Subaru Telescope —History, active/adaptive optics, instruments, and scientific achievements—

Author:

IYE Masanori1

Affiliation:

1. National Astronomical Observatory of Japan

Publisher

Japan Academy

Subject

General Physics and Astronomy,General Agricultural and Biological Sciences,General Medicine

Reference165 articles.

1. 1) Sandage, A., Osmer, P., Giacconi, R., Gorenstein, P., Gursky, H., Waters, J. et al. (1966) On the optical identification of Sco X-1. ApJ 146, 316–321.

2. 2) Gursky, H., Giacconi, R., Gorenstein, P., Waters, J.R., Oda, M., Bradt, H. et al. (1966) A measurement of the angular size of the X-ray source Sco X-1. ApJ 144, 1249–1252.

3. 3) Fujita, Y. (1970) Interpretation of Spectra and Atmospheric Structure in Cool Stars. University of Tokyo Press, Tokyo.

4. 4) Yamashita, Y. (1972) The C-classification of the spectra of carbon stars. Ann. Tokyo Astron. Obs. 2nd Ser. 13, 167–217.

5. 5) Robinson, B. (1981) 4-meter primary mirror – KPNO. Kitt Peak National Observatory News Letter 14, 5.

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Active lateral support system for a thin 1-meter meniscus mirror with virtual fixed points;Journal of Astronomical Telescopes, Instruments, and Systems;2023-06-16

2. Development of active optics for thin meniscus mirrors in 1-meter-class telescopes;Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation V;2022-08-29

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