GCN Circular 5735
F.E. Marshall (NASA/GSFC) and C. Guidorzi (Univ Bicocca&INAF-OAB) report on behalf of the Swift-UVOT team: The Swift UVOT began observing the GRB 061019 field (trigger 234516) 2790 seconds after the BAT trigger (Guidorzi et al. GCN Circ. 5728). Exposures were taken with the V, B, U, W1, M2, and W2 filters. No new source was detected within the XRT error circle (Guidorzi et al. GCN Circ. 5733). The effects of a nearby bright star complicate the analysis, but we estimate a 3-sigma upper limit of ~19th magnitude at the position of the optical afterglow (Covino et al. GCN Circ. 5730; Cobb et al. GCN Circ. 5734) for the initial exposure with the V filter.