GCN Circular 7308
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 080212 (GCN 7296) at a frequency of 8.46 GHz on 2008 February 13.53 UT. The radio afterglow of the GRB is undetected at the Swift-XRT position (GCN 7300) or optical afterglow position (GCN 7303). The peak flux density at the afterglow position is 83 +/- 51 uJy. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc."