[vsnet-grb-info 17218] GRB 151111A: Enhanced Swift-XRT position

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Wed Nov 11 22:42:58 JST 2015


TITLE:   GCN CIRCULAR
NUMBER:  18579
SUBJECT: GRB 151111A: Enhanced Swift-XRT position
DATE:    15/11/11 13:39:52 GMT
FROM:    Phil Evans at U of Leicester  <pae9 at leicester.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 639 s of XRT Photon Counting mode data and 1 UVOT
images for GRB 151111A, 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 = 56.84455, -44.16154 which is equivalent
to:

RA (J2000): 03h 47m 22.69s
Dec (J2000): -44d 09' 41.5"

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) 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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