[vsnet-grb-info 6110] GRB 080517: Enhanced Swift-XRT position
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Sun May 18 09:01:32 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 7744
SUBJECT: GRB 080517: Enhanced Swift-XRT position
DATE: 08/05/18 00:00:38 GMT
FROM: Phil Evans at U of Leicester <pae9 at 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 88 s of overlapping XRT Photon Counting mode and UVOT
data for GRB 080517, 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 = 102.24189, +50.73496 which is equivalent
to:
RA (J2000): 06h 48m 58.05s
Dec (J2000): +50d 44' 05.8"
with an uncertainty of 1.8 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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