TITLE:   GCN CIRCULAR
NUMBER:  43289
SUBJECT: GRB 260101A: Enhanced Swift-XRT position
DATE:    26/01/01 07:52:37 GMT
FROM:    Phil Evans at U of Leicester <pae9@star.le.ac.uk>

A.P. Beardmore, P.A. Evans, M.R. Goad and J.P. Osborne (U. Leicester) 
report on behalf of the Swift-XRT team.

Using 1689 s of XRT Photon Counting mode data and 3 UVOT
images for GRB 260101A, 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 = 86.42902, +63.59238 which is equivalent
to:

RA (J2000): 05h 45m 42.96s
Dec (J2000): +63d 35' 32.6"

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 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.