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Table 3
Fit of the P-GRB and the afterglow of GRB 110709B, episode 2.
| Parameter | P-GRB | P-GRB+afterglow |
|
|
||
| kT [keV] | 14 ± 1 | |
| BB Amp | 0.30 ± 0.02 | |
| γ | 1.03 ± 0.1 | |
| PL Amp | 0.5 ± 0.1 | |
| Red χ2 | 1.448 (56 D.O.F.) | 0.77 (55 D.O.F.) |
| Energy flux | 2.413 × 10-8 | 6.34 × 10-8 |
| (15 − 150 keV) | ||
| [ erg cm-2 s-1 ] | ||
| Energy [erg] | 3.44 × 1050 | 2.43 × 1052 |
Notes. The P-GRB is well-fit with a BB model, while the whole episode 2 is best fit by a cutoffPL model. From this fit and the value of the redshift we are able to calculate Eiso and EP − GRB.
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