GCN Circular 14966
P.A. Evans (U. Leicester) and S. R. Oates (UCL-MSSL) report on behalf of the Swift-XRT team: Swift performed a second epoch observation of GRB 130627B (Oates et al., GCN Circ. 14936) on 2013 July 2nd, collecting 7.3 ks of Photon Counting mode data from T0+390 ks to T0+415 ks. The X-ray object reported by Evans et al. (GCN Circ. 14947) is no longer detected. The 3-sigma upper limit is 1.7 x 10^-3 ct/sec, which is well below the level of 8.8(+/-2.0) x 10^-3 ct/sec at which the source was previously detected. We therefore confirm that this object was the afterglow of GRB 130627B. This circular is an official product of the Swift-XRT team.