{
  "bibcode": "2016GCN.20128....1B",
  "body": "D.N. Burrows (PSU), T.G.R. Roegiers (PSU), L.M. McCauley (PSU), B.\nMingo (U. Leicester), A.P. Beardmore (U. Leicester), A. Melandri\n(INAF-OAB), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC) and B. Mingo (U\nLeicester) report on behalf of the Swift-XRT team:\n\nWe have analysed 6.3 ks of XRT data for GRB 161104A (Mingo et al. GCN\nCirc. 20123), from 68 s to 23.6 ks after the  BAT trigger. The data are\nentirely in Photon Counting (PC) mode. The enhanced XRT position for\nthis burst was given by Goad et al. (GCN Circ. 20124).\n\nThe light curve can be modelled with a power-law decay with a decay\nindex of alpha=0.37 (+0.17, -0.16).\n\nIf the light curve continues to decay with a power-law decay index of\n0.37, the count rate at T+24 hours will be 1.6 x 10^-3 count s^-1\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/00720568.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 20128,
  "createdOn": 1478293238000,
  "email": "klp5@leicester.ac.uk",
  "subject": "GRB 161104A: Swift-XRT refined Analysis",
  "submitter": "Kim Page at U.of Leicester  <klp5@leicester.ac.uk>",
  "eventId": "GRB 161104A"
}