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This book provides a unified treatment of the characteristics of
telescopes of all types, both those whose performance is set by
geometrical aberrations and the effect of the atmosphere, and those
diffraction-limited telescopes designed for observations from above
the atmosphere. The emphasis throughout is on basic principles,
such as Fermat's principle, and their application to optical
systems specifically designed to image distant celestial
sources. * Geometrical aberration theory based on Fermat's
principle
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