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Fig. 16.

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Slow cooling: Evolution of the derived dynamical (top) and microphysical (bottom) parameters of the afterglow of GRB 100418A without SSC emission. The blue dashed lines and shaded regions represent the results from the fit of the observed temporal evolution. The horizontal dashed purple lines show the average value for each parameter. EK, iso is in units of 1052 erg.

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