{
  "bibcode": "2016GCN.19504....1B",
  "body": "D.N. Burrows (PSU), T.G.R. Roegiers (PSU), L.M. McCauley (PSU), S.L.\nGibson (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U.\nLeicester), A. Melandri (INAF-OAB), P. D'Avanzo (INAF-OAB), V. D'Elia\n(ASDC) and T.N. Ukwatta report on behalf of the Swift-XRT team:\n\nWe have analysed 7.1 ks of XRT data for GRB 160607A (Ukwatta et al. GCN\nCirc. 19502), from 65 s to 24.3 ks after the  BAT trigger. The data\ncomprise 935 s in Windowed Timing (WT) mode (the first 9 s were taken\nwhile Swift was slewing) with the remainder in Photon Counting (PC)\nmode. The enhanced XRT position for this burst was given by Goad et al.\n(GCN Circ. 19503).\n\nThe light curve can be modelled with a series of power-law decays. The\ninitial decay index is alpha=1.38 (+0.38, -0.21). At T+125 s  the decay\nflattens to an alpha of 0.66 (+/-0.04) before breaking again at T+2142\ns to a final decay with index alpha=1.25 (+0.08, -0.07).\n\nA spectrum formed from the WT mode data can be fitted with an absorbed\npower-law with a photon spectral index\tof 1.85 (+0.06, -0.05). The\nbest-fitting absorption column is  1.87 (+0.23, -0.22) x 10^21 cm^-2,\nin excess of the Galactic value of 5.1 x 10^20 cm^-2 (Willingale et al.\n2013). The PC mode spectrum has a photon index of 1.98 (+/-0.09) and a\nbest-fitting absorption column of 2.3 (+/-0.3) x 10^21 cm^-2. The\ncounts to observed (unabsorbed) 0.3-10 keV flux conversion factor\ndeduced from this spectrum  is 3.6 x 10^-11 (5.1 x 10^-11) erg cm^-2\ncount^-1. \n\nA summary of the PC-mode spectrum is thus:\nTotal column:\t     2.3 (+/-0.3) x 10^21 cm^-2\nGalactic foreground: 5.1 x 10^20 cm^-2\nExcess significance: 9.0 sigma\nPhoton index:\t     1.98 (+/-0.09)\n\nIf the light curve continues to decay with a power-law decay index of\n1.25, the count rate at T+24 hours will be 0.048 count s^-1,\ncorresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.7 x\n10^-12 (2.4 x 10^-12) erg cm^-2 s^-1.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/00689597.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 19504,
  "createdOn": 1465334573000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 160607A: Swift-XRT refined Analysis",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 160607A"
}