[AAVSO-HEN] GRB 100206A: Enhanced Swift-XRT position

[grb at aavso.org]

The following is a GCN Circular circulated via the AAVSO network.
For an archive and more information on circulars visit:
http://lheawww.gsfc.nasa.gov/docs/gamcosray/legr/bacodine/gcn3_archive.html

TITLE:   GCN CIRCULAR
NUMBER:  10378
SUBJECT: GRB 100206A: Enhanced Swift-XRT position
DATE:    10/02/06 17:30:38 GMT
FROM:    Phil Evans at U of Leicester  <pae9 at 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 1262 s of XRT Photon Counting mode data and 1 UVOT
images for GRB 100206A, 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 = 47.16225, +13.15708 which is equivalent
to:

RA (J2000): 03h 08m 38.94s
Dec (J2000): +13d 09' 25.5"

with an uncertainty of 3.2 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.