ± 3.8 8.2‡ 1.7 ± 0.5 36 ± 10 1216.0/1191
(5) 1.67 ± 0.01 6.425 ± 0.011 0.094 ± 0.018 2.9 ± 0.3 8.6‡  −2.8 ± 0.3 1219.4/1191

Notes.  ⋄ : assuming σFe   Kβ = σFe   Kα; ‡: assuming σFe   Kβ = σFe   Kα and NFe   Kβ = 0.15 × NFe   Kα; †: in units of 10-5 ph cm-2 s-1. Model (1) Single Fe Kα: Power law + GausFe Kα. Model (2) Single Fe Kα + β: Power law + GausFe Kα + GausFe Kβ. Model (3) Photo-ionised gas + Single Fe Kα + β: Power law + GausFe Kα + GausFe Kβ + GausFeXXV + GausFeXXVI. Model (4) Broad lineFeXXV + Single Fe Kα + β: Power law + GausFe Kα + GausFe Kβ + DisklineFeXXV. Model (5) Broad lineFeXXVI + Single Fe Kα + β: Power law + GausFe Kα + GausFe Kβ + DisklineFeXXVI.

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