A low-cost, high-speed, very high-order Shack-Hartmann sensor for testing TMT deformable mirrors
Mojtaba Taheri (1, 2), David Andersen (3), Jean-Pierre Veran (4),, Olivier Lardi\`ere (4) ((1) Laboratoire d'Astrophysique de Marseille, (2), W.M. Keck Observatory, (3) TMT International Observatory, (4) NRC Herzberg, Astronomy, Astrophysics)

TL;DR
This paper presents a low-cost, high-speed, high-order Shack-Hartmann wavefront sensor designed for testing large deformable mirrors in adaptive optics systems, capable of high-resolution measurements at 50 FPS.
Contribution
The authors developed a cost-effective, very high-order Shack-Hartmann sensor with 248+ sub-apertures, enabling detailed testing of large deformable mirrors for advanced telescopes.
Findings
Achieved 50 FPS wavefront recording at full resolution.
Successfully sampled large deformable mirrors with over 248 sub-apertures.
Kept total sensor cost below $20,000 USD.
Abstract
The Thirty Meter Telescope will use a sophisticated adaptive optics system called NFIRAOS. This system utilizes two deformable mirrors conjugate to 0 km and 11.2 km to apply a Multi-Conjugate Adaptive Optics (MCAO) correction over a 2 arcminute field of view. DM0 and DM11 have 63 and 75 actuators across their respective diameters. To study the behavior of these mirrors, we have developed a low-cost, very high-order Shack-Hartmann Wavefront Sensor (WFS). We will use our WFS to calibrate the flatness of the DMs and measure the influence functions of the actuators. NFIRAOS is cooled to reduce the thermal emissivity of optical surfaces visible to the science detectors, so we will also measure the behaviour of the DMs in both warm and cold environments. As the cold chamber is prone to vibrations, a WFS is preferred to a phase-shifting interferometer. Our design was driven by the need to be…
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