{
  "bibcode": "2014GCN.16665....1M",
  "body": "A. Maselli, M. De Pasquale (INAF-IASFPA) and E. Troja (NASA/GSFC/UMCP) \nreport on behalf of the Swift-XRT team:\n\nWe report on further Swift XRT observations in the field of the \nFERMI/GBM-discovered GRB 140801A (Pelassa, GCN Circ. 16658). A new \nexposure of 2.0 ks has been obtained, 123 ks after the Fermi/GBM \ntrigger. The X-ray counterpart reported by Maselli & De Pasquale (GCN \nCirc. 16661) is still detected at a count rate of 9.9 (+/-2.5) x 10^-3 \ncts s^-1. This latest measurement corresponds to a decay slope of 0.8 \n(+0.5, -0.4): thus we confirm that this source is the afterglow of GRB \n140801A.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 16665,
  "createdOn": 1407074725000,
  "email": "maselli@ifc.inaf.it",
  "subject": "GRB140801A: Swift/XRT further observations",
  "submitter": "Alessandro Maselli at INAF/IASF Palermo  <maselli@ifc.inaf.it>",
  "eventId": "GRB 140801A"
}