{
  "bibcode": "2010GCN.11415....1E",
  "body": "P.A. Evans (U. Leicester) reports on behalf of the Swift-XRT team:\n\nWe have performed a second epoch observation with Swift-XRT of GRB\n101114A (Sakamoto et al., GCN Circ. 11405). This observation was 5.5 ks\nin length, beginning 3.5 days after the GRB trigger. The source reported\nby Evans et al. (GCN Circ. 11406) is still detected, but has faded\nsignificantly to a level of 1.6 (+/- 0.9) x 10^-3 ct/sec. We thus\nconfirm that this is the afterglow of GRB 101114A.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 11415,
  "createdOn": 1290091576000,
  "email": "pae9@star.le.ac.uk",
  "subject": "GRB 101114A: Confirmation of the X-ray afterglow",
  "submitter": "Phil Evans at U of Leicester  <pae9@star.le.ac.uk>",
  "eventId": "GRB 101114A"
}