Table 1
Best-Fit parameters for the four selected GRBs.
| GRB | Pi [ms] | B14 [G] | k | E0,50 [erg] | T0 [s] |
|
|
|||||
| 050319 | 1.05 ± 0.03 | 5.5 ± 0.4 | 0.80 ± 0.25 | 10.0 ± 2.1 | 100 |
| 060729 | 2.12 ± 0.08 | 3.2 ± 0.2 | 0.58 ± 0.11 | 1.3 ± 0.2 | 300 |
| 061121 | 1.18 ± 0.06 | 12.2 ± 0.7 | 0.66 ± 0.21 | 10.4 ± 3.0 | 100 |
| 080430 | 3.7 ± 0.6 | 11.7 ± 1.1 | 0.33 ± 0.09 | 1.2 ± 0.3 | 200 |
Notes. The time T0 is the time from which we fit observed lightcurves (see text for more details) and the energy E0 respresents the total energy in units of 1050 erg within the blastwave at time T0. The dipole magnetic field of the NS is expressed in units of 1014. Reported errors are at 1σ.
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