The burst alert telescope (BAT) on the Swift MIDEX mission

被引:1475
作者
Barthelmy, SD [1 ]
Barbier, LM
Cummings, JR
Fenimore, EE
Gehrels, N
Hullinger, D
Krimm, HA
Markwardt, CB
Palmer, DM
Parsons, A
Sato, G
Suzuki, M
Takahashi, T
Tashiro, M
Tueller, J
机构
[1] NASA, Goddard Space Flight Ctr, High Energy Phys Lab, Greenbelt, MD 20771 USA
[2] CNR, Washington, DC 20418 USA
[3] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA
[5] Univ Space Res Assoc, Columbia, MD 21044 USA
[6] Inst Space & Astronaut Sci, Kanagawa 2298510, Japan
[7] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 113, Japan
关键词
gamma-ray; GRB; hard X-ray; survey; burst; afterglow; CZT; coded aperture; astrophysics; cosmology;
D O I
10.1007/s11214-005-5096-3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The 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 20s 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 (4x4x2 mm), and the coded-aperture mask is composed of similar to 52,000 pieces of lead (5x5x1 mm) with a 1-m separation between mask and detector plane. The BAT operates over the 15-150 keV energy range with similar to 7 keV resolution, a sensitivity of similar to 10(-8) ergg s(-1) cm(-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 similar to 2 m Crab (systematic limit) and it serves as a hard X-ray transient monitor.
引用
收藏
页码:143 / 164
页数:22
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