TITLE: GCN CIRCULAR NUMBER: 42116 SUBJECT: GRB 251005C: Enhanced Swift-XRT position DATE: 25/10/05 19:33:09 GMT FROM: Phil Evans at U of Leicester pae9@star.le.ac.uk
M.R. Goad, J.P. Osborne, A.P. Beardmore and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team.
Using 1541 s of XRT Photon Counting mode data and 2 UVOT images for GRB 251005C, 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 = 75.68325, +16.88054 which is equivalent to:
RA (J2000): 05h 02m 43.98s Dec (J2000): +16d 52' 49.9"
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 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.
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