TITLE: GCN CIRCULAR NUMBER: 24151 SUBJECT: GRB 190422A: Enhanced Swift-XRT position DATE: 19/04/23 02:43:14 GMT FROM: Phil Evans at U of Leicester P.A. Evans, M.R. Goad, J.P. Osborne and A.P. Beardmore (U. Leicester) report on behalf of the Swift-XRT team. Using 1699 s of XRT Photon Counting mode data and 1 UVOT images for GRB 190422A, 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 = 182.03450, -60.22425 which is equivalent to: RA (J2000): 12h 08m 8.28s Dec (J2000): -60d 13' 27.3" with an uncertainty of 1.8 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.