arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 2011.03132astro-ph.IMastro-ph.GA
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基于环境和望远镜工作条件的天文图像质量预测

Astronomical Image Quality Prediction based on Environmental and Telescope Operating Conditions

Sankalp Gilda, Yuan-Sen Ting, Kanoa Withington, Matthew Wilson, Simon Prunet, William Mahoney, Sebastien Fabbro, Stark C. Draper, Andrew Sheinis

摘要:

智能调度在地面天文观测站进行的科学曝光序列是非常具有挑战性的。观测时间已超额预定,大气条件不断变化。我们建议使用机器学习来指导天文台的调度。利用加拿大-法国-夏威夷望远镜记录的15年曝光,环境和操作条件档案,我们构建了一个概率数据驱动模型,可以准确预测图像质量。我们证明,通过优化12个通风口的打开和关闭放置在圆顶的望远镜,我们可以减少圆顶引起的湍流和提高望远镜的图像质量(0.05-0.2弧秒)。这意味着$\sim 10-15\%$的暴露时间(因此成本)减少。我们的研究是对当前和下一代望远镜数百万美元操作进行基于数据的优化的第一步。

英文摘要:

Intelligent scheduling of the sequence of scientific exposures taken at ground-based astronomical observatories is massively challenging. Observing time is over-subscribed and atmospheric conditions are constantly changing. We propose to guide observatory scheduling using machine learning. Leveraging a 15-year archive of exposures, environmental, and operating conditions logged by the Canada-France-Hawaii Telescope, we construct a probabilistic data-driven model that accurately predicts image quality. We demonstrate that, by optimizing the opening and closing of twelve vents placed on the dome of the telescope, we can reduce dome-induced turbulence and improve telescope image quality by (0.05-0.2 arc-seconds). This translates to a reduction in exposure time (and hence cost) of $\sim 10-15\%$. Our study is the first step toward data-based optimization of the multi-million dollar operations of current and next-generation telescopes.

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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