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Fig. 7


Distribution of the power law indices for the subsample of INTEGRAL GRBs that were fitted with the single power law model on the energy range 20−1000 keV (black line). BATSE results (violet) and Fermi GBM results (red) are shown for the GRBs for which the best spectral model was a single power law. The results for the analysis of the time-integrated spectra are shown, using GRBs within the same fluence range as INTEGRAL GRBs.

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