CNNCat:利用卷积神经网络对康普顿/派尔望远镜中的高能光子进行分类

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Jan Peter Lommler, Uwe Gerd Oberlack
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引用次数: 0

摘要

康普顿/Pair 望远镜的设计目的是提供从亚兆电子伏到 GeV 能量的宇宙光子的光谱分辨图像,它在跟踪探测器和热量计的组合中记录了大量数据。在数据传输带宽有限的情况下,需要进行星载事件分类,以决定优先下链哪些数据。事件分类也是重建数据的第一步,也是最关键的一步。它的结果决定了对事件的进一步处理,即重建类型(康普顿,对),或可能决定丢弃事件。这一阶段的错误会导致重建错误和源信息丢失。我们提出了一种由卷积神经网络驱动的分类算法。它完全基于低级探测器数据,对电磁相互作用的类型进行分类。我们介绍了任务,描述了所使用的架构和数据集,并在拟议的 (e-)ASTROGAM 和类似望远镜的背景下展示了该方法的性能。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
CNNCat: categorizing high-energy photons in a Compton/Pair telescope with convolutional neural networks

A Compton/Pair telescope, designed to provide spectral resolved images of cosmic photons from sub-MeV to GeV energies, records a wealth of data in a combination of tracking detector and calorimeter. Onboard event classification can be required to decide on which data to down-link with priority, given limited data-transfer bandwidth. Event classification is also the first and one of the most crucial steps in reconstructing data. Its outcome determines the further handling of the event, i.e., the type of reconstruction (Compton, pair) or, possibly, the decision to discard it. Errors at this stage result in misreconstruction and loss of source information. We present a classification algorithm driven by a Convolutional Neural Network. It provides classification of the type of electromagnetic interaction, based solely on low-level detector data. We introduce the task, describe the architecture and the dataset used, and present the performance of this method in the context of the proposed (e-)ASTROGAM and similar telescopes.

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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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