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Table 3

Fitted parameters during the peak of bursts by different models.

Double-blackbody model fa model Disk reflection model
Burst # (keV) (km) (keV) (km) (keV) (km)
1 5.2 ± 1.4 0.59 ± 0.02 151 ± 9 4.1 ± 0.7 5.5 ± 1.4 0.45 ± 0.02 154±10 4.5 ± 1.4 3.9 ± 0.1 0.62 ± 0.01 126±10 3.9 ± 0.2
2 5.1 ± 1.2 0.95 ± 0.04 55 ± 5 4.9 ± 0.7 5.5 ± 0.5 0.93 ± 0.11 33 ± 8 4.2 ± 0.3 3.6 ± 0.2 0.90 ± 0.03 55 ± 4 3.6 ± 0.2
3 4.7 ± 0.3 0.51 ± 0.02 192±14 3.4 ± 0.6 5.7 ± 0.5 0.38 ± 0.02 215 ± 25 4.4 ± 0.3 4.2 ± 0.2 0.53 ± 0.02 157±14 3.4 ± 0.2
4 5.0 ± 0.6 0.59 ± 0.02 142 ± 9 3.3 ± 0.5 6.1 ± 0.4 0.47 ± 0.02 143 ± 12 4.1 ± 0.3 3.9 ± 0.1 0.63 ± 0.02 116±7 3.3 ± 0.1
5 4.9 ± 1.2 0.68 ± 0.02 108 ± 8 4.8 ± 0.9 5.0 ± 0.4 0.60 ± 0.07 72 ± 10 4.0 ± 0.4 3.5 ± 0.2 0.70 ± 0.02 92 ± 6 3.5 ± 0.2
6 5.8 ± 0.3 0.42 ± 0.01 284 ± 16 5.8 ± 0.3 6.1 ± 0.3 0.37 ± 0.01 284 ± 21 6.1 ± 0.3 5.0 ± 0.2 0.42 ± 0.01 271 ± 15 5.0 ± 0.2
7 5.3 ± 1.3 0.35 ± 0.02 340 ± 23 5.3 ± 1.0 5.9 ± 0.4 0.27 ± 0.01 397 ± 36 4.7 ± 0.4 4.3 ± 0.2 0.33 ± 0.01 331 ± 22 4.3 ± 0.2
8 5.0 ± 0.9 0.20 ± 0.01 1012 ± 53 5.0 ± 0.8 4.6 ± 0.4 0.17 ± 0.01 1318 ± 95 4.5 ± 0.2 4.5 ± 0.2 0.13 ± 0.02 1484 ± 105 4.5 ± 0.2
9 4.7 ± 1.0 0.49 ± 0.02 195 ± 19 4.7 ± 0.8 3.6 ± 0.1 0.39 ± 0.01 250 ± 18 3.5 ± 0.3 3.7 ± 0.1 0.50 ± 0.02 166 ± 20 3.7 ± 0.1
10 5.0 ± 0.7 0.40 ± 0.01 317 ± 17 4.4 ± 0.6 5.3 ± 0.3 0.36 ± 0.01 309 ± 24 4.4 ± 0.2 4.1 ± 0.2 0.40 ± 0.02 301 ± 19 4.1 ± 0.2
11 4.9 ± 0.9 0.45 ± 0.01 252 ± 13 4.9 ± 0.8 4.7 ± 0.8 0.40 ± 0.01 253 ± 13 4.7 ± 0.8 4.3 ± 0.1 0.48 ± 0.01 226 ± 13 4.3 ± 0.1
12 5.4±1.2 0.49 ± 0.01 219 ± 12 5.4 ± 0.9 5.3 ± 1.1 0.45 ± 0.02 166 ± 23 5.0 ± 0.3 5.0 ± 0.2 0.49 ± 0.02 103 ± 11 5.0 ± 0.2
13 4.8 ± 0.3 0.52 ± 0.02 201 ± 12 3.6 ± 0.5 4.6 ± 0.2 0.39 ± 0.02 198 ± 15 4.2 ± 0.3 4.5 ± 0.2 0.54 ± 0.02 175 ± 13 3.9 ± 0.1
14 4.9 ± 0.3 0.44 ± 0.01 243 ± 13 4.8 ± 0.9 4.7 ± 0.3 0.40 ± 0.01 256 ± 17 4.3 ± 0.3 4.4 ± 0.1 0.46 ± 0.01 238 ± 11 4.0 ± 0.1
15 5.2 ± 0.2 0.43 ± 0.01 256 ± 14 4.4 ± 0.8 5.1 ± 0.4 0.40 ± 0.01 255 ± 18 4.3 ± 0.3 4.4 ± 0.1 0.45 ± 0.02 193 ± 19 4.2 ± 0.1

Notes. (a)The bolometric peak flux of each burst in units of 10−8 erg s−1cm−2. (b)The minimum blackbody temperature of each burst. (c)The maximum blackbody radii. (d)The bolometric touchdown flux in units of 10−8 erg s −1cm−2.

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