{
  "bibcode": "2016GCN.19486....1M",
  "body": "A. Maselli  (INAF-IASFPA), B. Sbarufatti (INAF-OAB/PSU), D.N. Burrows\n(PSU), T.G.R. Roegiers (PSU), P.A. Evans (U. Leicester), S.L. Gibson\n(U. Leicester), J.P. Osborne (U. Leicester), A. Melandri (INAF-OAB), P.\nD'Avanzo (INAF-OAB) and D. Kocevski report on behalf of the Swift-XRT\nteam:\n\nWe have analysed 7.9 ks of XRT data for GRB 160601A (Kocevski et al.\nGCN Circ. 19478), from 94 s to 23.6 ks after the  BAT trigger. The data\nare entirely in Photon Counting (PC) mode. The enhanced XRT position\nfor this burst was given by Evans et al. (GCN Circ. 19484).\n\nThe light curve can be modelled with a power-law decay with a decay\nindex of alpha=0.49 (+0.14, -0.15).\n\nIf the light curve continues to decay with a power-law decay index of\n0.49, the count rate at T+24 hours will be 2.0 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/00688452.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 19486,
  "createdOn": 1464827394000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 160601A: Swift-XRT refined Analysis",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 160601A"
}