Table 1.
Integration times used for the reconstruction of HXR images shown in Fig. 5.
| Peak no. | Time range | Integration | Counts above |
|---|---|---|---|
| (UT at Earth) | time (s) | background (20−76 keV) | |
| 1 | 17:30:32.2–17:30:41.2 | 9 | 23 098 |
| 2 | 17:30:39.2–17:30:50.2 | 11 | 28 887 |
| 3 | 17:30:48.2–17:30:57.2 | 9 | 25 638 |
| 4 | 17:30:55.2–17:31:04.2 | 9 | 27 097 |
| 5 | 17:31:02.2–17:31:12.2 | 10 | 29 961 |
| 6 | 17:31:11.2–17:31:24.2 | 13 | 31 637 |
Notes. They correspond to the FWHM time ranges for the Gaussian components fit in Collier et al. (2023). The total counts above background in the 20−76 keV energy range for each interval is given.
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