{
  "bibcode": "2017GCN.20550....1G",
  "body": "M.R. Goad, J.P. Osborne, A.P. Beardmore and P.A. Evans (U. Leicester) \nreport on behalf of the Swift-XRT team.\n\nUsing 1434 s of XRT Photon Counting mode data and 2 UVOT\nimages for GRB 170127B, 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 = 19.97709, -30.35807 which is equivalent\nto:\n\nRA (J2000): 01h 19m 54.50s\nDec (J2000): -30d 21' 29.1\"\n\nwith an uncertainty of 2.0 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": 20550,
  "createdOn": 1485555393000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 170127B: Enhanced Swift-XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 170127B"
}