Refined astrometry and positions for 179 Swift X-ray afterglows

Research output: Contribution to journalArticle

45 Scopus citations

Abstract

We present a refined catalog for the positions of 179 gamma-ray burst (GRB) X-ray afterglows observed by the X-Ray Telescope (XRT) on Swift prior to 2006 November 1. The positions are determined by detecting X-ray field sources in the deep X-ray images and comparing the centroids to those of optical sources in the Digitized Sky Survey red2 catalog or the Sloan Digital Sky Survey Data Release 5 catalog. Half of the 90% confidence error region radii are <2.2″. The error regions areas are typically ∼4 times smaller than the best XRT team error regions, although the positions require deep X-ray integration (>20 ks) and cannot be generated nearly as rapidly after the GRB. The positions derived for <90% of 77 bursts with optical afterglows are consistent with the optical transient positions, without the need for systematic error. About 20% of the afterglow positions require a sizable shift in the Swift satellite aspect. We discuss the optical/X-ray properties of the field sources and discuss the implications of the frame offsets for studies of optically dark GRBs.

Original languageEnglish (US)
Pages (from-to)1027-1033
Number of pages7
JournalAstronomical Journal
Volume133
Issue number3
DOIs
StatePublished - Mar 1 2007
Externally publishedYes

Keywords

  • Gamma rays: bursts
  • Supernovae: general
  • Telescopes
  • X-rays: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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