Prototype TIGRE compton γ-ray balloon-borne telescope

被引:12
作者
Bhattacharya, D
O'Neill, TJ
Akyüz, A
Samimi, J
Zych, AD [1 ]
机构
[1] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
[2] Cukurova Univ, Dept Phys, TR-01330 Adana, Turkey
[3] Sharif Univ Technol, Dept Phys, Tehran, Iran
关键词
gamma-ray astronomy; Compton telescope; electron tracking;
D O I
10.1016/j.newar.2003.11.033
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A prototype balloon-borne telescope is being constructed for gamma-ray observations in the MeV energy range. The Tracking and Imaging Gamma-Ray Experiment (TIGRE) uses multi-layers of thin silicon detectors to track and measure the energy losses of Compton recoil electrons. When combined with the direction and energy of the Compton scattered gamma-ray a unique incident direction for each photon event is determined. This facilitates background rejection, improved sensitivity and image reconstruction. The converter/tracker also serves as an electron-positron pair detector for gamma-rays up to 100 MeV. The initial continental US flight will be used to determine the sub-orbital atmospheric backgrounds and search for polarized gamma-emission for the Crab pulsar. Longer southern hemisphere flights with an enhanced instrument will map out the Al-26 emissions from the galactic center region. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:287 / 292
页数:6
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