GCN Circular 4244
Dale A. Frail (NRAO), P. Brian Cameron (Caltech), and Alicia M. Soderberg (Caltech) report on behalf of a larger collaboration: "We observed the field of GRB 051109A (GCN 4213) with the Very Large Array at 8.5 GHz around November 11.15 UT. At the position of the optical transient (GCN 4211) there is a weak radio source with flux density 117 � 24 uJy. We identify this as the radio afterglow of GRB 051109A. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc."