Control and systems software for the Cosmology Large Angular Scale Surveyor (CLASS)

Control and systems software for the Cosmology Large Angular Scale Surveyor (CLASS)
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宇宙学大角尺度测量仪 (CLASS) 的控制和系统软件

DOI:
10.1117/12.2561609
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发表时间:
2020
期刊:
114521O
影响因子:
--
通讯作者:
Eimer, Joseph R.
Eimer, Joseph R.
中科院分区:
--
文献类型:
--
作者:
Petroff, Matthew;Appel, John W.;Bennett, Charles L.;Brewer, Michael K.;Chan, Manwei;Chuss, David T.;Cleary, Joseph;Couto, Jullianna D.;Dahal, Sumit;Eimer, Joseph R.

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宇宙学大角尺度勘测者(CLASS)是一组偏振敏感的毫米波望远镜,从智利北部的阿塔卡马沙漠观测到以40 GHz、90 GHz、150 GHz和220 GHz为中心的频段约70%的天空。在这里,我们描述了用于控制望远镜的软件架构,从各种仪器获取数据,安排观测,监测仪器和观测的状态,创建存档数据包,并将数据包传输到北美进行分析。本文还简要讨论了CLASS观测站的计算机和网络结构。该软件和架构自2016年以来一直在使用,全年日夜运行望远镜,并已被证明成功地实现了其设计目标。
The Cosmology Large Angular Scale Surveyor (CLASS) is an array of polarization-sensitive millimeter wave telescopes that observes ∼ 70% of the sky at frequency bands centered near 40 GHz, 90 GHz, 150 GHz, and 220 GHz from the Atacama desert of northern Chile. Here, we describe the architecture of the software used to control the telescopes, acquire data from the various instruments, schedule observations, monitor the status of the instruments and observations, create archival data packages, and transfer data packages to North America for analysis. The computer and network architecture of the CLASS observing site is also briefly discussed. This software and architecture has been in use since 2016, operating the telescopes day and night throughout the year, and has proven successful in fulfilling its design goals.
用于 CLASS 望远镜的可变延迟偏振调制器
DOI: 10.1117/12.2313614
发表时间: 2018
期刊: and Far-Infrared Detectors and Instrumentation for Astronomy IX
影响因子: --
作者:
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发表时间: 2008
期刊:
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发表时间: 2018
期刊: The Astrophysical Journal
影响因子: --
作者:
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