Fig. 9.
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Temporal evolution of the synchrotron break frequencies for afterglow emission of GRB 160131A, based on analysis of UVOIR/X-ray data (Table 5, second column). See the caption of Fig. 7 for a full description of the modelling. The self-absorption frequency produced by noncooled electrons νac makes sense only in fast-cooling regime (≲0.02 d).
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