An off-axis, wide-field, diffraction-limited, reflective Schmidt Telescope
Abstract
Off-axis telescopes with unobstructed pupils offer great advantages in terms of emissivity, throughput, and diffractionlimited energy concentration. For most telescope designs, implementation of an off-axis configuration imposes enormous penalties in terms of cost, optical difficulty and performance, and for this reason off-axis telescopes are rarely constructed. However, for the reflective Schmidt design, implementation of an off-axis configuration is very straightforward, and involves only a modest optical penalty. Moreover, the reflective Schmidt gets particular benefits, avoiding the obstruction of its large focal plane and support column, and gaining a highly accessible, gravity-invariant prime focus, capable of accommodating very large instrumentation. We present an off-axis f/8 reflective Schmidt design for the proposed 'KDUST' Chinese infrared telescope at Dome A on the Antarctic plateau, which offers simultaneous diffraction-limited NIR imaging over 1°, and close to diffraction-limited imaging out to 2° for fibre-fed NIR spectroscopy.
- Publication:
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Ground-based and Airborne Telescopes III
- Pub Date:
- July 2010
- DOI:
- arXiv:
- arXiv:1008.1235
- Bibcode:
- 2010SPIE.7733E..3CS
- Keywords:
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- Astrophysics - Instrumentation and Methods for Astrophysics
- E-Print:
- 7 pages, Proc. SPIE 7733-118