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Table 1.

Comparison between different models used for the episode-wise time-averaged joint spectral analysis of Fermi/GBM and Swift/BAT data of GRB 180728A and GRB 190829A.

GRB 180728A

Episode Time (s) Model Log(Likelihood) AIC (a) BIC (b)
1 −1.70 − 1.31 PL* 1475.81 2961.76 2981.78
CPL 1475.81 2963.82 2987.81
Band 1471.44 2957.15 2985.11
PL+BB 1475.81 2965.89 2993.85
CPL+BB 1487.62 2985.39 3005.41
Band+BB 1471.24 2960.92 2996.77

2 8.61 − 23.39 PL 4358.70 8729.56 8755.10
CPL 3395.31 6804.84 6834.60
Band 3472.00 6960.27 6994.25
PL+BB 3877.83 7771.93 7805.91
CPL+BB 3347.10 6712.54 6750.74
Band+BB* 3273.44 6567.31 6609.71

GRB 190829A

1 −0.64 − 8.06 PL 2268.45 4549.07 4574.61
CPL* 2261.82 4537.84 4567.62
Band 2262.13 4540.54 4574.54
PL+BB 2264.48 4545.24 4579.24
CPL+BB 2261.43 4541.21 4579.43
Band+BB Unconstrained Unconstrained Unconstrained

2 47.04 − 62.46 PL 2182.14 4374.42 4394.47
CPL 2175.54 4363.29 4387.31
Band* 2147.17 4308.61 4336.60
PL+BB 2150.16 4314.60 4342.59
CPL+BB 2148.33 4313.02 4344.97
Band+BB 2142.71 4303.85 4339.75

Notes. In the model column, the best-fit model is marked with a star. The PL, CPL, and BB correspond to the power law, cut-off power law and blackbody models, respectively.

(a)

Akaike information criterion,

(b)

Bayesian information criterion.

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