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A precise method of monitoring the alignment of two-mirror telescopes, based on a system of synthesized annular holograms

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Abstract

This paper presents the results of a study of the possibility of monitoring the alignment of two-mirror Cassegrain and Ritchey–Crétien telescopes during both fabrication and operation under observatory conditions, as well as in space. The method is based on a system of coaxial synthesized annular holograms as optical compensators and reference optical elements.

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