GCN Circular 1827
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."