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Table 2
Best fit results of the summed EPIC-pn spectrum of the 10 XMM-Newton observations performed during the 2009 campaign and of the XMM-Newton observations performed between 2000 and 2006.
| 2009 campaign – summed spectrum – 2 components of theFe K α line | ||||||||||||||
| Narrow Fe Kα | Resolved Fe Kα | Fe xxv | Fe xxvi | Absorption line | ||||||||||
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| Model | Γ | EFe Kα | NFe KαN † | E WFe KαN | σFe KαR | NFe KαR† | E WFe KαR | NFe xxv† | E WFe xxv | NFe xxvi† | E WFe xxvi | Eabs | Nabs† | χ2/d.o.f. |
| (keV) | (phcm-2 s-1) | (eV) | (keV) | (ph cm-2 s-1) | (eV) | (ph cm-2 s-1) | (eV) | (ph cm-2 s-1) | (eV) | (ph cm-2 s-1: eV) | ||||
| (6) | 1.67 ± 0.01 | 6.420 ± 0.010 | 1.5† | 27† | 0.22 ± 0.04 |
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0.21 ± 0.15 | 3.9 ± 2.7 | 0.20 ± 0.13 | 4.2 ± 2.6 | 7.31 ± 0.1 | −0.15 ± 0.12:3.4 ± 2.7 | 1197.9/1190 |
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| 2000–2006 XMM-Newton observations – summed spectrum – 2 components of the Fe K α line | ||||||||||||||
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| (6) | 1.67 ± 0.01 | 6.427 ± 0.014 | 1.5† | 33† |
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<0.47 | <10.4 | 0.37 ± 0.18 | 9.5 ± 4.5 | 7.34 ± 0.05 | −3.6 ± 0.2:10.1 ± 3.8 | 1212.3/1190 |
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