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Removal of Seeing and Instrumental Blur Effects from Astronomical Scanner Observations

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Abstract

The Phillips-Twomey method for solving simultaneous integral equations is applied to the problem of removing blur effects arising from atmospheric and instrumental sources from astronomical observations made with photoelectric area-scanning instruments. Details of the method and the effects of observational errors on the quality of the results are discussed in the context of applications to actual observations of stars and the planet Saturn.

© 1974 Optical Society of America

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