Editing Reflecting telescope (section)

====Yolo====

The Yolo was developed by Arthur S. Leonard in the mid-1960s.<ref>[https://web.archive.org/web/20030302111137/http://www.atmsite.org/contrib/Holm/yolo/index.html Arthur S. Leonard THE YOLO REFLECTOR]</ref> Like the Schiefspiegler, it is an unobstructed, tilted reflector telescope. The original Yolo consists of a primary and secondary concave mirror, with the same curvature, and the same tilt to the main axis. Most Yolos use [[toroidal reflector]]s. The Yolo design eliminates coma, but leaves significant astigmatism, which is reduced by deformation of the secondary mirror by some form of warping harness, or alternatively, polishing a toroidal figure into the secondary.
Like Schiefspieglers, many Yolo variations have been pursued. The needed amount of toroidal shape 
can be transferred entirely or partially to the primary mirror. In large focal ratios optical assemblies, both primary and secondary mirror can be left spherical and a spectacle correcting lens is added between the secondary mirror and the focal plane (''catadioptric Yolo''). The addition of a convex, long focus tertiary mirror leads to Leonard's ''Solano'' configuration. The Solano telescope doesn't contain any toric surfaces.
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