GCN Circular 1827
Subject
GRB 030115: Radio detection of IR candidate
Date
2003-01-17T14:13:23Z (22 years ago)
From
Dale A. Frail at NRAO <dfrail@nrao.edu>
D. A. Frail (NRAO), and E. Berger (Caltech) report on behalf of a
larger collaboration:
"Radio observations made with the VLA at a frequency of 8.46 GHz on
2003 January 17.42 UT detect a weak radio source coincident with the
IR afterglow candidate detected by Levan et al. (GCN1818). The flux
density at the position of the IR source is 94+/-22 uJy. At this same
position two days earlier (GCN1817) no source was seen with a measured
flux density at the postion of the IR candidate of -86+/- 62 uJy.
Further observations are planned."