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End-to-end data acquisition pipeline for the Cherenkov Telescope Array

机译:Cherenkov望远镜阵列的端到端数据采集管道

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摘要

The Cherenkov Telescope Array (CTA) will operate several types of telescopesand cameras. The individual camera trigger rates will vary much - from 0.6 to15 kHz - while the content of the raw data will be heterogeneous. Raw datastreams of up to 43 Gbps per telescope must be handled efficiently, from thecamera front-ends down to the on-site repository and real-time analysis. Inaddition, the system must transcode all raw data to a common, pre-calibratedformat. We will present the pipeline that we propose to implement this dataacquisition pipeline. It will format the raw data to a common structure,provide facilities to run camera-specific algorithms and compress and writedata to the on-site repository. We will also present the Python interface thatallows the analysis pipeline to access the data. Eventually, the two strategiesforeseen to interface the camera servers will be detailed and the currentstatus of the developments for CTA will be given, with the last performancefigures measured.
机译:切伦科夫望远镜阵列(CTA)将运行几种类型的望远镜和照相机。各个相机的触发速率将相差很大-从0.6到15 kHz-而原始数据的内容将是异构的。从摄像机前端到现场存储库和实时分析,必须有效处理每台望远镜高达43 Gbps的原始数据流。此外,系统必须将所有原始数据转码为通用的,预先校准的格式。我们将介绍为实现此数据采集管道而建议的管道。它将原始数据格式化为通用结构,提供运行特定于相机的算法并将数据压缩和写入现场存储库的工具。我们还将展示Python接口,该接口允许分析管道访问数据。最终,将详细介绍连接相机服务器的两种预见策略,并给出CTA的最新发展现状,并评估最后的性能指标。

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