Improving Swift-XRT positions of GRBs

P. A. Evans, A. P. Beardmore, M. R. Goad, J. P. Osborne, D. N. Burrows, N. Gehrels

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

Since GRBs fade rapidly, it is important to publish accurate, precise positions at early times. For Swift-detected bursts, the best promptly available position is most commonly the X-ray Telescope (XRT) position. We present two processes, developed by the Swift team at Leicester, which are now routinely used to improve the precision and accuracy of the XRT positions reported by the Swift team. Both methods, which are fully automated, make use of a PSF-fitting approach which accounts for the bad columns on the CCD. The first method yields positions with 90% error radii <4.4″90% of the time, within 10-20 minutes of the trigger. The second method astrometrically corrects the position using UVOT field stars and the known mapping between the XRT and UVOT detectors, yielding enhanced positions with 90% error radii of <2.8″90% of the time, usually 2 hours after the trigger.

Original languageEnglish (US)
Title of host publicationGamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference
Pages539-542
Number of pages4
DOIs
StatePublished - 2008
EventSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM, United States
Duration: Nov 5 2007Nov 9 2007

Publication series

NameAIP Conference Proceedings
Volume1000
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherSanta Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
CountryUnited States
CitySanta Fe, NM
Period11/5/0711/9/07

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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