TITLE: GCN CIRCULAR NUMBER: 19229 SUBJECT: GRB 160325A: Enhanced Swift-XRT position DATE: 16/03/25 17:07:26 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 2264 s of XRT Photon Counting mode data and 3 UVOT images for GRB 160325A, 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 = 15.65055, -72.69659 which is equivalent to: RA (J2000): 01h 02m 36.13s Dec (J2000): -72d 41' 47.7" with an uncertainty of 1.7 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.