ULTIMATE-subaru: Wide-field near-infrared surveyor with GLAO at subaru telescope

Yosuke Minowa; Christophe Clergeon; Masayuki Akiyama; Francois Rigaut; Celine D'Orgeville; Ian Price; Nick Herrald; Yusei Koyama; Ikuru Iwata; Takashi Hattori; Tadayuki Kodama; Yutaka Hayano; Shin Oya; Ichi Tanaka; Kentaro Motohara; Nobuo Arimoto; Michitoshi Yoshida

ULTIMATE-subaru: Wide-field near-infrared surveyor with GLAO at subaru telescope

Yosuke Minowa, Christophe Clergeon, Masayuki Akiyama, Francois Rigaut, Celine D'Orgeville, Ian Price, Nick Herrald, Yusei Koyama, Ikuru Iwata, Takashi Hattori, Tadayuki Kodama, Yutaka Hayano, Shin Oya, Ichi Tanaka, Kentaro Motohara, Nobuo Arimoto, Michitoshi Yoshida

理学研究科・天文学専攻

研究成果: Paper › 査読

2 被引用数 (Scopus)

抄録

ULTIMATE-Subaru is a next large facility instrument program at Subaru telescope, which will develop 14 x14 arcmin2 wide-field near-infrared imager and multi-object spectrograph with the aid of ground-layer adaptive optics system (GLAO) at the Cassegrain and Nasmyth foci of the telescope in mid 2020s. Our preliminary performance simulation indicates that the GLAO system at Subaru telescope can provide uniform seeing improvement down to FWHM~0.2 arcsec in K band under moderate seeing condition across the field of view up to 20 arcmin in diameter. The main science case of the ULTIMATE-Subaru is a complete census of galaxy evolution from cosmic dawn (z>8) to cosmic noon (z=1-3) with ultradeep, wide-field narrow-band imaging and multi-object spectroscopies of a statistical sample of galaxies especially in K band.

本文言語	English
出版ステータス	Published - 2017 1月 1
イベント	5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017 - Tenerife, Canary Islands, Spain 継続期間: 2017 6月 25 → 2017 6月 30

Other

Other	5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017
国/地域	Spain
City	Tenerife, Canary Islands
Period	17/6/25 → 17/6/30

ASJC Scopus subject areas

宇宙惑星科学
機械工学
制御およびシステム工学
器械工学
天文学と天体物理学
電子材料、光学材料、および磁性材料

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引用スタイル

Minowa, Y., Clergeon, C., Akiyama, M., Rigaut, F., D'Orgeville, C., Price, I., Herrald, N., Koyama, Y., Iwata, I., Hattori, T., Kodama, T., Hayano, Y., Oya, S., Tanaka, I., Motohara, K., Arimoto, N., & Yoshida, M. (2017). ULTIMATE-subaru: Wide-field near-infrared surveyor with GLAO at subaru telescope. Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain.

Minowa, Y, Clergeon, C, Akiyama, M, Rigaut, F, D'Orgeville, C, Price, I, Herrald, N, Koyama, Y, Iwata, I, Hattori, T, Kodama, T, Hayano, Y, Oya, S, Tanaka, I, Motohara, K, Arimoto, N & Yoshida, M 2017, 'ULTIMATE-subaru: Wide-field near-infrared surveyor with GLAO at subaru telescope', Paper presented at 5th Adaptive Optics for Extremely Large Telescopes, AO4ELT 2017, Tenerife, Canary Islands, Spain, 17/6/25 - 17/6/30.

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AU - Minowa, Yosuke

AU - Clergeon, Christophe

AU - Akiyama, Masayuki

AU - Rigaut, Francois

AU - D'Orgeville, Celine

AU - Price, Ian

AU - Herrald, Nick

AU - Koyama, Yusei

AU - Iwata, Ikuru

AU - Hattori, Takashi

AU - Kodama, Tadayuki

AU - Hayano, Yutaka

AU - Oya, Shin

AU - Tanaka, Ichi

AU - Motohara, Kentaro

AU - Arimoto, Nobuo

AU - Yoshida, Michitoshi

PY - 2017/1/1

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N2 - ULTIMATE-Subaru is a next large facility instrument program at Subaru telescope, which will develop 14 x14 arcmin2 wide-field near-infrared imager and multi-object spectrograph with the aid of ground-layer adaptive optics system (GLAO) at the Cassegrain and Nasmyth foci of the telescope in mid 2020s. Our preliminary performance simulation indicates that the GLAO system at Subaru telescope can provide uniform seeing improvement down to FWHM~0.2 arcsec in K band under moderate seeing condition across the field of view up to 20 arcmin in diameter. The main science case of the ULTIMATE-Subaru is a complete census of galaxy evolution from cosmic dawn (z>8) to cosmic noon (z=1-3) with ultradeep, wide-field narrow-band imaging and multi-object spectroscopies of a statistical sample of galaxies especially in K band.

AB - ULTIMATE-Subaru is a next large facility instrument program at Subaru telescope, which will develop 14 x14 arcmin2 wide-field near-infrared imager and multi-object spectrograph with the aid of ground-layer adaptive optics system (GLAO) at the Cassegrain and Nasmyth foci of the telescope in mid 2020s. Our preliminary performance simulation indicates that the GLAO system at Subaru telescope can provide uniform seeing improvement down to FWHM~0.2 arcsec in K band under moderate seeing condition across the field of view up to 20 arcmin in diameter. The main science case of the ULTIMATE-Subaru is a complete census of galaxy evolution from cosmic dawn (z>8) to cosmic noon (z=1-3) with ultradeep, wide-field narrow-band imaging and multi-object spectroscopies of a statistical sample of galaxies especially in K band.

KW - Adaptive optics

KW - Instrumentation

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M3 - Paper

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Y2 - 25 June 2017 through 30 June 2017

ER -

ULTIMATE-subaru: Wide-field near-infrared surveyor with GLAO at subaru telescope

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