Are GRB 980425 and GRB 031203 real outliers or twins of GRB 060218?

Abstract

Amati et al. (2001) found a correlation between the energy emitted (assuming isotropy) during the prompt phase of Gamma–Ray Bursts (GRBs), Eiso, and the frequency where most of this energy is emitted, Epeak (the so called Amati relation).

Citations and references