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Proceedings Paper

The Swift X-Ray Telescope
Author(s): David N. Burrows; Joanne E. Hill; John A. Nousek; Alan A. Wells; Guido Chincarini; Anthony F. Abbey; Andrew P. Beardmore; J. Bosworth; Heinrich W. Brauninger; Wolfgang Burkert; Sergio Campana; Milvia Capalbi; W. Chang; Oberto Citterio; Michael J. Freyberg; Paolo Giommi; Gisela D. Hartner; Ronnie Killough; B. Kittle; R. Klar; C. Mangels; M. McMeekin; B. J. Miles; Alberto Moretti; Koji Mori; Dave C. Morris; Kallol Mukerjee; Julian P. Osborne; Alexander D. T. Short; Gianpiero Tagliaferri; Francesca Tamburelli; D. J. Watson; Richard Willingale; Michael E. Zugger
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Paper Abstract

The Swift Gamma-Ray Explorer is designed to make prompt multiwavelength observations of Gamma-Ray Bursts (GRBs) and GRB Afterglows. The X-ray Telescope (XRT) provides key capabilities that permit Swift to determine GRB positions with a few arcseconds accuracy within 100 seconds of the burst onset. The XRT utilizes a superb mirror set built for JET-X and a state-of-the-art XMM/EPIC MOS CCD detector to provide a sensitive broad-band (0.2-10 keV) X-ray imager with effective area of 135 cm2 at 1.5 keV, field of view of 23.6 x 23.6 arcminutes, and angular resolution of 18 arcseconds (HEW). The detection sensitivity is 2x10-14 erg/cm2/s in 104 seconds. The instrument is designed to provide automated source detection and position reporting within 5 seconds of target acquisition. It can also measure redshifts of GRBs for bursts with Fe line emission or other spectral features. The XRT will operate in an auto-exposure mode, adjusting the CCD readout mode automatically to optimize the science return for each frame as the source fades. The XRT will measure spectra and lightcurves of the GRB afterglow beginning about a minute after the burst and will follow each burst for days as it fades from view.

Paper Details

Date Published: 3 February 2004
PDF: 16 pages
Proc. SPIE 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII, (3 February 2004); doi: 10.1117/12.504868
Show Author Affiliations
David N. Burrows, The Pennsylvania State Univ. (United States)
Joanne E. Hill, The Pennsylvania State Univ. (United States)
John A. Nousek, The Pennsylvania State Univ. (United States)
Alan A. Wells, Univ. of Leicester (United Kingdom)
Guido Chincarini, Osservatorio Astronomico di Brera (Italy)
Anthony F. Abbey, Univ. of Leicester (United Kingdom)
Andrew P. Beardmore, Univ. of Leicester (United Kingdom)
J. Bosworth, Swales Aerospace (United States)
Heinrich W. Brauninger, Max-Planck-Institut fuer extraterrestrische Physik (Germany)
Wolfgang Burkert, Max-Planck-Institut fuer extraterrestrische Physik (Germany)
Sergio Campana, Osservatorio Astronomico di Brera (Italy)
Milvia Capalbi, Agenzia Spaziale Italiana (Italy)
W. Chang, Swales Aerospace (United States)
Oberto Citterio, Osservatorio Astronomico di Brera (Italy)
Michael J. Freyberg, Max-Planck-Institut fuer extraterrestrische Physik (Germany)
Paolo Giommi, Agenzia Spaziale Italiana (Italy)
Gisela D. Hartner, Max-Planck-Institut fuer extraterrestrische Physik (Germany)
Ronnie Killough, Southwest Research Institute (United States)
B. Kittle, Swales Aerospace (United States)
R. Klar, Southwest Research Institute (United States)
C. Mangels, Southwest Research Institute (United States)
M. McMeekin, Swales Aerospace (United States)
B. J. Miles, The Pennsylvania State univ. (United States)
Alberto Moretti, Osservatorio Astronomico di Brera (Italy)
Koji Mori, The Pennsylvania State Univ. (United States)
Dave C. Morris, The Pennsylvania State Univ. (United States)
Kallol Mukerjee, Univ. of Leicester (United Kingdom)
Julian P. Osborne, Univ. of Leicester (United Kingdom)
Alexander D. T. Short, Univ. of Leicester (United Kingdom)
Gianpiero Tagliaferri, Osservatorio Astronomico di Brera (Italy)
Francesca Tamburelli, Agenzia Spaziale Italiana (Italy)
D. J. Watson, Univ. of Leicester (United Kingdom)
Richard Willingale, Univ. of Leicester (United Kingdom)
Michael E. Zugger, The Pennsylvania State Univ. (United States)

Published in SPIE Proceedings Vol. 5165:
X-Ray and Gamma-Ray Instrumentation for Astronomy XIII
Kathryn A. Flanagan; Oswald H. W. Siegmund, Editor(s)

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