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Study of the quality of the Zeiss-1000 telescope optical system using the Shack-Hartmann wavefront sensorстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 12 июля 2017 г.
- Авторы: Drabek S.V., Komarov V.V., Potanin S.A., Savvin A.D., Moskvitin A.S., Spiridonova O.I.
- Журнал: Astrophysical Bulletin
- Том: 72
- Номер: 2
- Год издания: 2017
- Первая страница: 206
- DOI: 10.1134/S1990341317020122
- Аннотация: The results of studies of the optics of the 1-m Zeiss-1000 telescope of the SAO RAS by the Shack-Hartmann (SH) method are presented. Using a Shack-Hartmann wavefront sensor (SH WFS) we have adjusted the telescope optical system by means of shifts and tilts of the secondary mirror. The procedure has significantly reduced the aberrations that appeared during the long-term instrument operation. A new method to investigate the surface quality of the mirrors of the Zeiss-1000 being applied, characteristics close to the diffraction limit are achieved. In general, the entire opto-mechanical telescope system provides an image quality of about 0.5 angular seconds at 80% energy level. Study of the quality of the Zeiss-1000 telescope optical system using the Shack-Hartmann wavefront sensor (PDF Download Available). Available from: https://www.researchgate.net/publication/317031025_Study_of_the_quality_of_the_Zeiss-1000_telescope_optical_system_using_the_Shack-Hartmann_wavefront_sensor [accessed May 26, 2017].
- Добавил в систему: Потанин Сергей Александрович