Table 3.
X-ray photon indices and model flux from power-law fits to all X-ray spectra.
| Date | Telescope | ΓX | F0.2 − 5.0 keVa |
|---|---|---|---|
| (MJD) | |||
| 58886 | Swift-XRT | 1.90 ± 0.21 | 3.57 ± 0.48 |
| 58895 | Swift-XRT | 1.75 ± 0.36 | 2.66 ± 0.48 |
| 58899 | Swift-XRT | 1.91 ± 0.63 | 2.98 ± 1.00 |
| 58901 | Swift-XRT | 1.69 ± 0.24 | 2.69 ± 0.41 |
| 58907 | Swift-XRT | 1.8 ± 0.2 | 2.08 ± 0.42 |
| 58911 | eROSITA | 1.73 ± 0.34 | 3.06 ± 0.42 |
| 58912 | Swift-XRT | 1.99 ± 0.33 | 3.0 ± 0.6 |
| 58914 | Swift-XRT | 1.90 ± 0.25 | 3.34 ± 0.42 |
| 58916 | Swift-XRT | 1.82 ± 0.41 | 1.79 ± 0.38 |
| 58919 | Swift-XRT | 1.89 ± 0.69 | 0.96 ± 0.28 |
| 59093 | eROSITA | 2.1 ± 0.4 | 0.74 ± 0.21 |
| 59263 | eROSITA | 2.35 ± 0.55 | 0.52 ± 0.15 |
| 59452 | eROSITA | 2.61 ± 1.49 | 0.19 ± 0.12 |
| 59550 | Swift-XRT | 1.72 ± 0.19 | 1.54 ± 0.18 |
| 59651 | XMM-Newton | 1.82 ± 0.03 | 0.48 ± 0.02 |
| 59786 | Swift-XRT | 1.56 ± 0.71 | 0.22 ± 0.09 |
| 60017 | XMM-Newton | 1.76 ± 0.02 | 0.41 ± 0.01 |
Notes. Photon indices and values of 0.2–5.0 keV absorbed flux from the power-law fits to all X-ray spectra. All errors correspond to the 90% confidence limit of the BXA-Ultranest posteriors. The photon indices are mostly moderately flat, with ΓX usually near 1.9. (a) In units of 10−12 erg s−1 cm−2.
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