Automation of the AST3 optical sky survey from Dome A, Antarctica

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Ma, Bin, Hu, Yi, Shang, Zhaohui, Hu, Keliang, Wang, Yongjiang, Yang, Xu, Ashley, Michael C B, Yuan, Xiangyan, Wang, Lifan
• Other Authors: National Basic Research Program of China, National Natural Science Foundation of China, Australian Antarctic Division, Astronomy Australia Limited
• Format: Article in Journal/Newspaper
• Language: English
• Published: Oxford University Press (OUP) 2020
• Subjects: Antarc*; Antarctic; Antarctica
• Online Access: http://dx.doi.org/10.1093/mnras/staa1730; http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa1730/33398601/staa1730.pdf; http://academic.oup.com/mnras/article-pdf/496/3/2768/33451617/staa1730.pdf

ABSTRACT The 0.5-m Antarctic Survey Telescopes (AST3) were designed for time-domain optical/infrared astronomy. They are located in Dome A, Antarctica, where they can take advantage of the continuous dark time during winter. Since the site is unattended in winter, everything for the operation, from observing to data reduction, had to be fully automated. Here, we present a brief overview of the AST3 project and some of its unique characteristics due to its location in Antarctica. We summarize the various components of the survey, including the customized hardware and software, that make complete automation possible.