Paper
28 September 2004 A large reflective Schmidt telescope for the Antarctic plateau
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Abstract
We present a design concept for a 16 metre, wide-field, fixed-axis, all-reflective, segmented f/4 Schmidt telescope to take advantage of the unique possibilities of Antarctica for both optical and near infrared astronomy. The design allows observation of all RA/dec's accessible from Antarctica, with tracking times of several hours. Prime and Cassegrain foci are provided, giving plate scales 300-3000microns/", over fields of view 1.5'-0.5°. Diffraction limited, natural guide-star AO-corrected Kdark images are possible over arc-minute sized fields, over 70% of the sky. The sensitivity, resolution, field of view and cost all compare favourably with current or proposed space or ground-based telescopes.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Will Saunders and Andrew J. McGrath "A large reflective Schmidt telescope for the Antarctic plateau", Proc. SPIE 5489, Ground-based Telescopes, (28 September 2004); https://doi.org/10.1117/12.550870
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Cited by 5 scholarly publications.
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KEYWORDS
Telescopes

Space telescopes

Mirrors

Adaptive optics

James Webb Space Telescope

Optical instrument design

Stars

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