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Table 6.
He-like and H-like emission lines detected at the 3σ level.
| Line | λobs (Å) | Flux | FWHM (Å) |
|---|---|---|---|
| (ph m−2 s−1) | |||
| Averaged spectrum | |||
| He-like Ne | 13.541![]() |
0.52![]() |
0.07![]() |
| He-like Mg | 9.233![]() |
0.76 ± 0.14 | 0.005 |
| H-like Mg | 8.360![]() |
0.43 ± 0.19 | 0.005 |
| HCR spectrum | |||
| He-like Ne | 13.536![]() |
0.62 ± 0.21 | 0.05![]() |
| H-like Ne | 10.257![]() |
0.57![]() |
0.005 |
| He-like Mg | 9.233![]() |
0.88 ± 0.18 | 0.005 |
| H-like Mg | 8.364![]() |
0.83 ± 0.23 | 0.005 |
| HCR out-of-dips spectrum | |||
| He-like Ne | 13.541![]() |
0.6![]() |
0.01![]() |
| H-like Ne | 10.253![]() |
0.58 ± 0.17 | 0.005 |
| He-like Mg | 9.233![]() |
0.96![]() |
0.005 |
| H-like Mg | 8.364![]() |
0.96 ± 0.24 | 0.005 |
Notes. FWHM was fixed to 0.005 Å except for the He-like Ne. In the LCR spectrum no emission lines, if present, are detected at the 3σ level.
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