GCN Circular 8896
Poonam Chandra (RMC) 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 090205 (GCN 8884) at a frequency of 8.46 GHz on 2009 Jan 07.50 UT. The GRB radio afterglow is undetected at 3-sigma level. The flux density at the VLT afterglow position (GCB 8887) is 21 � 47 uJy. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc."