AstroPix:用于未来伽马射线望远镜的新型单片有源像素硅传感器

A. Steinhebel, H. Fleischhack, N. Striebig, Manoj Jadhav, Y. Suda, R. Luz, C. Kierans, R. Caputo, H. Tajima, R. Leys, I. Perić, J. Metcalfe, J. Perkins
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引用次数: 5

摘要

天基γ射线望远镜,如费米大面积望远镜,已经使用单面硅带探测器,以高分辨率跟踪由初级γ射线产生的二次带电粒子。在keV-MeV望远镜瞄准的较低能量下,事件重建需要单个探测器内的二维位置信息,特别是在康普顿区域。这项工作描述了单片CMOS有源像素硅传感器的发展- astropix -作为一种用于未来γ射线望远镜的新技术。基于专为大型强子对撞机ATLAS探测器设计的传感器(ATLASPix), AstroPix具有在保持高性能的同时以低功耗降低噪声的潜力。这是通过每个CMOS像素的双重检测和读出功能实现的。本文将介绍AstroPix的开发和测试现状,以及对未来测试和应用的展望。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
AstroPix: novel monolithic active pixel silicon sensors for future gamma-ray telescopes
Space-based γ-ray telescopes such as the Fermi Large Area Telescope have used single sided silicon strip detectors to track secondary charged particles produced by primary γ-rays with high resolution. At the lower energies targeted by keV-MeV telescopes, two dimensional position information within a single detector is required for event reconstruction—especially in the Compton regime. This work describes the development of monolithic CMOS active pixel silicon sensors—AstroPix—as a novel technology for use in future γ-ray telescopes. Based upon sensors (ATLASPix) designed for use in the ATLAS detector at the Large Hadron Collider, AstroPix has the potential to maintain high performance while reducing noise with low power consumption. This is achieved with the dual detection and readout capabilities in each CMOS pixel. The status of AstroPix development and testing, as well as outlook for future testing and application, will be presented.
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