Bibcode
                                    
                            Pizzichini, G.; Ferrero, P.; Genghini, M.; Gianotti, F.; Topinka, M.
    Referencia bibliográfica
                                    Il Nuovo Cimento C, vol. 28, Issue 3, p.319
Fecha de publicación:
    
                        5
            
                        2005
            
  Número de citas
                                    4
                            Número de citas referidas
                                    3
                            Descripción
                                    The present paper is a progress report on our work towards estimating
the energy emission involved in the many Gamma-Ray Bursts for which no
redshift has been actually measured. Once such an estimate is obtained,
we can try to extend the E peak
rest-Eiso relation found by Amati et al.(Astron.
Astrophys., 390 (2002) 81) to those events. Following Atteia (Astron.
Astrophys., 407 (2003) L1) we obtain a pseudo-redshift () estimate which
then allows us to estimate E peak rest and
Eiso for each burst.