久留米大学
The University of Texas at San Antonio
Institute for Astronomy, University of Hawaii
国立天文台ハワイ観測所
Columbia University
National Research Council Canada
Anton Pannekoek Institute for Astronomy, University of Amsterdam
Massachusetts Institute of Technology
北京大学科維理天文与天体物理研究所
Southwest Research Institute, USA
University of California, Davis
東京大学
茨城大学
宇宙航空研究開発機構宇宙科学研究所宇宙物理学研究系(JAXA)(ISAS)
著者所属（英）
Kurume University
The University of Texas at San Antonio
Institute for Astronomy, University of Hawaii
Subaru Telescope, National Astronomical Observatory of Japan
Columbia University
National Research Council Canada
Anton Pannekoek Institute for Astronomy, University of Amsterdam
Massachusetts Institute of Technology
The Kavli Institute for Astronomy and Astrophysics, Peking University
Southwest Research Institute, USA
University of California, Davis
The University of Tokyo
Ibaraki University
Department of Space Astronomy and Astrophysics, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
出版者
宇宙航空研究開発機構(JAXA)
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life
巻
JAXA-SP-17-009E
ページ
49 - 52
発行年
2018-03-09
会議概要（会議名, 開催地, 会期, 主催者等）
第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan
抄録（英）
A thermal imager and spectrometer is being investigated for possible construction in the early operation of the Thirty Meter Telescope (TMT). Combined with the mid-IR adaptive optics (AO) system (MIRAO), the instrument will afford 15 times higher sensitivity and 4 times better spatial resolution (0.07 arcsec) with a greatly improved and stable Strehl ratio at 10 micrometers compared to the images delivered by the fast guiding systems of 8m-class telescopes. Through exploiting the large collecting area of the TMT, a high-dispersion spectroscopy mode unrivaled by other ground- and space-based facilities is planned. Such capabilities offer the possibility for breakthrough science, as well as workhorse observing modes of imaging and low/moderate spectral resolution.
内容記述
形態: カラー図版あり
内容記述（英）
Physical characteristics: Original contains color illustrations
TMT/MICHI current concept
AA1730026006.pdf
(211.01KB)
