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Study of the readout configuration of the GAMMA-400 silicon tracker sensors

机译:GAMMA-400硅跟踪器传感器的读数配置研究

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摘要

The GAMMA-400 satellite is an upcoming international space mission designed to detect gamma and cosmic rays in a broad energy range up to 3 TeV, with an excellent angular and energy resolution. The present design foresees a 10 layers Si-W tracker formed by single sided silicon sensors with 80 μm strip pitch, with a readout pitch of 240 μm; the sensors are arranged in four towers, each one with an area of 50 × 50 cm~2, for a total of more than 150k channels. This paper presents an analysis of the spatial resolution of the proposed readout configuration, compared with different readout approaches, both in terms of readout pitch and strip/implant widths. The study has been performed with two specially developed silicon modules, each one divided into zones with different characteristics. The tests have been performed on the CERN PS-T9 beamline using 10 GeV negative particles.
机译:GAMMA-400卫星是一项即将进行的国际太空飞行任务,旨在探测高达3 TeV的宽能量范围内的伽马射线和宇宙射线,并具有出色的角度和能量分辨率。本设计预见了由单侧硅传感器形成的10层Si-W跟踪器,其条带间距为80μm,读出间距为240μm。传感器排列在四个塔中,每个塔的面积为50×50 cm〜2,总共有超过15万个通道。本文就读出节距和条/植入物宽度而言,与不同的读出方法相比,提出了一种拟议读出结构的空间分辨率分析。该研究是使用两个专门开发的硅模块进行的,每个硅模块分为具有不同特征的区域。测试使用10 GeV负粒子在CERN PS-T9光束线上进行。

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