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Table 1.
Estimated EW of Fe XXV (1s2–1s2p) and Fe XXVI (1s–2p) absorption line from model spectra (Sect. 5.1.3) and by fitting fake-spectra with multiple Gaussians (Sect. 5.2.2) for different magnetisations.
| μ | Fe XXV | Fe XXVI | ||||
|---|---|---|---|---|---|---|
| Model spectra | Fake-spectra | Model spectra | Fake-spectra | |||
| XRISM | Athena | XRISM | Athena | |||
| 0.0010 | 6.3 | 6.3 (4.0–8.8) | 6.7 (4.5–8.7) | 27.1 | 31.1 (22.6–39.8) | 27.2 (19.4–35.2) |
| 0.0029 | 5.4 | 4.2 (3.1–5.5) | 6.3 (4.9–7.7) | 22.2 | 20.4 (14.4–26.9) | 28.2 (16.6–41.6) |
| 0.0059 | 3.9 | 4.6 (2.7–6.5) | 4.4 (2.7–5.1) | 18.1 | 19.8 (15.7–23.9) | 18.3 (12.6–23.2) |
| 0.0160 | 3.0 | 2.8 (2.3–3.6) | 3.0 (2.2–3.9) | 16.0 | 15.5 (12.3–18.7) | 16.1 (14.2–18.0) |
| 0.0674 | 3.5 | 3.1 (2.5–3.9) | 3.5 (2.8–4.3) | 16.6 | 15.0 (12.6–17.2) | 17.6 (11.7–23.4) |
Notes. All the EWs are presented in eV. The range in brackets represents the 90% confidence range from fitting.
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