The PLATO Antarctic site testing observatory

J. S. Lawrence; G. R. Allen; M. C. B. Ashley; C. Bonner; S. Bradley; X. Cui; J. R. Everett; L. Feng; X. Gong; S. Hengst; J. Hu; Z. Jiang; C. A. Kulesa; Y. Li; D. Luong-Van; A. M. Moore; C. Pennypacker; W. Qin; R. Riddle; Z. Shang; J. W. V. Storey; B. Sun; N. Suntzeff; N. F. H. Tothill; T. Travouillon; C. K. Walker; L. Wang; J. Yan; J. Yang; H. Yang; D. York; X. Yuan; X. G. Zhang; Z. Zhang; X. Zhou; Z. Zhu

doi:10.1117/12.787166

10 July 2008 The PLATO Antarctic site testing observatory

J. S. Lawrence, G. R. Allen, M. C. B. Ashley, C. Bonner, S. Bradley, X. Cui, J. R. Everett, L. Feng, X. Gong, S. Hengst, J. Hu, Z. Jiang, C. A. Kulesa, Y. Li, D. Luong-Van, A. M. Moore, C. Pennypacker, W. Qin, R. Riddle, Z. Shang, J. W. V. Storey, B. Sun, N. Suntzeff, N. F. H. Tothill, T. Travouillon, C. K. Walker, L. Wang, J. Yan, J. Yang, H. Yang, D. York, X. Yuan, X. G. Zhang, Z. Zhang, X. Zhou, Z. Zhu

Author Affiliations +

Proceedings Volume 7012, Ground-based and Airborne Telescopes II; 701227 (2008) https://doi.org/10.1117/12.787166
Event: SPIE Astronomical Telescopes + Instrumentation, 2008, Marseille, France

Abstract

Over a decade of site testing in Antarctica has shown that both South Pole and Dome C are exceptional sites for astronomy, with certain atmospheric conditions superior to those at existing mid-latitude sites. However, the highest point on the Antarctic plateau, Dome A, is expected to experience colder atmospheric temperatures, lower wind speeds, and a turbulent boundary layer that is confined closer to the ground. The Polar Research Institute of China, who were the first to visit the Dome A site in January 2005, plan to establish a permanently manned station there within the next decade. As part of this process they conducted a second expedition to Dome A, arriving via overland traverse in January 2008. This traverse involved the delivery and installation of the PLATeau Observatory (PLATO). PLATO is an automated self-powered astrophysical site testing observatory, developed by the University of New South Wales. A number of international institutions have contributed site testing instruments measuring turbulence, optical sky background, and sub-millimetre transparency. In addition, a set of science instruments are providing wide-field high time resolution optical photometry and terahertz imaging of the Galaxy. We present here an overview of the PLATO system design and instrumentation suite.

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J. S. Lawrence, G. R. Allen, M. C. B. Ashley, C. Bonner, S. Bradley, X. Cui, J. R. Everett, L. Feng, X. Gong, S. Hengst, J. Hu, Z. Jiang, C. A. Kulesa, Y. Li, D. Luong-Van, A. M. Moore, C. Pennypacker, W. Qin, R. Riddle, Z. Shang, J. W. V. Storey, B. Sun, N. Suntzeff, N. F. H. Tothill, T. Travouillon, C. K. Walker, L. Wang, J. Yan, J. Yang, H. Yang, D. York, X. Yuan, X. G. Zhang, Z. Zhang, X. Zhou, and Z. Zhu "The PLATO Antarctic site testing observatory", Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 701227 (10 July 2008); https://doi.org/10.1117/12.787166

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