[vsnet-grb-info 7272] GRB090123: Enhanced Swift-XRT position
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Fri Jan 23 21:51:02 JST 2009
TITLE: GCN CIRCULAR
NUMBER: 8843
SUBJECT: GRB090123: Enhanced Swift-XRT position
DATE: 09/01/23 12:50:55 GMT
FROM: Phil Evans at U of Leicester <pae9 at 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 1885 s of XRT Photon Counting mode data and 1 UVOT
images for GRB090123, 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 = 6.78599, -23.50156 which is equivalent
to:
RA (J2000): 00h 27m 8.64s
Dec (J2000): -23d 30' 05.6"
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.
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