{
  "body": "P.A. Evans, M.R. Goad, J.P. Osborne and A.P. Beardmore (U. Leicester) \nreport on behalf of the Swift-XRT team.\n\nUsing 3740 s of XRT Photon Counting mode data and 7 UVOT\nimages for GRB 250605A, 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 = 166.95715, -19.78841 which is equivalent\nto:\n\nRA (J2000): 11h 07m 49.72s\nDec (J2000): -19d 47' 18.3\"\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.\n",
  "circularId": 40642,
  "eventId": "GRB 250605A",
  "createdOn": 1749199440926,
  "subject": "GRB 250605A: Enhanced Swift-XRT position",
  "bibcode": "2025GCN.40642....1E",
  "submittedHow": "email",
  "submitter": "Phil Evans at U of Leicester <pae9@star.le.ac.uk>"
}