Primary Mirror Design
Primary Mirror Design is a methodological framework in telescope optics that specifies the geometric, material, and reflective characteristics of the principal optical element responsible for collecting and focusing incident light, distinguishing it from auxiliary optical components by its fundamental role in determining the imaging performance and structural configuration of the telescope system.
409
Publications
11.9K
Citations
2.2K
Authors
418
Institutions
Publications per year
2017–2026
54
Parents
409
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)
Xiangqun Cui, Yongheng Zhao, Yaoquan Chu et al. · Research in Astronomy and Astrophysics · 2012 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +16
Large Synoptic Survey Telescope: From science drivers to reference design
Željko Ivezić, T. S. Axelrod, W. N. Brandt et al. · Serbian Astronomical Journal · 2008 · 244 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 409
2.2K
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11
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418
University of Arizona
Tucson, United States
25 h-index
309 publications
7.6K citations

Chinese Academy of Sciences
Beijing, China
16 h-index
112 publications
2.8K citations
California Institute of Technology
Pasadena, United States
14 h-index
28 publications
694 citations
Goddard Space Flight Center
Greenbelt, United States
13 h-index
109 publications
5K citations
Jet Propulsion Laboratory
Pasadena, United States
13 h-index
44 publications
2.2K citations
Marshall Space Flight Center
Redstone Arsenal, United States
12 h-index
30 publications
784 citations
Changchun Institute of Optics, Fine Mechanics and Physics
Changchun, China
12 h-index
59 publications
1.5K citations

Las Cumbres Observatory Global Telescope Network
Goleta, United States
12 h-index
46 publications
1.3K citations
1–8 of 418
234 publications · 4.6K citations
31
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28 publications · 990 citations
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AO · 15 publications · 344 citations
12
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12 publications · 469 citations
11
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8 publications · 176 citations
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