GCN Circular 6709
D. E. Vanden Berk (PSU), P. Kuin (MSSL), F. E. Marshall (NASA/GSFC), and A. M. Parsons (GSFC) report on behalf of the Swift-UVOT team: UVOT took a finding chart exposure of 100 seconds with the White (160-650 nm) filter starting 1977 seconds after the BAT trigger. No afterglow candidate has been found in the initial data products. The overlap of the sub-image and the BAT error circle is uncertain at this time. The 8'x8' region for the list of sources generated on-board covers 100% of the BAT error circle. Because of the density of catalogued stars, further analysis is required to report an upper limit for any afterglow in the region. No correction has been made for the extinction of E(B-V)=0.202.