{
  "bibcode": "2014GCN.16011....1P",
  "body": "K.L. Page, C. Pagani, P.A. Evans and M.R. Goad (U. Leicester) report on\nbehalf of the Swift-XRT team:\n\nUsing 715 s of XRT Photon Counting mode data and 1 UVOT images, we find an\nastrometrically corrected X-ray position (using the XRT-UVOT alignment and\nmatching UVOT field sources to the USNO-B1 catalogue): RA, Dec =\n281.85530, -11.19412 which is equivalent to:\n\nRA (J2000):  18 47 25.27\nDec (J2000): -11 11 38.8\n\nwith an uncertainty of 4.9 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 is an official product of the Swift-XRT team.",
  "circularId": 16011,
  "createdOn": 1395347393000,
  "email": "klp5@leicester.ac.uk",
  "subject": "GRB 140320A: Enhanced Swift-XRT position",
  "submitter": "Kim Page at U.of Leicester  <klp5@leicester.ac.uk>",
  "eventId": "GRB 140320A"
}