The Burst Alert Telescope (BAT) on the Swift MIDEX mission

被引:43
作者
Barthelmy, SD [1 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
X-RAY AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY XI | 2000年 / 4140卷
关键词
gamma-ray; GRB; hard x-ray; survey; burst; afterglow; CZT; coded aperture; astrophysics; cosmology;
D O I
10.1117/12.409149
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 3 instruments on the Swift MIDEX spacecraft to study gamma-ray bursts (GRBs). The BAT instrument is the instrument that first detects the GRB and localizes the burst direction to an accuracy of 1-4 arcmin within 10 sec after the start of the event. These locations cause the spacecraft to autonomously slew to point the two narrow-FOV instruments at the burst location within 20-70 sec to make follow-up x-ray and optical observations. BAT is a wide-FOV coded-aperture instrument with a CdZnTe detector plane. The detector plane is composed of 32,768 pieces of CdZnTe (4x4x2mm), and the coded-aperture mask is composed of similar to 50,000 pieces of lead (5x5x1mm) with a 1-m separation between mask and detector plane. The BAT operates over the 10-150 keV energy range with similar to7 keV resolution, a sensitivity of 0.2 ph/cm(2)-sec, and a 1.4 sr (half-coded) FOV. We expect to detect similar to 300 GRBs/yr for a 3-year mission. The BAT also performs an all-sky hard x-ray survey with a sensitivity of similar to1 mCrab (systematic limit) and as a hard x-ray transient monitor.
引用
收藏
页码:50 / 63
页数:14
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