Improving the pointing and tracking performance of the Keck telescopes

被引:4
作者
Kwok, Shui Hung [1 ]
Krasuski, Tomas [1 ]
Lyke, Jim [1 ]
Mader, Jeff [1 ]
McCann, Kevin [1 ]
Tsubota, Kevin [1 ]
机构
[1] WM Keck Observ, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743 USA
来源
SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV | 2016年 / 9913卷
关键词
telescope; pointing model; control system;
D O I
10.1117/12.2231825
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Pointing and tracking performance is one of the key metrics that characterize a telescope's overall efficiency. The pointing performance of the Keck telescopes, which use rotary friction encoders to provide position feedback to the control system, has been surpassed by newer large telescopes with more precise encoder systems. While poor tracking can be compensated with guiding, poor blind pointing performance can lead to loss of observing time. In this paper we present a history of the efforts to reduce the impact of poor pointing, as well as the improvements achieved after the installation of new tape encoders. We will discuss the calibration and testing methods and the tools for monitoring and maintaining the desired pointing performance. A comparative analysis of the pointing performance before and after the telescope control system upgrade will also be presented.
引用
收藏
页数:16
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