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arXiv 1901.08293astro-ph.IM
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SONG原型:机器人望远镜的效率

The SONG prototype: Efficiency of a robotic telescope

M. F. Andersen, F. Grundahl, A. H. Beck, P. Pallé

摘要:

泰德天文台的恒星观测网络组原型望远镜自2014年3月以来一直以科学模式运行。第一年的观测完全是使用高分辨率阶梯光栅摄谱仪进行的。选定了几个小行星地震目标进行科学和技术核查。选择了几颗明亮的次巨星和一颗红巨星,因为这些恒星的振荡幅度很大,周期足够长,很容易被检测到。这些目标也将用于评估仪器,因为对单个目标的长期观察将揭示潜在的问题。在本文中的第一个机器人宋节点的性能进行了描述,以说明在有一个机器人望远镜的效率和可能性。

英文摘要:

The Stellar Observations Network Group prototype telescope at the Teide Observatory has been operating in scientific mode since March 2014. The first year of observations has entirely been carried out using the high resolution echelle spectrograph. Several asteroseismic targets were selected for scientific and technical verification. A few bright subgiants and one red giant were chosen since the oscillations in these stars have large amplitudes and the periods long enough to easily be detected. These targets would also be used for evaluation of the instruments since long term observations of single targets would reveal potential problems. In this paper the performance of the first robotic SONG node is described to illustrate the efficiency and possibilities in having a robotic telescope.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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