{
  "bibcode": "2022GCN.31673....1P",
  "body": "M. Perri (SSDC & INAF-OAR), V. D'Elia (SSDC & INAF-OAR), A. D'Ai\n(INAF-IASFPA), J. D. Gropp (PSU), J.A. Kennea (PSU), A. Tohuvavohu (U.\nToronto), P.A. Evans (U. Leicester), J.P. Osborne (U. Leicester), K.L.\nPage (U. Leicester) and E. Troja report on behalf of the Swift-XRT\nteam:\n\nWe have analysed 3.4 ks of XRT data for GRB 220302A (Troja et al. GCN\nCirc. 31661), from 32.5 ks to 160.8 ks after the  BAT trigger. The data\nare entirely in Photon Counting (PC) mode. The enhanced XRT position\nfor this burst was given by Osborne et al. (GCN Circ. 31666).\n\nThe light curve can be modelled with a power-law decay with a decay\nindex of alpha=0.7 (+0.5, -0.4).\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/01094950.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 31673,
  "createdOn": 1646376157000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 220302A: Swift-XRT refined Analysis",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 220302A"
}