GCN Circular 4384
Subject
GRB 051221: Redshift from Gemini
Date
2005-12-22T09:33:06Z (18 years ago)
From
Edo Berger at Carnegie Obs <eberger@ociw.edu>
E. Berger (Carnegie Observatories) and A. M. Soderberg (Caltech) report:
"We obtained 2x1200 sec spectra of the afterglow + host galaxy of the
short GRB 051221 (GCN 4383) with Gemini/GMOS. We detect several strong
emission lines at the position of the afterglow+host which we identify as
[OIII]4959,5006, H-beta, and [OII]3727 at a redshift of z=0.5465. Weak
absorption at the CaII H&K and G-band wavelengths at the same redshift may
also be present, but at a low significance.
The detection of strong emission lines indicates that the host galaxy is
under-going active star formation, and is possibly similar to that of GRB
050709 (Fox et al. 2005).
At the redshift of 0.5465, the isotropic-equivalent gamma-ray energy
release of the burst is 9e50 erg, the highest measured to date."