{
  "bibcode": "2011GCN.11680....1E",
  "body": "P.A. Evans and O.M. Littlejohns (U. Leicester) report on behalf of the \nSwift team:\n\nSwift observed the field of GRB 110207A (Littlejohns et al., GCN Circ. \n11658) for 5 ks from T0+99 ks to T0+112 ks; earlier observations were \nimpossible due to the proximity of the GRB to the Moon. We find no X-ray \nsources in the BAT field of view, placing a 3-sigma upper limit on the \nafterglow brightness of 7.6e-14 erg/cm^2/sec during this interval \n(0.3-10 keV; assuming a typical GRB spectrum). Due to the proximity of \nthe GRB to the Sun, no further observations are planned.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 11680,
  "createdOn": 1297262677000,
  "email": "pae9@star.le.ac.uk",
  "subject": "GRB 110207A: Swift-XRT observations",
  "submitter": "Phil Evans at U of Leicester  <pae9@star.le.ac.uk>",
  "eventId": "GRB 110207A"
}