摘要: The third Antarctic Survey Telescope array instrument at Dome A in
Antarctica, the AST3-3 telescope, has been in commissioning from March 2021. We
deployed AST3-3 at the Yaoan astronomical station in Yunnan Province for an
automatic time-domain survey and follow-up observations with an optimised
observation and protection system. The telescope system of AST3-3 is similar to
that of AST3-1 and AST3-2, except that it is equipped with a 14K~$ \times$~10K
QHY411 CMOS camera. AST3-3 has a field of view of $1.65^\circ \times
1.23^\circ$ and is currently using the $g$ band filter. During commissioning at
Yaoan, AST3-3 aims to conduct an extragalactic transient survey, coupled with
prompt follow-ups of opportunity targets. In this paper, we present the
architecture of the AST3-3 automatic observation system. We demonstrate the
data processing of observations by representatives SN 2022eyw and GRB 210420B.
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分类:
天文学
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天文学
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引用:
ChinaXiv:202303.04876
(或此版本
ChinaXiv:202303.04876V1)
DOI:10.12074/202303.04876V1
CSTR:32003.36.ChinaXiv.202303.04876.V1
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科创链TXID:
aeb9d3f6-a3b3-428f-bf31-75e72ef113a1
- 推荐引用方式:
Tianrui Sun,Xiaoyan Li,Lei Hu,Kelai Meng,Zijian Han,Maokai Hu,Zhengyang Li,Haikun Wen,Fujia Du,Shihai Yang,Bozhong Gu,Xiangyan Yuan,Yun Li,Huihui Wang,Lei Liu,Zhenxi Zhu,Xuehai Huang,Chengming Lei,Lifan Wang,Xuefeng Wu.Antarctic Survey Telescope 3-3: Overview, System Performance and
Preliminary Observations at Yaoan, Yunnan.中国科学院科技论文预发布平台.[ChinaXiv:202303.04876V1]
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