{
  "bibcode": "2009GCN..9991....1P",
  "body": "K.L. Page, R.L.C. Starling, P.A. Evans & A.P. Beardmore (U. Leicester) \nreport on behalf of the Swift-XRT team:\n\nWe have now collected 15 ks of Swift-XRT Photon Counting mode data on the \nFermi burst GRB 091003 (Rau, GCN Circ. 9983; McEnery, Chiang & Hanabata, \nGCN Circ. 9985), between 56 and 168 ks after the trigger. The light-curve \nis fading, with alpha = 1.02 +0.21/-0.20. We therefore confirm that the \nsource given by Starling et al. in GCN Circ. 9986 and 9988 is, indeed, the \nX-ray afterglow.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 9991,
  "createdOn": 1254729580000,
  "email": "kpa@star.le.ac.uk",
  "subject": "GRB 091003: Swift-XRT confirmation of fading afterglow",
  "submitter": "Kim Page at U.of Leicester  <kpa@star.le.ac.uk>",
  "eventId": "GRB 091003"
}