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Table 3

Best-fit spectral parameters for the emission lines detected in the soft X-ray band.

Energy Intensity Identification
(1) (2) (3)

0.57  ±  0.02 OVII Lyα
0.72  ±  0.01 3.0  ±  1.3  ×  10-5 OVII RRC, Fe XVII 3s-2p
0.84  ±  0.02 2.5  ±  0.7  ×  10-5 Fe XVII-XVIII 3d-2p, OVIII RRC
0.93  ±  0.02 3.3  ±  0.9  ×  10-5 NeIX Heα
1.02 NeX Lyα, Fe XXI 3d-2p
1.14  ±  0.03 9.3  ±  5.8  ×  10-6 Fe XXIII-XXIV L
1.21 1.1  ±  0.5  ×  10-5 NeX Lyβ
1.34  ±  0.02 MgXI Heα
1.50  ±  0.02 MgXII Lyα
1.82  ±  0.02 SXIII Heα
Si XXIV-XVI Lyα
6.2  ±  1.8  ×  10-6 SXV Heα

Notes. See Sect. 3.2 for details. The columns give the following information: (1) energy of the line (keV); (2) intensity of the line (photons cm-2 s-1); (3) likely identification (e.g., Brinkman et al. 2002; Guainazzi & Bianchi 2007).

(†)

indicates that the energy has been fixed to the laboratory energy of NeX Lyα due to the likely superposition of many unresolved Fe lines.

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