Fig. 7.
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Amati correlation for GRB 150309A. As there is no redshift measurement is available, we had to vary the redshift from 0.1 to 10. For comparison, we also show other long bursts studied by Nava et al. (2012). The solid red line shows the best-fit line, and the pink shaded band shows the associated 2-σ uncertainty using the study of a sample of long bursts by Nava et al. (2012).
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