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Fig. 8


Spectal fits for GRB 090424. a) The high-time resolution lightcurve of GRB 090424 with the hatched region being the region of interest. b) A simple Band fit to selected region. c) A Band + blackbody fit to the data. d) A double broken power-law fit with parameters of keV, keV, Index1 = , Index2 = , Index3 = (where Index1 < Ebreak1, Ebreak1 < Index2 < Ebreak2, Index3 > Ebreak2).

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