Poster + Paper
29 August 2022 Optical design of the wavefront sensing in the ULTIMATE-Subaru Ground Layer Adaptive Optics system
Author Affiliations +
Conference Poster
Abstract
ULTIMATE-Subaru (Ultra-wide Laser Tomographic Imager and MOS with AO Transcendent Exploration) is the next-generation development project of the Subaru Telescope in Hawaii, U.S.A. Ground Layer Adaptive Optics (GLAO) technology corrects atmospheric turbulence near the ground and improves the star image to realize wider fields of view (14 x 14 arcmin) than conventional adaptive optics can do. In the GLAO system, the laser launch system emits four lasers of up to 20 minutes of asterism, then these four lasers excite four artificial stars from 80km to 200km in the sky. The wavefront sensor (WFS) system observes them and corrects atmospheric turbulence. The WFS system also utilizes four natural stars outside the science field of view as well. This paper presents the preliminary optical design of the WFS system.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yoko Tanaka, Yosuke Minowa, Yoshito Ono, Koki Terao, Hiroshige Yoshida, Masayuki Akiyama, Noelia Martínez Rey, Nicholas Herrald, Céline d'Orgeville, François Rigaut, Israel Vaughn, David Chandler, Dionne Haynes, and Warrick Schofield "Optical design of the wavefront sensing in the ULTIMATE-Subaru Ground Layer Adaptive Optics system", Proc. SPIE 12185, Adaptive Optics Systems VIII, 121856M (29 August 2022); https://doi.org/10.1117/12.2629581
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KEYWORDS
Mirrors

Monochromatic aberrations

Telescopes

Cameras

Optical design

Collimators

Wavefront sensors

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