Presentation + Paper
13 December 2020 ULTIMATE-Subaru: system performance modeling of GLAO and wide-field NIR instruments
Author Affiliations +
Abstract
ULTIMATE-Subaru is a next large facility instrument project at Subaru telescope. We will develop a 14x14 sq. arcmin wide-field near-infrared (NIR) imager and a multi-object spectrograph with the aid of a ground- layer adaptive optics system (GLAO), which will uniformly improve the seeing by a factor of 2 over a wide field of view up to ~20 arcmin in diameter. We have developed system modeling of the GLAO and wide-field NIR instruments to define the system level requirements flow down from science cases and derive the system performance budgets based on the GLAO end-to-end numerical simulation and optical system models of the telescope and wide-field NIR science instruments. In this paper, we describe the system performance modeling of ULTIMATE-Subaru and present an overview of the requirements flow down.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yosuke Minowa, Yusei Koyama, Kenshi Yanagisawa, Kentaro Motohara, Ichi Tanaka, Yoshito Ono, Takashi Hattori, Christophe Clergeon, Yutaka Hayano, Masayuki Akiyama, Tadayuki Kodama, Céline d'Orgeville, Francois Rigaut, Shiang-Yu Wang, and Michitoshi Yoshida "ULTIMATE-Subaru: system performance modeling of GLAO and wide-field NIR instruments", Proc. SPIE 11450, Modeling, Systems Engineering, and Project Management for Astronomy IX, 114500O (13 December 2020); https://doi.org/10.1117/12.2561950
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KEYWORDS
Near infrared

Performance modeling

Systems modeling

Imaging spectroscopy

Imaging systems

Cesium

Infrared telescopes

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