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Studies of the performance of the ATLAS detector using cosmic-ray muons

机译:利用宇宙射线μ子研究ATLAS探测器的性能

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摘要

Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response.
机译:大气中宇宙射线相互作用产生的μ子提供了粒子的高统计量来源,可用于研究ATLAS探测器的性能和校准。宇宙射线μ子可以穿透洞穴并在所有探测器子系统中沉积能量。自2005年安装阶段开始以来,此类事件在检测器的调试中发挥了重要作用,对于了解第一个LHC光束到达之前的时间内的检测器性能尤其重要。在2008年和2009年进行了全球宇宙射线运行,这些数据一直到碰撞数据的早期阶段都被用作校准,对准和检测器监测的工具。这些大型数据集还用于检测器性能研究,包括依赖于不同子系统综合性能的研究。本文介绍了与联合跟踪,轻子识别,射流重建和横向能量缺失有关的性能研究结果。基于宇宙射线事件发生器和探测器响应的完整模拟,将结果与期望值进行比较。

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