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Fig. 8
Positions in the Ep,i – Eiso plane of the eight cosmological GRBs, described in the text, characterized by a higher energy and a higher redshift than GRB 060218, GRB 161219B, and GRB 100316D. We note that the emission of these events as observed by BATSE and Beppo-SAX still satisfies the Ep,i – Eiso correlation.
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