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 | ||||||||
|
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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 |
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10.4‡ |
![]() |
9.8 |
![]() |
6 | 1219.8/1192 |
Fe Kα | Fe Kβ | Diskline | |||||||||
|
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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‡ |
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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 |
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8.6‡ |
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−2.8 ± 0.3 |
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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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