We first briefly present the last version of the Software Package AIRY, version 6.1, a CAOS-based tool which includes various deconvolution methods, accelerations, regularizations, super-resolution, boundary effects reduction, point-spread function extraction/extrapolation, stopping rules, and constraints in the case of iterative blind deconvolution (IBD). Then, we focus on a new formulation of our Strehl-constrained IBD, here quantitatively compared to the original formulation for simulated near-infrared data of an 8-m class telescope equipped with adaptive optics (AO), showing their equivalence. Next, we extend the application of the original method to the visible domain with simulated data of an AO-equipped 1.5-m telescope, testing also the robustness of the method with respect to the Strehl ratio estimation.
Strehl-constrained reconstruction of post-adaptive optics data & the Software Package AIRY, v. 6.1 / Marcel, Carbillet; Andrea La, Camera; Jeremy, Deguigneta; Prato, Marco; Mario, Bertero; Eric, Aristidia; Patrizia, Boccacci. - ELETTRONICO. - 9148:(2014), p. 91484U. (Intervento presentato al convegno Adaptive Optics Systems IV tenutosi a Montreal nel 22-27 giugno 2014) [10.1117/12.2058525].
Strehl-constrained reconstruction of post-adaptive optics data & the Software Package AIRY, v. 6.1
PRATO, Marco;
2014
Abstract
We first briefly present the last version of the Software Package AIRY, version 6.1, a CAOS-based tool which includes various deconvolution methods, accelerations, regularizations, super-resolution, boundary effects reduction, point-spread function extraction/extrapolation, stopping rules, and constraints in the case of iterative blind deconvolution (IBD). Then, we focus on a new formulation of our Strehl-constrained IBD, here quantitatively compared to the original formulation for simulated near-infrared data of an 8-m class telescope equipped with adaptive optics (AO), showing their equivalence. Next, we extend the application of the original method to the visible domain with simulated data of an AO-equipped 1.5-m telescope, testing also the robustness of the method with respect to the Strehl ratio estimation.Pubblicazioni consigliate
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