High strehl and high contrast for the ELT instrument METIS -- Final design, implementation, and predicted performance of the single-conjugate adaptive optics system
Markus Feldt, Thomas Bertram, Carlos Correia, Olivier Absil, M., Concepci\'on C\'ardenas V\'azquez, Hugo Coppejans, Martin Kulas, Andreas, Obereder, Gilles Orban de Xivry, Silvia Scheithauer, Horst Steuer

TL;DR
This paper details the final design, implementation, and predicted performance of the single-conjugate adaptive optics system for METIS on the ELT, enabling high-contrast, diffraction-limited imaging in the mid-infrared.
Contribution
It presents the complete design, hardware, software, and performance estimations of the ELT METIS AO system, including new insights into wavefront correction and contrast capabilities.
Findings
Achieved high Strehl ratios and contrast performance predictions.
Validated design choices through extensive simulations and analyses.
Outlined testing and verification strategies for the AO system.
Abstract
The Mid-infrared ELT Imager and Spectrograph (METIS) is a first-generation instrument for the Extremely Large Telescope (ELT), Europe's next-generation 39 m ground-based telescope for optical and infrared wavelengths. METIS will offer diffraction-limited imaging, low- and medium-resolution slit spectroscopy, and coronagraphy for high-contrast imaging between 3 and 13 microns, as well as high-resolution integral field spectroscopy between 3 and 5 microns. The main METIS science goals are the detection and characterisation of exoplanets, the investigation of proto-planetary disks, and the formation of planets. The Single-Conjugate Adaptive Optics (SCAO) system corrects atmospheric distortions and is thus essential for diffraction-limited observations with METIS. Numerous challenging aspects of an ELT Adaptive Optics (AO) system are addressed in the mature designs for the SCAO control…
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