The Santa Cruz Extreme AO Lab (SEAL): Design and First Light
Rebecca Jensen-Clem, Daren Dillon, Benjamin Gerard, M.A.M. van Kooten,, J. Fowler, Renate Kupke, Sylvain Cetre, Dominic Sanchez, Phil Hinz, Cesar, Laguna, David Doelman, Frans Snik

TL;DR
SEAL is a new high-contrast imaging testbed for large telescopes, featuring advanced wavefront control, multiple turbulence simulation options, and diverse wavefront sensors, aiming to improve adaptive optics performance.
Contribution
This paper introduces the design and initial performance results of SEAL, a versatile testbed for advancing wavefront control in high contrast imaging on large telescopes.
Findings
Successful first light demonstration of SEAL.
Integration of multiple wavefront sensors and turbulence simulators.
Initial performance metrics show promising adaptive optics capabilities.
Abstract
The Santa Cruz Extreme AO Lab (SEAL) is a new visible-wavelength testbed designed to advance the state of the art in wavefront control for high contrast imaging on large, segmented, ground-based telescopes. SEAL provides multiple options for simulating atmospheric turbulence, including rotating phase plates and a custom Meadowlark spatial light modulator that delivers phase offsets of up to 6pi at 635nm. A 37-segment IrisAO deformable mirror (DM) simulates the W. M. Keck Observatory segmented primary mirror. The adaptive optics system consists of a woofer/tweeter deformable mirror system (a 97-actuator ALPAO DM and 1024-actuator Boston Micromachines MEMs DM, respectively), and four wavefront sensor arms: 1) a high-speed Shack-Hartmann WFS, 2) a reflective pyramid WFS, designed as a prototype for the ShaneAO system at Lick Observatory, 3) a vector-Zernike WFS, and 4) a Fast Atmospheric…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Systems and Laser Technology · Advanced optical system design
