GCN Circular 7614
Poonam Chandra (NRAO/UVA) and Dale A. Frail (NRAO) report on behalf of the Caltech-NRAO-Carnegie GRB Collaboration: "We used the Very Large Array to observe the field of view toward GRB 080413A (GCN 7594) at a frequency of 8.46 GHz at 2008 April 14.53 UT. We do not detect the GRB afterglow at the ROTSE optical position (GCN 7593). The flux density at the GRB afterglow position is -61 +/- 49 uJy. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc."