Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 6151

Subject
GRB070224: Swift-XRT Astrometrically Corrected Position
Date
2007-02-26T19:22:30Z (17 years ago)
From
Judith Racusin at PSU <racusin@astro.psu.edu>
J. Racusin (PSU), M. Goad (U. Leicester), D.N. Burrows (PSU), O. Godet (U. 
Leicester), R. Starling (U. Leicester) report on behalf of the Swift XRT 
team:

Based on an accurate mapping between the XRT and UVOT detector coordinate 
systems, we have used the simultaneous UVOT V-band images to 
astrometrically correct (relative to stellar catalogues, e.g. USNO-B1) the 
XRT world coordinate system, and thereby refine the XRT position.  We 
obtain a new XRT position at RA,Dec=179.02792,-13.3304 which is:

RA(J2000):  11h 56m 06.7s
Dec(J2000): -13d 19' 49.6"

with an uncertainty of 2.6 arcseconds (90% containment).  This is 3.8 
arcseconds from the refined XRT position (Racusin et al., GCN 6143), and 
2.0 arcseconds from the optical candidate first identified by Thoene et 
al. (GCN 6142).

This circular is an official product of the Swift-XRT team.
Looking for U.S. government information and services? Visit USA.gov