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Fig. 3


a) Expected spectra of GRB 110918. The analytic model of Guetta et al. (2004) (blue) is shown with the usual simple treatment (blue solid) and accounting for different break energies of νμ and (blue dashed). The numerical NeuCosmA prediction is presented in red. b) Individual NeuCosmA spectra of the 296 GRBs (thin lines) and their sum (thick line).

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