High Contrast and High Angular Imaging at Subaru Telescope
Olivier Guyon, Kyohoon Ahn, Masayuki Akiyama, Thayne Currie, Vincent, Deo, Takashi Hattori, Tomoyuki Kudo, Julien Lozi, Yosuke Minowa, Yoshito Ono,, Nour Skaf, Motohide Tamura, Vincent Vievard

TL;DR
This paper discusses Subaru Telescope's adaptive optics systems, including current and upcoming high-contrast, high-angular-resolution imaging capabilities for various astronomical observations.
Contribution
It details the latest developments and upgrades in Subaru's adaptive optics systems, enhancing imaging performance for diverse scientific applications.
Findings
Implementation of GLAO providing partial correction over 20 arcmin FOV
Development of SCExAO for high-contrast, narrow field imaging
Upcoming 3000-actuator upgrade to improve AO performance
Abstract
Adaptive Optics projects at Subaru Telescope span a wide field of capabilities ranging from ground-layer adaptive optics (GLAO) providing partial correction over a 20 arcmin FOV to extreme adaptive optics (ExAO) for exoplanet imaging. We describe in this paper current and upcoming narrow field-of-view capabilities provided by the Subaru Extreme Adaptive Optics Adaptive Optics (SCExAO) system and its instrument modules, as well as the upcoming 3000-actuator upgrade of the Nasmyth AO system.
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
