用于硬x射线偏振和光谱成像的小型3D CZT有效载荷

E. Caroli, N. Auricchio, C. Budtz-Jørgensen, R. M. Curado da Silva, G. De Cesare, S. del Sordo, P. Ferrando, J. Galvez, M. Hernanz, J. Isern, I. Kuvvetli, P. Laurent, O. Limousin, J. Maia, A. Meuris, M. Pinto, Nicolas Produit, J. Stephen, A. Zappettini
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引用次数: 1

摘要

目前,人们普遍认为,测量宇宙源高能发射的偏振状态是了解其主动产生机制及其几何结构的关键观测参数。因此,在这个能量范围内工作的新仪器也应该针对这种类型的测量进行优化。在此框架下,我们提出了一种小型高性能成像光谱仪的概念,设计用于100和600 keV之间的极化测量,既适合平流层气球载有效载荷,也适合小型卫星任务。该仪器能够在进行精细光谱测量的同时,对不同类型宇宙射线源的偏振状态进行准确、可靠的测量。具有三维空间分辨率的探测器是基于CZT光谱仪的高度分段配置,设计为高性能散射偏振计。我们根据最近的开发结果和目前正在研究的可能改进报告不同的配置。此外,我们描述了有效载荷的可能基线设计,并提出了偏振可实现灵敏度的蒙特卡罗评估,作为不同探测器特性的函数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A small 3D CZT payload for hard X-ray polarimetry and spectroscopic imaging
Currently, it is widely recognised that a measurement of the polarization status of cosmic sources high energy emission is a key observational parameter to understand the active production mechanism and its geometry. Therefore, new instrumentation operating in this energy range should be optimized also for this type of measurement. In this framework, we present the concept of a small high-performance imaging spectrometer designed for polarimetry between 100 and 600 keV suitable both for a stratospheric balloon-borne payload, and a small satellite mission. This instrument would be able to perform accurate and reliable measurement of the polarization status of different cosmic ray sources types simultaneously with fine spectroscopic measurements. The detector with 3D spatial resolution is based on a CZT spectrometer in a highly segmented configuration designed to operate as a high performance scattering polarimeter. We report on different configuration based on recent development results and possible improvements currently under study. Furthermore, we describe a possible baseline design of the payload and we present Monte Carlo evaluations of the achievable sensitivity for polarisation as a function of different detector characteristics.
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