Table 2.
Implied magnetic field strength for three different epochs following the method given by Gao & Li (2021).
| MJD | L(a) | ṁ(b) | P(c) | Ṗ(d) | Low B |
High B |
||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| RM/Rsph | B(e) | Lcrit(f) | RM/Rsph | B(e) | Lcrit(f) | |||||||
| Epoch 1 | Case 1 | 52690.67 | 6.73 | 64.68 | 1.43 | −0.81 | 0.16 | 0.31 | 0.08 | 0.92 | 26.63 | 188.82 |
| Case 2 | 0.16 | 0.31 | 0.08 | 1.05 | 45.96 | 249.53 | ||||||
| Epoch 2 | Case 1 | 56847.95 | 9.34 | 75.14 | 1.14 | −2.04 | 0.40 | 3.68 | 14.08 | 0.61 | 12.43 | 95.96 |
| Case 2 | 0.38 | 3.36 | 11.96 | 0.73 | 25.89 | 223.80 | ||||||
| Epoch 3 | Case 1 | 59053.74 | 5.95 | 61.14 | 1.03 | −1.32 | 0.40 | 2.27 | 7.26 | 0.73 | 12.08 | 105.02 |
| Case 2 | 0.39 | 2.16 | 6.62 | 0.86 | 23.97 | 223.06 | ||||||
Notes. The values for L, ṁ, and P are based on the observation at the given date (MJD). We note that for epoch 1, we do not know if the given luminosity is representative of the average luminosity during this epoch, due to the lack of X-ray flux monitoring during that time.
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