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BARTHELMY, Scott D; BARRIER, Louis M; SATO, Goro; SUZUKI, Masaya; TAKAHASHI, Tadayuki; TASHIRO, Makota; TUELLER, Jack; CUMMINGS, Jay R; FENIMORE, Ed E; GEHRELS, Neil; HULLINGER, Derek; KRIMM, Hans A; MARKWARDT, Craig B; PALMER, David M; PARSONS, Ann
Space science reviews, 12/2005, Volume: 120, Issue: 3-4Journal Article
he burst alert telescope (BAT) is one of three instruments on the Swift MIDEX spacecraft to study gamma-ray bursts (GRBs). The BAT first detects the GRB and localizes the burst direction to an accuracy of 1-4 arcmin within 20 s after the start of the event. The GRB trigger initiates an autonomous spacecraft slew to point the two narrow field-of-view (FOV) instruments at the burst location within 20-70 s so to make follow-up X-ray and optical observations. The BAT is a wide-FOV, coded-aperture instrument with a CdZnTe detector plane. The detector plane is composed of 32,768 pieces of CdZnTe (4×4×2 mm), and the coded-aperture mask is composed of 52,000 pieces of lead (5×5×1 mm) with a 1-m separation between mask and detector plane. The BAT operates over the 15-150 keV energy range with 7 keV resolution, a sensitivity of 10^sup -8^ erg s^sup -1^ cm^sup -2^, and a 1.4 sr (half-coded) FOV. We expect to detect > 100 GRBs/year for a 2-year mission. The BAT also performs an all-sky hard X-ray survey with a sensitivity of 2 m Crab (systematic limit) and it serves as a hard X-ray transient monitor.PUBLICATION ABSTRACT
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