New types of prime focus field correctors for Ritchey-Chretien telescopes which have significantly better imaging than those presently in use are discussed. A corrector consisting of two contiguous positive lenses of relatively low power followed by separated negative and positive lenses has been applied to the f/2.7 focus of the Cerro Tololo 4-m telescope. Also considered is a 2.0-deg corrector for the Anglo-Australian 2.9-m telescope.
CITATION STYLE
Wynne, C. G. (1989). Wide field imaging. Monthly Notices of the Royal Astronomical Society, 236(1), 47P-50P. https://doi.org/10.1093/mnras/236.1.47p
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