TITLE: GCN CIRCULAR NUMBER: 42159 SUBJECT: GRB 251007B: Enhanced Swift-XRT position DATE: 25/10/08 07:13:08 GMT FROM: Phil Evans at U of Leicester <pae9@star.le.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 1164 s of XRT Photon Counting mode data and 2 UVOT images for GRB 251007B, 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 = 102.13270, -10.30374 which is equivalent to: RA (J2000): 06h 48m 31.85s Dec (J2000): -10d 18' 13.4" with an uncertainty of 2.5 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. View this GCN Circular online at https://gcn.nasa.gov/circulars/42159. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...