Abstract
The current trend in building medium-size telescopes for wide-field imaging is to use a Ritchey–Chrétien (RC) design with a multilens corrector near the focus. Our goal is to find a cost-effective alternative design to the RC system for seeing-limited observations. We present an all-spherical catadioptric system with a field of view. The system consists of a spherical primary and flat secondary mirror combined with a meniscus lens and followed by a three-lens field corrector. The optical performance is comparable to an equivalent RC system. We conclude that, for telescopes with apertures up to , the catadioptric design is a good alternative to the RC system.
© 2010 Optical Society of America
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