Design Of The Apache Point Observatory 3.5m Telescope III. Primary Mirror Support System

Author(s):  
Edward J. Mannery ◽  
Walter A. Siegmund ◽  
M. Thomas Hull
Author(s):  
Alikhan Basheer ◽  
Sripadmanaban Nadar Sriram ◽  
Vineeth Valsan ◽  
Kambhala Sudharsan ◽  
Viswanatha Narasimhiah ◽  
...  

1984 ◽  
Vol 79 ◽  
pp. 75-93 ◽  
Author(s):  
G. Ballio ◽  
R. Contro ◽  
C. Poggi ◽  
O. Citterio

A way to follow in order to reduce the weight of the primary mirror is to accept an higher ratio diameter-thickness and to find a remedy to the consequent greater deformability of the mirror by an active control system of it. A technique using closed loop active optics control has been proposed in references.In these papers, a coherent scheme of active optics control for the ESO New Technology Telescope (NTT) was presented, based on analysis of the image errors in terms of an appropriate polynomial (the ESO off-line telescope test polynomial) and the production of equivalent correction terms by force modulation of the primary axial support.


2018 ◽  
Vol 55 (10) ◽  
pp. 100002
Author(s):  
徐宏 Xu Hong ◽  
杨利伟 Yang Liwei ◽  
杨会生 Yang Huisheng

2010 ◽  
Vol 49 (8) ◽  
pp. 1234 ◽  
Author(s):  
Pietro Schipani ◽  
Sergio D'Orsi ◽  
Luigi Ferragina ◽  
Davide Fierro ◽  
Laurent Marty ◽  
...  

2008 ◽  
Author(s):  
Eric C. Williams ◽  
Curtis Baffes ◽  
Terry Mast ◽  
Jerry Nelson ◽  
Benjamin Platt ◽  
...  

2017 ◽  
Vol 46 (9) ◽  
pp. 918003
Author(s):  
赵勇志 Zhao Yongzhi ◽  
邵 亮 Shao Liang ◽  
明 名 Ming Ming ◽  
吕天宇 Lv Tianyu ◽  
刘昌华 Liu Changhua

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