AstroPix: Status and Outlook of Monolithic Active Pixel Sensors for Future Gamma-ray Telescopes

A. Steinhebel, R. Caputo, H. Fleischhack, N. Striebig, Manoj Jadhav, Y. Suda, R. Luz, Daniel E. Violette, C. Kierans, H. Tajima, Y. Fukazawa, R. Leys, I. Perić, J. Metcalfe, M. Negro, J. Perkins
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引用次数: 1

Abstract

Space-based gamma-ray telescopes such as the Fermi Large Area Telescope have used single sided silicon strip detectors to measure the position of charged particles produced by incident gamma rays with high resolution. At energies in the Compton regime and below, two dimensional position information within a single detector is required. Double sided silicon strip detectors are one option; however, this technology is difficult to fabricate and large arrays are susceptible to noise. This work outlines the development and implementation of monolithic CMOS active pixel silicon sensors, AstroPix, for use in future gamma-ray telescopes. Based upon detectors designed using the HVCMOS process at the Karlsruhe Institute of Technology, AstroPix has the potential to maintain the high energy and angular resolution required of a medium-energy gamma-ray telescope while reducing noise with the dual detection-and-readout capabilities of a CMOS chip. The status of AstroPix development and testing as well as outlook for application in future telescopes is presented.
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AstroPix:用于未来伽马射线望远镜的单片有源像素传感器的现状与展望
像费米大面积望远镜这样的天基伽玛射线望远镜已经使用单面硅带探测器,以高分辨率测量入射伽玛射线产生的带电粒子的位置。在康普顿能级及以下的能量下,需要单个探测器内的二维位置信息。双面硅条探测器是一种选择;然而,这种技术很难制造,而且大型阵列容易受到噪声的影响。这项工作概述了单片CMOS有源像素硅传感器AstroPix的开发和实现,用于未来的伽马射线望远镜。基于卡尔斯鲁厄理工学院采用HVCMOS工艺设计的探测器,AstroPix有可能保持中等能量伽玛射线望远镜所需的高能量和角分辨率,同时通过CMOS芯片的双重探测和读出功能降低噪声。介绍了AstroPix的研制和测试现状,并展望了AstroPix在未来望远镜中的应用前景。
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