Fig. 12
Our trio of GRBs on the Ep – Eiso,γ plane. The sample of GRBs presented in Amati et al. (2008) are shown in grey, along with their best fit to a single power-law (α = 0.57) and the 2σ uncertainty in their fit. GRBs 120729A and 130831A lie perfectly on the Amati relation, while GRB 130215A is within the 2-σ confidence interval.
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