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PILOT – the Pathfinder for an International Large Optical Telescope

Published online by Cambridge University Press:  23 May 2007

N. Epchtein ,
M. Candidi ,
J.W.V. Storey ,
M.C.B. Ashley ,
M.G. Burton  and
J.S. Lawrence
J.W.V. Storey*
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
M.C.B. Ashley
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
M.G. Burton
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
J.S. Lawrence
Affiliation:
School of Physics, University of New South Wales, Sydney, NSW 2052, Australia
*
[email protected]
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Abstract

PILOT is proposed as a partnership between Australia and Europe todevelop a 2.4 m optical/infrared telescope for Dome C,Antarctica. Funding for a detailed designed study is being soughtfrom Australian sources, with a view to commencing construction inearly 2008. The current “strawman” design is for an f/10 dualNasmyth configuration with provision for both a silicon carbide fasttip-tilt secondary mirror for the thermal infrared, and an adaptivesecondary mirror to achieve diffraction-limited imaging atwavelengths as short as V-band.


Type
Research Article
Information
European Astronomical Society Publications Series , Volume 25: 1st ARENA Conference on "Large Astronomical Infrastructures at CONCORDIA, prospects and constraints for Antarctic Optical/IR Astronomy" , 2007 , pp. 255 - 259
Copyright
© EAS, EDP Sciences, 2007

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