DOI | Resolve DOI: https://doi.org/10.1117/12.672566 |
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Author | Search for: Szeto, Kei1; Search for: Andersen, David1; Search for: Crampton, David1; Search for: Morris, Simon; Search for: Lloyd-Hart, Michael; Search for: Myers, Richard; Search for: Jensen, Joseph B.; Search for: Fletcher, Murray1; Search for: Gardhouse, W. Rusty; Search for: Milton, N. Mark; Search for: Pazder, John1; Search for: Stoesz, Jeff; Search for: Simons, Doug; Search for: Véran, Jean-Pierre1 |
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Editor | Search for: McLean, Ian S.; Search for: Iye, Masanori |
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Affiliation | - National Research Council of Canada. NRC Herzberg Institute of Astrophysics
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Format | Text, Article |
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Conference | Ground-based and Airborne Instrumentation for Astronomy, May 24, 2006, Orlando, Florida, United States |
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Abstract | We describe a simple and cost-effective concept for implementing a Ground Layer Adaptive Optics (GLAO) system on Gemini that will feed all instruments mounted at the Cassegrain focus. The design concept can provide a GLAO correction to any of the current or future seeing-limited optical or near-infrared Gemini instruments. The GLAO design uses an adaptive secondary mirror and provides a significant upgrade to the current telescope acquisition-and-guide system while reusing and building upon the existing telescope facilities and infrastructure. This paper discusses the overall design of the GLAO system including optics, opto-mechanics, laser guide star facilities, natural and laser guide stars wavefront sensors. Such a GLAO system will improve the efficiency of essentially all observations with Gemini and also will help with scheduling since it virtually eliminates poor seeing. |
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Publication date | 2006-06-28 |
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In | |
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Series | |
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Language | English |
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Peer reviewed | Yes |
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NPARC number | 13054241 |
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Export citation | Export as RIS |
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Report a correction | Report a correction (opens in a new tab) |
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Record identifier | e6b5c0fe-d70d-4988-b24b-a33f9f713e9d |
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Record created | 2009-11-25 |
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Record modified | 2023-06-22 |
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