AUTOMATION AND QUEUE MANAGEMENT FOR NEO SURVEYING AND FOLLOW-UP

被引:0
|
作者
Gibbs, Alex R. [1 ]
Christensen, E. C. [1 ]
Fuls, D. C. [1 ]
Grauer, A. D. [1 ]
Johnson, J. A. [1 ]
Kowalski, R. A. [1 ]
Larson, S. M. [1 ]
Leonard, G. J. [1 ]
Matheny, R. G. [1 ]
Seaman, R. L. [1 ]
Shelly, F. C. [1 ]
机构
[1] Univ Arizona, Lunar & Planetary Lab, 1629 E Univ Blvd, Tucson, AZ 85721 USA
来源
V WORKSHOP ON ROBOTIC AUTONOMOUS OBSERVATORIES, 2017 | 2019年 / 51卷
关键词
methods: observational; minor planets; asteroids:; general; surveys;
D O I
10.22201/ia.14052059p.2019.51.17
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Catalina Sky Survey (CSS) at the University of Arizona operates three telescopes full-time in the search for near-Earth objects (NEOs). CSS has discovered 47% of all known NEOs, reported over 46 million asteroid positions, and our photometry has been used to generate light curves for half a billion sources. Our telescopes are capable of highly automated data acquisition and we are working on making one of them autonomous from target selection to reporting of high-confidence data. I cover various aspects of the high-level automation at CSS, with emphasis on the queue manager software, and give a brief overview of CSS and our results.
引用
收藏
页码:105 / 110
页数:6
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