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Fig. 6.


Top panel: comparison of the light curves of a large sample of GRB afterglows shifted to a common redshift of z = 1 (adapted from Kann et al. 2018). The afterglow of GRB 161023A is amongst the most luminous afterglows observed so far. More details can be found in the text. Bottom panel: comparison of the observed peak fluxes in the mm/submm bands (adapted from de Ugarte Postigo et al. 2012a).

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