Various Wavefront Sensing and Control Developments on the Santa Cruz Extreme AO Laboratory (SEAL) Testbed
Benjamin L. Gerard, Javier Perez-Soto, Vincent Chambouleyron, Maaike, A.M. van Kooten, Daren Dillon, Sylvain Cetre, Rebecca Jensen-Clem, Qiang Fu,, Hadi Amata, Wolfgang Heidrich

TL;DR
This paper reports on three wavefront sensing and control advancements at the SEAL testbed, aiming to improve high contrast imaging of exoplanets by reducing wavefront errors and speckles.
Contribution
It introduces novel developments in multi-WFS SCAO, pupil chopping for focal plane sensing, and enhanced linearity of Pyramid WFS, advancing adaptive optics capabilities.
Findings
Multi-WFS SCAO with FAST and Shack Hartmann WFS demonstrated.
Pupil chopping techniques with amplitude modulator and DM as phase modulator explored.
Enhanced linearity of non-modulated Pyramid WFS shown in laboratory tests.
Abstract
Ground-based high contrast imaging (HCI) and extreme adaptive optics (AO) technologies have advanced to the point of enabling direct detections of gas-giant exoplanets orbiting beyond the snow lines around nearby young star systems. However, leftover wavefront errors using current HCI and AO technologies, realized as "speckles" in the coronagraphic science image, still limit HCI instrument sensitivities to detecting and characterizing lower-mass, closer-in, and/or older/colder exoplanetary systems. Improving the performance of AO wavefront sensors (WFSs) and control techniques is critical to improving such HCI instrument sensitivity. Here we present three different ongoing wavefront sensing and control project developments on the Santa cruz Extreme AO Laboratory (SEAL) testbed: (1) "multi-WFS single congugate AO (SCAO)" using the Fast Atmospheric Self-coherent camera (SCC) Technique…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Stellar, planetary, and galactic studies · Optical Systems and Laser Technology
