GCN Circular 9834
S. T. Holland (CRESST/GSFC/USRA), A. Breeveld (MSSL/UCL), and W. Baumgartner (GSFC/UMBC) report on behalf of the Swift UVOT team: Swift/UVOT observed the USNO-B1.0 source 1341-0096763 (Evans et al. 2009, GCN Circ. 9819; Rumyantsev et al. 2009, GCN Circ. 9828; Holland et al. 2009, GCN Circ. 9831), which is located inside the XRT error circle (Evans et al., 2009, GCN Circ. 9819), at approximately 6 and 7 days after the INTEGRAL trigger (Beckman et al., 2009, GCN Circ. 9815). A preliminary examination of the UVOT data yields weak evidence that the source may have brightened by approximately 0.5 mag in the UVOT v band between approximately 6.5 and 7.1 days. Our observations are consistent with a supernova rising to maximum light. However, we stress that further observations are needed to confirm this. Follow-up photometric and spectroscopic observations of this source are strongly encouraged.