TITLE: GCN CIRCULAR NUMBER: 42558 SUBJECT: GRB 251103B: Enhanced Swift-XRT position DATE: 25/11/03 20:12:14 GMT FROM: Phil Evans at U of Leicester pae9@star.le.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 1251 s of XRT Photon Counting mode data and 1 UVOT images for GRB 251103B, 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 = 105.87339, -24.87217 which is equivalent to:

RA (J2000): 07h 03m 29.61s Dec (J2000): -24d 52' 19.8"

with an uncertainty of 2.3 arcsec (radius, 90% confidence).

This position may be improved as more data are received. The latest position can be viewed at https://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.

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