DOI | Resolve DOI: https://doi.org/10.1117/12.926854 |
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Author | Search for: Andersen, David R.1; Search for: Bradley, C.; Search for: Lardière, O.; Search for: Blain, C.; Search for: Correia, C.1; Search for: Desmarais, R.; Search for: Gamroth, D.; Search for: Ito, M.; Search for: Jackson, K.; Search for: Lach, P.; Search for: Nash, R.; Search for: Pham, L.; Search for: Véran, J.-P.1 |
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Affiliation | - National Research Council of Canada. National Science Infrastructure
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Format | Text, Article |
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Conference | Adaptive Optics Systems III, July 1-6, 2012, Amsterdam, Netherlands |
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Subject | Alignment technique; Calibration unit; Deformable mirrors; Ground layer; Laser guide star; Multiobject; Multiple source; Phase screen; Wave front sensors; Calibration; Electric appliances; Adaptive optics |
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Abstract | Raven is a Multi-Object Adaptive Optics (MOAO) scientific demonstrator which will be used on-sky at the Subaru observatory. Raven is currently being built at the University of Victoria AO Lab. In this paper, we present an overview of the final Raven design and then describe lab tests involving prototypes of Raven subsystems. The final design includes three open loop wavefront sensors (WFSs), a laser guide star WFS and two figure/truth WFSs. Two science channels, each containing a deformable mirror (DM), feed light to the Subaru IRCS spectrograph. Central to the Raven MOAO system is a Calibration Unit (CU) which contains multiple sources, a telescope simulator including two rotating phase screens and a ground layer DM that can be used to calibrate and test Raven. We are working with the Raven CU and open loop WFSs to test and validate our open loop calibration and alignment techniques. |
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Publication date | 2012-09-13 |
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Series | |
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Language | English |
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Peer reviewed | Yes |
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NPARC number | 21270297 |
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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 | 44f70959-30be-4822-a9db-04ab7ac36c9b |
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Record created | 2014-01-21 |
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Record modified | 2020-04-21 |
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