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Table 3

Best–fitting model along with means and standard deviations of the parameters’ posterior distributions for each GRB of the sample of 215 events in the 1550 keV energy band.

GRB Model log N log fb α B p(TR) a p AD b p KS c
(Hz)

050117 PL −0.277 ± 0.061 NA 1.355 ± 0.062 1.911 ± 0.026 0.305 0.749 0.752
050124 PL 0.125 ± 0.247 NA 3.012 ± 0.590 1.993 ± 0.133 0.994 0.301 0.239
050128 PL −0.059 ± 0.106 NA 1.546 ± 0.137 2.079 ± 0.064 0.566 0.693 0.541
050219A PL −2.605 ± 0.643 NA 3.156 ± 0.506 2.032 ± 0.057 0.743 0.563 0.728
050219B PL −0.200 ± 0.077 NA 1.875 ± 0.096 1.948 ± 0.038 0.895 0.418 0.510
050306 PL −1.439 ± 0.224 NA 1.529 ± 0.150 1.987 ± 0.023 0.768 0.841 0.898
050315 PL −1.708 ± 0.287 NA 2.018 ± 0.199 1.999 ± 0.027 0.201 0.862 0.774
050326 BPL 3.563 ± 0.353 −1.269 ± 0.185 2.408 ± 0.139 1.943 ± 0.051 0.127 0.691 0.606
050401 BPL 2.496 ± 0.341 −1.184 ± 0.216 3.050 ± 0.572 1.983 ± 0.049 0.238 0.364 0.242

Notes.

(a)

p(TR) is the significance associated with statistic TR.

(b)

pAD is the significance of the Anderson-Darling test.

(c)

pKS is the significance of the Kolmogorov-Smirnov test.

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