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Astrophysics from Dome A

Published online by Cambridge University Press:  13 November 2008

H. Zinnecker ,
N. Epchtein ,
H. Rauer ,
N.F.H. Tothill ,
C.A. Kulesa ,
C.K. Walker ,
M.C.B. Ashley ,
C. Bonner ,
X. Cui  and
J. Everett
...Show all authors
N.F.H. Tothill*
Affiliation:
School of Physics, University of Exeter, Stocker Road, Exeter, EX4 4QL, UK
C.A. Kulesa
Affiliation:
Steward Observatory, 933 N. Cherry Ave., Tucson, AZ 85721, USA
C.K. Walker
Affiliation:
Steward Observatory, 933 N. Cherry Ave., Tucson, AZ 85721, USA
M.C.B. Ashley
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
C. Bonner
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
X. Cui
Affiliation:
Nanjing Institute of Astronomical Optics Technology, China
J. Everett
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
L. Feng
Affiliation:
Purple Mountain Observatory, China
S. Hengst
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
J. Hu
Affiliation:
National Astronomical Observatory of China, China
Z. Jiang
Affiliation:
National Astronomical Observatory of China, China
J.S. Lawrence
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
Y. Li
Affiliation:
Polar Research Institute of China, China
D. Luong-Van
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
A.M. Moore
Affiliation:
Caltech Optical Observatories, 1200 E. California Blvd., Pasadena, CA 91125, USA
C. Pennypacker
Affiliation:
Space Sciences Laboratory, U C Berkeley, CA, USA
W. Qin
Affiliation:
Polar Research Institute of China, China
R. Riddle
Affiliation:
TMT Project, Pasadena, CA, USA
J.W.V. Storey
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
Z. Shang
Affiliation:
Tianjin Normal University, China
B. Sun
Affiliation:
Polar Research Institute of China, China
T. Travouillon
Affiliation:
TMT Project, Pasadena, CA, USA
L. Wang
Affiliation:
Purple Mountain Observatory, China
Z. Xu
Affiliation:
National Astronomical Observatory of China, China
H. Yang
Affiliation:
Polar Research Institute of China, China
J. Yan
Affiliation:
Purple Mountain Observatory, China
D.G. York
Affiliation:
Dept. of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA
X. Yuan
Affiliation:
Nanjing Institute of Astronomical Optics Technology, China
Z. Zhu
Affiliation:
Purple Mountain Observatory, China
*
nfht@astro.ex.ac.uk
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Abstract

Dome A, the summit of the Antarctic plateau, is expected to have even better atmospheric conditions for ground-based astronomy than Dome C. Instruments to evaluate and exploit Dome A's astronomical potential must operate within logistical constraints, which are currently very stringent. Instrumentation now at Dome A exemplifies the techniques and solutions required by this environment. Future instrumentation and infrastructure will allow the qualities of the site to be exploited much more fully.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 33: 2nd ARENA Conference: The Astrophysical Science Cases at Dome C , 2008 , pp. 301 - 306
Copyright
© EAS, EDP Sciences, 2008

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References

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