{
  "bibcode": "2009GCN..9810....1E",
  "body": "P.A. Evans (U. Leicester) and W.H. Baumgartner (GSFC/UMBC) report on\nbehalf of the Swift-XRT team:\n\nThe Swift-XRT conducted a second observation of GRB 090814B (Beckmann et\nal. GCN. Circ. 9795), gathering 3.3 ks of data between T0+48 ks and\nT0+60 ks. The source reported by Evans & Baumgartner (GCN Circ. 9803)\nhas faded to a level of 0.11 �� 0.03 count/sec, with a power-law decay\nindex of alpha=0.7+/-0.3. This source is thus confirmed as the afterglow\nof GRB 090814B.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/00020107.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 9810,
  "createdOn": 1250324209000,
  "email": "pae9@star.le.ac.uk",
  "subject": "GRB 090814B: Confirmation of the X-ray afterglow",
  "submitter": "Phil Evans at U of Leicester  <pae9@star.le.ac.uk>",
  "eventId": "GRB 090814B"
}