ASTENA:宽带高能天体物理学的创新任务概念

E. Virgilli, F. Frontera, L. Ferro, M. Moita, L. Cavazzini, P. Rosati, C. Guidorzi, M. Orlandini, C. Labanti, E. Caroli, N. Auricchio, J. Stephen, S. del Sordo, L. Amati
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引用次数: 1

摘要

硬x/软伽马射线是宇宙中最强大现象的探测器。与软x射线天体物理学不同,由于难以吸收这种辐射和缺乏聚焦仪器,该波段从技术进步中受益较少。由于这些原因,对创新型软伽马射线仪器的探索迫在眉睫,它们的有效识别和实现迫在眉睫。在这种背景下,在欧洲委员会资助的AHEAD项目框架内,ASTENA实验被提出作为一个创新的任务概念,以面对硬x /伽马射线天文学中一些最具争议的问题。这项工作将通过使用基于突破性技术的仪器来完成,这些仪器能够在广阔的视野中提供前所未有的宽能量通带,高灵敏度观测,同时,亚弧分钟定位伽马射线源和偏振测量。在本文中,我们描述了ASTENA上的仪器,所涉及的技术,利用它们可以实现的性能以及它们的准备水平。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
ASTENA: an innovative mission concept for broadband high-energy astrophysics
Hard-x/soft gamma-rays are probes of the most powerful phenomena in the universe. Unlike soft x-ray astrophysics, this band has benefited less from the technological advancement due to the difficulty to absorb this radiation and to the lack of focusing instrumentation. For these reasons the quest for innovative soft gamma-ray instrumentation is pressing and their effective recognition and realization are urgent. In this context, and in the framework of the AHEAD project, funded by the European Commission, the ASTENA experiment was proposed as an innovative mission concept to face some of the most debated questions in hard x-/gamma-ray astronomy. This effort will be done through the use of instruments based on groundbreaking technologies, capable of providing unprecedented broad energy passband in a wide field of view, high sensitivity observations and, at the same time, sub-arcminute localization of gamma-ray sources and polarimetric measurement. In this paper we describe the instruments on board ASTENA, the technologies involved, the performances achievable with their exploitation and their level of readiness.
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