Table 2.
Best-fit parameters for the synchrotron model obtained in the three time intervals in which the first SED has been split.
| Time interval | Flux | Ec | Em | p(β) |  (d.o.f.) |
||
|---|---|---|---|---|---|---|---|
| [10−7 erg s−1 cm2] | [keV] | [keV] | |||||
| 0–14 s |
 |
 |
 |
 |
1.11(341) | ||
| 14–21 s |
 |
 |
 |
 |
1.17(341) | ||
| 27–35 s |
 |
 |
 |
 |
1.12(341) |
Notes. For these time intervals, we used GBM and LLE data together, modelling the spectrum from 10 keV up to 100 MeV. The first column reports the time interval over which the spectrum has been integrated. The second column onwards list the following fit parameters: energy flux computed in the energy range 10 keV–100 MeV, photon energy Ec corresponding to the electron cooling Lorentz factor γc, photon energy Emcorresponding to the electron injection Lorentz factor γm, electron energy distribution slope p (corresponding high-energy photon index β = −p/2 − 1 in parentheses), and the reduced χ2 of the fit with the degrees of freedom in parentheses.
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