[vsnet-grb-info 17829] GRB 160410A: Enhanced Swift-XRT position
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Sun Apr 10 21:40:47 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19273
SUBJECT: GRB 160410A: Enhanced Swift-XRT position
DATE: 16/04/10 12:39:51 GMT
FROM: Phil Evans at U of Leicester <pae9 at leicester.ac.uk>
A.P. Beardmore, P.A. Evans, M.R. Goad and J.P. Osborne (U. Leicester)
report on behalf of the Swift-XRT team.
Using 380 s of XRT Photon Counting mode data and 2 UVOT
images for GRB 160410A, 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 = 150.68560, +3.47856 which is equivalent
to:
RA (J2000): 10h 02m 44.54s
Dec (J2000): +03d 28' 42.8"
with an uncertainty of 3.0 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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