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Proceedings Paper

PILOT: a wide-field telescope for the Antarctic plateau
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Paper Abstract

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed Australian/European optical/infrared telescope for Dome C on the Antarctic Plateau, with target first light in 2012. The telescope is 2.4m diameter, with overall focal ratio f/10, and a 1 degree field-of-view. It is mounted on a 30m tower to get above most of the turbulent surface layer, and has a tip-tilt secondary for fast guiding. In median seeing conditions, it delivers 0.3" FWHM wide-field image quality, from 0.7-2.5 microns. In the best quartile of conditions, it delivers diffraction-limited imaging down to 1 micron, or even less with lucky imaging. The major challenges have been (a) preventing frost-laden external air reaching the optics, (b) overcoming residual surface layer turbulence, (c) keeping mirror, telescope and dome seeing to acceptable levels in the presence of large temperature variations with height and time, (d) designing optics that do justice to the site conditions. The most novel feature of the design is active thermal and humidity control of the enclosure, to closely match the temperature of external air while preventing its ingress.

Paper Details

Date Published: 10 July 2008
PDF: 9 pages
Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 70124F (10 July 2008); doi: 10.1117/12.788651
Show Author Affiliations
Will Saunders, Anglo-Australian Observatory (Australia)
Peter Gillingham, Anglo-Australian Observatory (Australia)
Andrew McGrath, Anglo-Australian Observatory (Australia)
Roger Haynes, Anglo-Australian Observatory (Australia)
Jurek Brzeski, Anglo-Australian Observatory (Australia)
John Storey, Univ. of New South Wales (Australia)
Jon Lawrence, Univ. of New South Wales (Australia)


Published in SPIE Proceedings Vol. 7012:
Ground-based and Airborne Telescopes II
Larry M. Stepp; Roberto Gilmozzi, Editor(s)

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