Table 3: Results of the fit of the normalized analytic model to the soft (0.1-1 keV) light curves of all simulated models. $\gamma _{\rm b}^{\rm sim}$ is the ratio $\Gamma _{\rm b}^{\rm sim}/\Gamma _{\rm f}^{\rm sim}$ computed from the models (see Table 1). The rest of the columns provide the other parameters obtained by fitting the normalized analytic model.
Sim. $\gamma _{\rm b}^{\rm sim}$ $\gamma_{\rm b}$ $K_{\rm b}$ $K_{\rm f}$ $t_{\rm b}$

S10- F10 0.943 0.832 $3.4\times 10^{-6}$ 1.07 0.429

S10- F07 0.940 0.867 $1.2\times 10^{-4}$ 1.68 0.434

S10- F05 0.937 0.861 $2.5\times 10^{-4}$ 1.39 0.445

S10- F14 0.944 0.855 $6.4\times 10^{-4}$ 2.35 0.414

S07- F10 0.946 0.913 $7.2\times 10^{-5}$ 1.40 0.567

S05- F10 0.948 0.887 $1.1\times 10^{-4}$ 1.95 0.579

S14- F10 0.941 0.839 $1.09\times 10^{-4}$ 1.34 0.415

**Table 3:** Results of the fit of the normalized analytic model to the soft (0.1-1 keV) light curves of all simulated models. $\gamma _{\rm b}^{\rm sim}$ is the ratio $\Gamma _{\rm b}^{\rm sim}/\Gamma _{\rm f}^{\rm sim}$ computed from the models (see Table 1). The rest of the columns provide the other parameters obtained by fitting the normalized analytic model.
Sim.	$\gamma _{\rm b}^{\rm sim}$	$\gamma_{\rm b}$	$K_{\rm b}$	$K_{\rm f}$	$t_{\rm b}$
S10- F10	0.943	0.832	$3.4\times 10^{-6}$	1.07	0.429
S10- F07	0.940	0.867	$1.2\times 10^{-4}$	1.68	0.434
S10- F05	0.937	0.861	$2.5\times 10^{-4}$	1.39	0.445
S10- F14	0.944	0.855	$6.4\times 10^{-4}$	2.35	0.414
S07- F10	0.946	0.913	$7.2\times 10^{-5}$	1.40	0.567
S05- F10	0.948	0.887	$1.1\times 10^{-4}$	1.95	0.579
S14- F10	0.941	0.839	$1.09\times 10^{-4}$	1.34	0.415

Source LaTeX | All tables | In the text

	1 Introduction
	2 Internal shock scenario
	3 Numerical simulations
	4 Analytic modeling of flares
	5 Fits of the analytic model to synthetic light curves
	6 Space time emissivity distribution
	7 Discussion
	References