A non-linear curvature wavefront sensor for the Subaru Telescope’s AO3k system
Affiliation
Steward Observatory, University of ArizonaCollege of Optical Sciences, University of Arizona
Issue Date
2023-10-05
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SPIECitation
Ahn, K., Guyon, O., Lozi, J., Vievard, S., Deo, V., Lallement, M., & Bragg, J. C. (2023, October). A non-linear curvature wavefront sensor for the Subaru telescope’s AO3k system. In Techniques and Instrumentation for Detection of Exoplanets XI (Vol. 12680, pp. 75-83). SPIE.Rights
© 2023 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
A few years ago, we started upgrading AO188 into AO3k, including the real-time control system, laser guide star system, deformable mirror (DM), and wavefront sensors (WFSs). In this paper, we present the development of a non-linear curvature WFS (nlCWFS) as a new visible WFS for the upgraded AO3k system. We also introduce the optical and optomechanical design of the nlCWFS. The nlCWFS has two new features: one is the dual-stroke linear mode, and the other one is to deploy non-linear wavefront reconstruction. The dual-stroke linear mode provides a good sensitivity for both low- and high-order aberrations. Also, the non-linear wavefront reconstruction provides a large dynamic range. By combining the linear and non-linear methods, the nlCWFS takes both advantages. Finally, we present laboratory demonstration results of closed-loop experiments in the lab with linear and non-linear wavefront reconstruction algorithms. © 2023 SPIE.Note
Immediate accessISSN
0277-786XISBN
978-151066574-3Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2676667