GCN Circular 3132
A. M. Soderberg (Caltech) reports on behalf of the Caltech-NRAO-Carnegie GRB collaboration: "Using the Very Large Array at 8.5 GHz, we observed again the field of GRB050319 (GCN 3117) on 2005 Mar 21.4 UT. We still do not detect a radio source at the position of the optical afterglow (GCN 3116). We place a (2-sigma) limit of 133 uJy at that position. Combining these data with those of our previous epoch (GCN 3127), we derive a deeper limit of 70 uJy (2-sigma rms) for the field."