GCN Circular 11415
P.A. Evans (U. Leicester) reports on behalf of the Swift-XRT team: We have performed a second epoch observation with Swift-XRT of GRB 101114A (Sakamoto et al., GCN Circ. 11405). This observation was 5.5 ks in length, beginning 3.5 days after the GRB trigger. The source reported by Evans et al. (GCN Circ. 11406) is still detected, but has faded significantly to a level of 1.6 (+/- 0.9) x 10^-3 ct/sec. We thus confirm that this is the afterglow of GRB 101114A. This circular is an official product of the Swift-XRT team.