{
  "bibcode": "2020GCN.26999....1B",
  "body": "A.P. Beardmore, P.A. Evans, M.R. Goad and J.P. Osborne (U. Leicester) \nreport on behalf of the Swift-XRT team.\n\nUsing 1822 s of XRT Photon Counting mode data and 5 UVOT\nimages for GRB 200205B, 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 = 107.78760, -56.48741 which is equivalent\nto:\n\nRA (J2000): 07h 11m 9.03s\nDec (J2000): -56d 29' 14.7\"\n\nwith an uncertainty of 1.6 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": 26999,
  "createdOn": 1580961130000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 200205B: Enhanced Swift-XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 200205B"
}