[vsnet-grb-info 11649] GRB 120311B: Enhanced Swift-XRT position

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Mon Mar 12 06:54:15 JST 2012


TITLE:   GCN CIRCULAR
NUMBER:  13042
SUBJECT: GRB 120311B: Enhanced Swift-XRT position
DATE:    12/03/11 21:54:08 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 4834 s of XRT Photon Counting mode data and 10 UVOT
images for GRB 120311B, 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 = 258.56208, -13.05144 which is equivalent
to:

RA (J2000): 17h 14m 14.90s
Dec (J2000): -13d 03' 05.2"

with an uncertainty of 1.6 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.


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