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CSTAR and future plans for Dome A

Published online by Cambridge University Press:  21 October 2010

Xiangqun Cui
Xiangqun Cui*
Affiliation:
National Astronomical Observatories/Nanjing Institute of Astronomical Optics and Technology, CAS
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Abstract

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The first set of Chinese Antarctic telescopes at Dome A is called CSTAR. It consists of four 14.5 cm wide-field telescopes and was installed at Dome A during the traverse of 2007/2008. CSTAR successfully operated for 135 days in 2008 and for more than 200 days in 2009. This paper briefly introduces recent developments in Chinese Antarctic astronomy and their international collaborative activities. It also describes future plans for Dome A, as the building of Kunlun Station began in January of this year.

Keywords

AntarcticaTelescopesSite Testing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 639 - 640
Copyright
Copyright © International Astronomical Union 2010

References

Cui, X. Q., et al. 2008, Proc. SPIE 7012, 70122DCrossRefGoogle Scholar
Gong, X. F., et al. 2008, Proc. SPIE 7012, 701848CrossRefGoogle Scholar
Kulesa, C. A, et al. 2008, Proc. SPIE 7012, 701249CrossRefGoogle Scholar
Lawrence, J. S., et al. 2008, Proc. SPIE 7012, 701227CrossRefGoogle Scholar
Lawrence, J. S., et al. 2008, Rev. Sci. Inst. in pressGoogle Scholar
Tothill, N., et al. 2008, Proc. EAS 33, 301Google Scholar
Yang, H. G., et al. 2009, PASP 121, 174CrossRefGoogle Scholar
Yuan, X. Y., et al. 2008, Proc. SPIE 7012, 70124GCrossRefGoogle Scholar