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Table 1.

Time-resolved spectral analysis using BB.

Time Ep α Energy flux (ℱ) Liso Eiso
(ms) (keV) (×10−6 ergs s−1 cm−2) (×1047 erg⋅ s−1) (×1045 erg)
GRB 180128A

−12:−10 250 ± 50 6.0 ± 4.9 17.1 ± 4.6 0.28 ± 0.08 0.06 ± 0.02
−10:−7 (Peak 1) 560 ± 140 0.7 ± 0.6 64.5 ± 9.5 1.1 ± 0.2 0.32 ± 0.05
−7:−3 400 ± 120 8.2 ± 13.2 10.3 ± 4.1 0.17 ± 0.07 0.07 ± 0.03
−3:−1 (Peak 2) 490 ± 150 0.7 ± 0.8 50 ± 10 0.75 ± 0.17 0.15 ± 0.03
−1:18 190 ± 20 4.9 ± 2.3 3.7 ± 0.7 0.060 ± 0.010 0.12 ± 0.02
18:143 120 ± 30 1.6 ± 1.7 0.40 ± 0.11 0.007 ± 0.002 0.08 ± 0.02
TBB duration (155): 290 ± 50 0.6 ± 0.5 2.4 ± 0.4 0.039 ± 0.007 0.60 ± 0.10

GRB 200415A

−4.3:−3.9 (Peak 1) 320 ± 50 0.5 ± 0.4 170 ± 20 2.7 ± 0.4 0.11 ± 0.02
−3.9:−3.4 1100 ± 700 −0.8 ± 0.3 120 ± 60 2.0 ± 0.9 0.10 ± 0.05
−3.4:−2.9 (Peak 2) 800 ± 130 −0.1 ± 0.2 490 ± 80 8.0 ± 1.3 0.40 ± 0.07
−2.9:−2.5 (Peak 3) 1100 ± 200 −0.50 ± 0.14 850 ± 140 14 ± 2 0.56 ± 0.10
−2.5:−0.5 ( † ) 1210 ± 120 −0.1 ± 0.1 630 ± 60 10.5 ± 1.0 2.1 ± 0.2
−0.5:3.0 2040 ± 180 −0.16 ± 0.08 600 ± 50 10.0 ± 1.0 3.4 ± 0.3
3.0:5.0 ( * ) 900 ± 200 0.1 ± 0.3 110 ± 30 1.8 ± 0.4 0.36 ± 0.07
5.0:6.5 ( * ) Completely in the data gap
6.5:22.5 ( * ) 1040 ± 80 0.8 ± 0.2 124 ± 9 2.0 ± 0.2 3.3 ± 0.2
22.5:65.8 830 ± 50 0.46 ± 0.13 51 ± 3 0.84 ± 0.05 3.7 ± 0.2
65.8:93.4 590 ± 70 0.3 ± 0.2 19 ± 2 0.31 ± 0.03 0.85 ± 0.09
93.4:121.2 430 ± 50 0.8 ± 0.4 9.7 ± 1.1 0.16 ± 0.02 0.44 ± 0.05
121.2:150.3 250 ± 40 0.9 ± 0.6 3.1 ± 0.5 0.051 ± 0.007 0.15 ± 0.02

TBB duration (155) ( † †): 998 ± 40 0.04 ± 0.05 56 ± 2 0.91 ± 0.04 14.2 ± 0.5

GRB 150101B

−16:−8 (Peak 1) 1100 ± 600 −0.4 ± 0.4 16 ± 7 8000 ± 4000 6000 ± 3000
−8:−2 (Peak 1) 220 ± 70 −0.8 ± 0.3 6.3 ± 1.3 3200 ± 700 1900 ± 400
−2:4 61 ± 12 0.3 ± 1.2 1.4 ± 0.3 730 ± 150 440 ± 90
4:74 25 ± 6 −0.8 ± 1.0 0.35 ± 0.05 180 ± 30 1300 ± 200

TBB duration (90): 150 ± 80 −1.5 ± 0.2 1.1 ± 0.2 550 ± 120 4100 ± 900

Notes. The fluence is from fitting the spectrum with a Comptonized function over a combined (NaI and BGO detectors) spectral range of 8 keV–40 MeV.

( † )Includes the saturated portion of the spectrum from about T0 − 2.4 to −0.8 ms.

( * )Includes the data gap, from about T0 + 4.6 to 6.6 ms.

( † †)This does not include the correction for the brightest part of the event that was saturated in Fermi/GBM as in Roberts et al. (2021), which accounts for the lower values in this study.

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