Fig. 2.
Peak flux densities of GRB 100418A as compared to the mm/submm and radio samples from de Ugarte Postigo et al. (2012a) and Chandra & Frail (2012). In blue we indicate lines of equal luminosity, with the most luminous events being found in the top right region of the plots. We have highlighted in green other GRBs where strong rebrightenings have been observed (see Sect. 3.3).
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