GCN Circular 9206
A. Levan (U. Warwick), N. Tanvir (U. Leicester), K. Wiersema (U. Leicester) Further analysis of the data reported in GCN 9202 reveals that the source did not fade appreciably (i.e. by more than ~0.15 mag) between observations with mid-times 25 and 41 minutes post-burst. However, we do believe that the extension of the image is consistent with it being a point source. We note that the revised XRT error circle (GCN 9205) now contains this source, making it likely the counterpart or host of this GRB.