The burst alert telescope (BAT) on the SWIFT midex mission

Scott D. Barthelmy*, Louis M. Barbier, Jay R. Cummings, Ed E. Fenimore, Neil Gehrels, Derek Hullinger, Hans A. Krimm, Craig B. Markwardt, David M. Palmer, Ann Parsons, Goro Sato, Masaya Suzuki, Tadayuki Takahashi, Makota Tashiro, Jack Tueller

*この研究の対応する著者

研究成果: Article査読

1231 被引用数 (Scopus)

抄録

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 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 -8 erg 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 ∼2 m Crab (systematic limit) and it serves as a hard X-ray transient monitor.

本文言語English
ページ(範囲)143-164
ページ数22
ジャーナルSpace Science Reviews
120
3-4
DOI
出版ステータスPublished - 2005 12

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学
  • 物理学および天文学(その他)

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