[vsnet-grb-info 21851] GRB 190311A: Enhanced Swift-XRT position
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Mar 12 01:38:28 JST 2019
TITLE: GCN CIRCULAR
NUMBER: 23950
SUBJECT: GRB 190311A: Enhanced Swift-XRT position
DATE: 19/03/11 16:37:34 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 1682 s of XRT Photon Counting mode data and 2 UVOT
images for GRB 190311A, 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 = 212.06539, +53.50037 which is equivalent
to:
RA (J2000): 14h 08m 15.69s
Dec (J2000): +53d 30' 01.3"
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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