Adaptive optics with programmable Fourier-based wavefront sensors: a spatial light modulator approach to the LOOPS testbed
Pierre Janin-Potiron, Vincent Chambouleyron, Lauren Schatz, Olivier, Fauvarque, Charlotte Z. Bond, Yannick Abautret, Eduard Muslimov, Kacem, El-Hadi, Jean-Fran\c{c}ois Sauvage, Kjetil Dohlen, Beno\^it Neichel, Carlos, M. Correia, Thierry Fusco

TL;DR
This paper introduces an upgraded adaptive optics testbed using a programmable Spatial Light Modulator to generate phase masks for Fourier-based wavefront sensors, enabling flexible testing of novel sensor concepts in real-time.
Contribution
It presents the integration of a SLM into the LOOPS testbed for dynamic phase mask generation, allowing flexible testing of Fourier-based wavefront sensors.
Findings
Successful generation of phase masks with the SLM
First closed-loop results with various wavefront sensors on the SLM
Demonstration of real-time adaptive optics correction
Abstract
Wavefront sensors encode phase information of an incoming wavefront into an intensity pattern that can be measured on a camera. Several kinds of wavefront sensors (WFS) are used in astronomical adaptive optics. Amongst them, Fourier-based wavefront sensors perform a filtering operation on the wavefront in the focal plane. The most well known example of a WFS of this kind is the Zernike wavefront sensor, and the pyramid wavefront sensor (PWFS) also belongs to this class. Based on this same principle, new WFSs can be proposed such as the n-faced pyramid (which ultimately becomes an axicone) or the flattened pyramid, depending on whether the image formation is incoherent or coherent. In order to test such novel concepts, the LOOPS adaptive optics testbed hosted at the Laboratoire d'Astrophysique de Marseille has been upgraded by adding a Spatial Light Modulator (SLM). This device, placed…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Advanced optical system design · Stellar, planetary, and galactic studies
