GCN Circular 4442
Subject
GRB 060105: pseudo-z from spectral parameters of the prompt emission
Date
2006-01-06T17:02:38Z (18 years ago)
From
Jean-Luc Atteia at Lab d Astrophys.,OMP,Toulouse <atteia@ast.obs-mip.fr>
A. Pelangeon & J-L. Atteia (LATT-OMP) report:
We have used the spectral parameters of the most intense part
of GRB 060105 provided by Golenetskii et al. (GCNC 4439) to
compute the spectral pseudo-redshift of this GRB, assuming that
the most intense part of the burst contains half of the total fluence.
We find a pseudo-redshift pz= 4.0 +/- 1.3