Development of the ComPair gamma-ray telescope prototype

D. Shy, C. Kierans, N. Cannady, R. Caputo, S. Griffin, E. Grove, E. Hays, E. Kong, N. Kirschner, I. Liceaga-Indart, J. Mcenery, J. Mitchell, A. Moiseev, L. Parker, J. Perkins, B. Phlips, M. Sasaki, Adam J. Schoenwald, C. Sleator, J. Smith, L. Smith, S. Wasti, R. Woolf, E. Wulf, A. Zajczyk
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引用次数: 6

Abstract

There is a growing interest in the science uniquely enabled by observations in the MeV range, particularly in light of multi-messenger astrophysics. The Compton Pair (ComPair) telescope, a prototype of the AMEGO Probe-class concept, consists of four subsystems that together detect and characterize gamma rays in the MeV regime. A double-sided strip silicon Tracker gives a precise measure of the first Compton scatter interaction and tracks pair-conversion products. A novel cadmium zinc telluride (CZT) detector with excellent position and energy resolution beneath the Tracker detects the Compton-scattered photons. A thick cesium iodide (CsI) calorimeter contains the high-energy Compton and pair events. The instrument is surrounded by a plastic anti-coincidence (ACD) detector to veto the cosmic-ray background. In this work, we will give an overview of the science motivation and a description of the prototype development and performance.
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ComPair伽玛射线望远镜原型机的研制
人们对MeV范围内的观测所特有的科学越来越感兴趣,特别是在多信使天体物理学方面。康普顿对(ComPair)望远镜是AMEGO探测器级概念的原型,由四个子系统组成,它们共同探测和表征MeV状态下的伽马射线。双面条形硅跟踪器提供了第一个康普顿散射相互作用和跟踪对转换产品的精确测量。在跟踪器下方的新型碲化镉锌(CZT)探测器具有优异的位置和能量分辨率,可检测康普顿散射光子。厚碘化铯(CsI)量热计包含高能康普顿事件和对事件。该仪器被一个塑料反巧合(ACD)探测器包围,以阻止宇宙射线背景。在这项工作中,我们将概述科学动机,并描述原型的开发和性能。
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