Roboscheduler: coordinating 50,000 observations over the 5 years of SDSS-V

被引:0
作者
Donor, John [1 ]
Blanton, Michael R. [2 ]
Covey, Kevin [3 ]
Dwelly, Tom [4 ]
Medan, Ilija [5 ]
Sanchez-Gallego, Jose [6 ]
机构
[1] Texas Christian Univ, Dept Phys & Astron, TCU Box 298840, Ft Worth, TX 76129 USA
[2] NYU, Ctr Cosmol & Particle Phys, Dept Phys, 726 Broadway Rm 1005, New York, NY 10003 USA
[3] Western Washington Univ, Dept Phys & Astron, 516 High St, Bellingham, WA 98225 USA
[4] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany
[5] Vanderbilt Univ, Dept Phys & Astron, VU Stn 1807, Nashville, TN 37235 USA
[6] Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA
来源
SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY VIII | 2024年 / 13101卷
基金
美国国家科学基金会;
关键词
Survey Scheduling;
D O I
10.1117/12.3020292
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The new Focal Plane Systems (FPS) built for the fifth iteration of the Sloan Digital Sky Survey (SDSS-V) at Las Campanas Observatory and Apache Point Observatory each consist of 500 robotic fiber positioners, feeding optical and infrared multi-object spectrographs, that can be arranged in configurations, internally called "designs", to match science targets in the night sky. SDSS-V plans to observe roughly 50,000 of these designs over the 5 year survey, with up to 30 being observed on a single night at each observatory. Besides the sheer volume of designs, there are strict time domain requirements ("cadences") that must be respected in order to complete the signature SDSS time domain surveys. This complex set of requirements necessitates software that can ensure cadence requirements are always respected, in addition to normal observing requirements such as maximum skybrightness, moon distance, etc., while also optimizing the designs scheduled in a night to ensure all designs are completed by the end of the survey. We present an overview of the roboscheduler package which was developed to solve these problems.
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页数:5
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