TITLE: GCN CIRCULAR NUMBER: 30900 SUBJECT: GRB 210930A: Enhanced Swift-XRT position DATE: 21/09/30 09:19:07 GMT FROM: Phil Evans at U of Leicester <pae9@leicester.ac.uk> J.P. Osborne, A.P. Beardmore, P.A. Evans and M.R. Goad (U. Leicester) report on behalf of the Swift-XRT team. Using 1714 s of XRT Photon Counting mode data and 2 UVOT images for GRB 210930A, 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 = 197.40188, +48.62856 which is equivalent to: RA (J2000): 13h 09m 36.45s Dec (J2000): +48d 37' 42.8" with an uncertainty of 2.4 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.