Presentation
28 August 2024 A review of super-resolution enabling tomographic reconstructors in adaptive optics
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Abstract
Recent work by Oberti+22 argued and showed that classical astronomical adaptive-optics tomography performance can be further improved by carefully designing and configuring the system to encompass and exploit any built-in super-resolution (SR) capabilities. Our goal now is to further materialise the concept by outlining the key models to compute SR-enabling tomographic reconstructors for AO. For that we assume the form of a review paper where we (i) clarify how model-and-deploy static reconstructors arise naturally from the solution of the inverse problem and how to make them cope with closed-loop systems, (ii) how this solution is obtained as a limiting-case of a properly-conceived optimal stochastic control problem, (iii) review the two forms of the minimum-mean-squared-error (MMSE) tomographic reconstructors, highlighting the necessary adaptations to accommodate super-resolution, (iii) review the implementation in either dense-format vector-matrix-multiplication or sparse iterative forms and (iv) discuss the implications for runtime and off-line real-time implementations. We illustrate our examples with simulations/on-sky results when possible for 10m and 40m-scale systems.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Carlos M. Correia, Pierre Jouve, Cédric Taïssir Héritier, Guido Agapito, Tom Major, Jesse Cranney, Yoshito H. Ono, Sylvain Oberti, and Avinash Surendran "A review of super-resolution enabling tomographic reconstructors in adaptive optics", Proc. SPIE 13097, Adaptive Optics Systems IX, 130970Z (28 August 2024); https://doi.org/10.1117/12.3020060
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