TITLE:   GCN CIRCULAR
NUMBER:  8796
SUBJECT: GRB 090111: Enhanced Swift-XRT position
DATE:    09/01/12 04:41:17 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 1667 s of XRT Photon Counting mode data and 2 UVOT
images for GRB 090111, 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 = 251.67557, +0.07728 which is equivalent
to:

RA (J2000): 16h 46m 42.14s
Dec (J2000): +00d 04' 38.2"

with an uncertainty of 1.7 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
http://www.swift.ac.uk/xrt_positions/Goad.pdf), the current algorithm is an
extension of this method.

This circular was automatically generated, and is an official product of the
Swift-XRT team.