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Table A.3.
Best fit parameters for the time-integrated analysis of the ten brightest short GRBs analysed in this work.
| Name | Time interval | Norm | α | Epeak | β | χ2/d.o.f. | Prob |
|---|---|---|---|---|---|---|---|
| (s) | (ph s−1cm2 keV) | (keV) | |||||
| 170206 | [−0.128 − 1.664 s] |  |
 |
 |
 |
361.63/346 | 0.2707 |
| 120323 | [−0.064 − 0.576 s] |  |
 |
 |
 |
372.44/353 | 0.2286 |
| 090227 | [−0.064 − 0.256 s] |  |
 |
 |
 |
358.17/349 | 0.3559 |
| 150819 | [−0.064 − 1.152 s] |  |
 |
 |
 |
349.53/347 | 0.4518 |
| 170127 | [−0.064 − 0.256 s] |  |
 |
 |
 |
312.4/348 | 0.9151 |
| 120624 | [0.000 − 0.320 s] |  |
 |
 |
 |
344.93/345 | 0.491 |
| 130701 | [−0.064 − 1.600 s] |  |
 |
 |
 |
324.75/347 | 0.7989 |
| 130504 | [−0.032 − 0.384 s] |  |
 |
 |
 |
375.6/352 | 0.1853 |
| 090228 | [−0.064 − 0.512 s] |  |
 |
 |
 |
346.76/349 | 0.5238 |
Notes. The best fit model is always a SBPL.
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