TITLE: GCN CIRCULAR NUMBER: 30987 SUBJECT: GRB 211025A: Enhanced Swift-XRT position DATE: 21/10/25 09:46:31 GMT FROM: Phil Evans at U of Leicester <pae9@leicester.ac.uk> P.A. Evans, M.R. Goad, J.P. Osborne and A.P. Beardmore (U. Leicester) report on behalf of the Swift-XRT team. Using 2418 s of XRT Photon Counting mode data and 5 UVOT images for GRB 211025A, we find an astrometrically corrected X-ray position (using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue): RA, Dec = 162.38304, +31.51233 which is equivalent to: RA (J2000): 10h 49m 31.93s Dec (J2000): +31d 30' 44.4" with an uncertainty of 2.1 arcsec (radius, 90% confidence). This position may be improved as more data are received. The latest position can be viewed at http://www.swift.ac.uk/xrt_positions. Position enhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans et al. (2009, MNRAS, 397, 1177). This circular was automatically generated, and is an official product of the Swift-XRT team.