The Read-Out and Control System of the DES Camera (SISPI)

被引:2
作者
Honscheid, K. [1 ,2 ]
Abbott, T.
Annis, J.
Buckley-Geer, E. [3 ]
Castander, F. [4 ]
Eiting, J. [1 ,2 ]
Gladders, M. [5 ]
Haney, M.
Karliner, I.
Kau, D.
Kuehn, K. [1 ]
Kuhlmann, S.
Qian, T. [6 ]
Selen, M. [6 ]
Thaler, J. [6 ]
Tucker, D.
Zhao, A. [7 ]
机构
[1] Ohio State Univ, Columbus, OH 43210 USA
[2] Natl Opt Astron Observ, Tucson, AZ USA
[3] Fermilab Natl Accelerator Lab, Batavia, IL USA
[4] IEEC, Barcelona, Spain
[5] Univ Chicago, Chicago, IL USA
[6] Univ Illinois, Urbana, IL USA
[7] Argonne Natl Lab, Argonne, IL USA
来源
ADVANCED SOFTWARE AND CONTROL FOR ASTRONOMY II, PTS 1 & 2 | 2008年 / 7019卷
基金
美国国家科学基金会; 英国科学技术设施理事会;
关键词
Dark Energy Survey; data acquisition; control system; camera; survey; Blanco; CTIO;
D O I
10.1117/12.787926
中图分类号
TP [自动化技术、计算机技术];
学科分类号
0812 ;
摘要
We describe the data acquisition and control system of the Dark Energy Camera (DECam), which will be the primary instrument used in the Dark Energy Survey (DES). DECam will be a 3 sq. deg. mosaic camera mounted at the prime focus of the Blanco 4m telescope at the Cerro-Tololo International Observatory (CTIO). The DECam data acquisition system (SISPI) is implemented as a distributed multi-processor system with a software architecture built on the Client-Server and Publish-Subscribe design patterns. The underlying message passing protocol is based on the SML inter-process communication software developed at CTIO [1]. For the DECam read-out and control system this software package was ported from LabVIEW to the Python and C programming languages. A shared variable system was added to support exchange of telemetry data and other information between different components of the system. In this paper we discuss the SISPI architecture, new concepts used in the design of the infrastructure software and provide an overview of the remaining components of the DES read-out and control system.
引用
收藏
页数:10
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