Table 2.
Coverage of GRB 221009A by multiwavelength instruments.
| Bin | t-T0GBM [s] | LHAASO | Fermi/LAT | AGILE | GBM | KONUS |
|---|---|---|---|---|---|---|
| BIN-0 | 232–237 | ✓ | ✗ | ✗ | ✗ | ✓(241–250) |
| BIN-1 | 237–242 | ✓ | ✗ | ✗ | ✗ | ✓ |
| †BIN-2 | 242–247 | ✓ | ✓(244–247) | ✗ | ✗ | ✓ |
| BIN-3 | 247–253 | ✓ | ✓ | ✗ | ✗ | ✗ |
| BIN-4 | 253–259 | ✓ | ✗ | ✗ | ✗ | ✗ |
| BIN-5 | 259–270 | ✓ | ✗ | ✗ | ✗ | ✗ |
| †BIN-6 | 270–308 | ✓ | ✓(277–308) | ✓/ bin-c1 | ✓(277–308) | ✗ |
| †BIN-7 | 308–350 | ✓ | ✓(308–350) | ✗/ bin-c2 | ✓(308–350) | ✗ |
| †BIN-8 | 350–401 | ✓ | ✓(350–401) | ✓(350–401.) | ✗ | |
| BIN-9 | 401–463 | ✓ | ✗ | ✗ | ✓ | ✗ |
| BIN-10 | 463–525 | ✓ | ✗ | ✗ | ✗ | ✗ |
| BIN-11 | 525–600 | ✓ | ✗ | ✗ | ✓ | ✗ |
| †BIN-12 | 600–800 | ✓ | ✗ | ✓(684–834) | ✓(600–800) | ✗ |
| BIN-13 | 800–1000 | ✓ | ✗ | ✗ | ✓ | ✗ |
| †BIN-14 | 1.0–1.35 k | ✓ | ✗ | ✓(1129–1279) | ✓(1000–1350) | ✗ |
Notes. The temporal bins are driven by the observation of LHAASO (1), and are numerically named from BIN-0 to BIN-14. The coverage (/availability) of the other instruments are marked as “✓” in the case of available usable data or “✗” in the case of unavailable data. Fermi/GBM mega-electronvolt data were only selected during the period when there is no pile-up (2). The energy band between 30 MeV and above 100 GeV is covered by both AGILE and Fermi/LAT. The LAT data are preferred for the time bin where it is covered by both AGILE and LAT. In total, six time bins (marked with “†”) are selected, where a kilo-electronvolt–tera-electronvolt spectrum can be constructed. References: 1. Cao et al. (2023); 2. Lesage et al. (2023).
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