{
  "bibcode": "2019GCN.24001....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 1829 s of XRT Photon Counting mode data and 5 UVOT\nimages for GRB 190324A, 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 = 49.61588, -47.21487 which is equivalent\nto:\n\nRA (J2000): 03h 18m 27.81s\nDec (J2000): -47d 12' 53.5\"\n\nwith an uncertainty of 1.5 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": 24001,
  "createdOn": 1553487289000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 190324A: Enhanced Swift-XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 190324A"
}