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Table 6
Fitted parameters for the iron emission lines and for the recombination emission lines of He- and H-like species detected in the eclipse spectra (Fig. 6).
| Component | Parameter | 2PL |
|
|
||
| Fluorescence | Energy (keV) |
|
| iron line | σ (eV) | ≤10 |
| EW (eV) |
|
|
| Identification | Fe Kα I–XVII | |
| Recombination | Energy (keV) |
|
| emission lines | σ (eV) | ≤49 |
| EW (eV) |
|
|
| Identification | Fe XXV | |
| Energy (keV) |
|
|
| σ (eV) | ≤18 | |
| EW (eV) |
|
|
| Identification | S XV Heα | |
| Energy (keV) |
|
|
| σ (eV) | ≤280 | |
| EW (eV) |
|
|
| Identification | Si XIV Lyα | |
| Energy (keV) |
|
|
| σ (eV) | ≤103 | |
| EW (eV) |
|
|
| Identification | Si XIII Heα | |
| Energy (keV) | 1.34 (fixed) | |
| σ (eV) | 30 (fixed) | |
| EW (eV) | ≤14 | |
| Identification | Mg Kα, Mg XI Heα | |
| C-statistic (d.o.f.) | 5148(3373) | |
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