{
  "bibcode": "2016GCN.20278....1O",
  "body": "J.P. Osborne, A.P. Beardmore, P.A. Evans and M.R. Goad (U. Leicester) \nreport on behalf of the Swift-XRT team.\n\nUsing 1529 s of XRT Photon Counting mode data and 2 UVOT\nimages for GRB 161217A, we find an astrometrically corrected X-ray\nposition (using the XRT-UVOT alignment and matching UVOT field sources\nto the USNO-B1 catalogue): RA, Dec = 150.65129, +52.35891 which is equivalent\nto:\n\nRA (J2000): 10h 02m 36.31s\nDec (J2000): +52d 21' 32.1\"\n\nwith an uncertainty of 1.9 arcsec (radius, 90% confidence).\n\nThis position may be improved as more data are received. The latest\nposition can be viewed at http://www.swift.ac.uk/xrt_positions. Position\nenhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans\net al. (2009, MNRAS, 397, 1177).\n\nThis circular was automatically generated, and is an official product of the\nSwift-XRT team.",
  "circularId": 20278,
  "createdOn": 1481952478000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 161217A: Enhanced Swift-XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 161217A"
}