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

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 observin...

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Bibliographic Details
Main Authors: Ma, Bin, Hu, Yi, Shang, Zhaohui, Hu, Keliang, Wang, Yongjiang, Yang, Xu, Ashley, Michael C. B., Yuan, Xiangyan, Wang, Lifan
Format: Article in Journal/Newspaper
Language:unknown
Published: arXiv 2020
Subjects:
Instrumentation and Methods for Astrophysics astro-ph.IM
FOS Physical sciences
Antarctic
Antarc*
Antarctica
Online Access:https://dx.doi.org/10.48550/arxiv.2006.08128
https://arxiv.org/abs/2006.08128
Description
Summary: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 summarise the various components of the survey, including the customized hardware and software, that make complete automation possible. : 9 pages, 10 figures, accepted for publication in MNRAS

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