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(a) Flux of the Band function (or of the cutoff power law) versus its E peak
when fitting Band-only (blue) or C+BB+PL (red)
to the fine time intervals of GRB 080916C. The dashed red line corresponds to the best fit of the red data points with a power law; (b)
Flux of the Band function (or of the cutoff power law) versus its E peak
when fitting Band-only (blue) or C+BB+PL (red) to the fine time intervals of GRB 090926A. The dashed red line corresponds to the best fit of the red data points with a power law; (c) Flux of the cutoff power law (i.e., non-thermal component, NT) versus its E peak
when C+BB or C+BB+PL are fitted to the time resolved data of four GRBs including short (green) and long ones (red, yellow and green). This is a refined version of the figure published in Guiriec et al. (2013) showing the similarity of the FNTi–ENT
peak, i relation for both short and long GRBs; (d) Luminosity of the cutoff power law versus its E peak when corrected for both the redshift and the k-correction (i.e., LNTi–E rest,NT peak, i relation) for the same sample of GRBs as in panel (c). The color dashed lines correspond to the best power law fit to the data of each individual GRB. The solid black line corresponds to the best
power law fit to the whole sample simultaneously.
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