{
  "bibcode": "2014GCN.16016....1P",
  "body": "K.L. Page, C. Pagani, P.A. Evans (U. Leicester) & J.K. Cannizzo\n(NASA/UMBC) report on behalf of the Swift-XRT team:\n\nWe have now analysed 9.8 ks of Swift-XRT data for GRB 140320A, between 93\ns and 33.5 ks after the trigger. The X-ray source given by Page, Pagani &\nCannizzo in GCN Circ. 16010 has now faded, with a 3-sigma upper limit on\nthe count rate centred at 27 ks after the trigger of 1.2 x 10^-3 count\ns^-1. We therefore confirm this source as the X-ray afterglow of GRB\n140320A.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 16016,
  "createdOn": 1395396491000,
  "email": "klp5@leicester.ac.uk",
  "subject": "GRB 140320A: Confirmation of a fading X-ray afterglow",
  "submitter": "Kim Page at U.of Leicester  <klp5@leicester.ac.uk>",
  "eventId": "GRB 140320A"
}