Table C.1.
Time-resolved spectral analysis using BBs.
Time | Ep | α | Energy Flux (ℱ) | Liso | Eiso |
---|---|---|---|---|---|
(ms) | (keV) | (×10−6 ergs s−1 cm−2) | (×1045 erg⋅ s−1) | (×1044 erg) | |
GRB 200415A | |||||
-4.3:-3.9 |
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-3.9:-3.4 |
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-3.4:-2.9 |
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-2.9:-2.5 |
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-2.5:-0.5 |
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-0.5:3.0 |
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3.0:5.0 |
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5.0:6.5 |
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6.5:22.5 |
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22.5:65.8 |
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65.8:93.3 |
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93.3:121.2 |
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121.2:150.2 |
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GRB 180128A | |||||
-12.0:-10.0 |
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-10.0:-7.0 |
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-7.0:-3.0 |
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-3.0:-1.0 |
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-1.0:18.0 |
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18.0:143.0 |
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Notes. The BB interval, time-resolved fluence is from fitting the spectrum with a COMPT over a combined (NaI and BGO detectors) spectral range of 8 keV–40 MeV for Fermi/GBM data. The Liso and Eiso values were calculated over the standardized bolometric energy range of 1 keV to 10 MeV. These values are consistent with those found in Roberts et al. (2021) and Trigg et al. (2024).
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