康普顿对望远镜:下一代MeV伽玛射线天文台的原型

J. Valverde, N. Kirschner, Z. Metzler, L. Smith, N. Cannady, R. Caputo, C. Kierans, I. Liceaga-Indart, A. Moiseev, L. Parker, M. Sasaki, A. Schoenwald, D. Shy, S. Wasti, R. Woolf, A. Bolotnikov, G. Carini, A. W. Crosier, T. Caligure, A. Dellapenna, J. Fried, P. Ghosh, S. Griffin, J. Grove, E. Hays, S. Herrmann, E. Kong, J. Mcenery, J. Mitchell, J. Perkins, B. Phlips, C. Sleator, E. Wulf, A. Zajczyk
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引用次数: 0

摘要

康普顿对(ComPair)望远镜是一个原型,旨在为未来的中能量伽玛射线任务开发必要的技术,并在伽玛射线束和气球飞行中设计、建造和测试原型。ComPair团队建造了一个由4个探测器子系统组成的仪器:一个双面硅条探测器跟踪器,一个新型的高分辨率虚拟飞盘网格碲化镉锌量热计,和一个高能全息碘化铯量热计,所有这些都被一个塑料闪烁体反符合探测器所包围。这些子系统通过康普顿散射和对产生共同探测和表征光子,实现宇宙射线的否决,并且是具有相同架构的空间望远镜的概念验证。ComPair支持的未来中能伽马射线任务将解决Astro2020年十年调查中新信使和新物理学以及宇宙生态系统主题提出的许多问题。在这篇文章中,我们将对ComPair项目进行概述,并进一步介绍气球飞行。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Compton Pair telescope: A prototype for a next-generation MeV gamma-ray observatory
The Compton Pair (ComPair) telescope is a prototype that aims to develop the necessary technologies for future medium energy gamma-ray missions and to design, build, and test the prototype in a gamma-ray beam and balloon flight. The ComPair team has built an instrument that consists of 4 detector subsystems: a double-sided silicon strip detector Tracker, a novel high-resolution virtual Frisch-grid cadmium zinc telluride Calorimeter, and a high-energy hodoscopic cesium iodide Calorimeter, all of which are surrounded by a plastic scintillator anti-coincidence detector. These subsystems together detect and characterize photons via Compton scattering and pair production, enable a veto of cosmic rays, and are a proof-of-concept for a space telescope with the same architecture. A future medium-energy gamma-ray mission enabled through ComPair will address many questions posed in the Astro2020 Decadal survey in both the New Messengers and New Physics and the Cosmic Ecosystems themes. In this contribution, we will give an overview of the ComPair project and steps forward to the balloon flight.
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