Fig. 2
Radius evolution of the black-body emitter given by Eq. (1) in the first episode of GRB 090618 (Izzo et al. 2012), here assumed as the radius of the SN. The time is here measured in the rest frame, i.e. divided by a factor 1 + z, where z = 0.54, compared that one of the first episode given in Fig. 1.
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