Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan : Korea Astronomy and Space Science Institute : Institute of Space and Astronautical Science, 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
Korean Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Seoul National University
Seoul National University
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)
著者所属(英)
Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan : Korea Astronomy and Space Science Institute : Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Korea Astronomy and Space Science Institute
Seoul National University
Seoul National University
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: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe
巻
JAXA-SP-17-010E
ページ
79 - 81
発行年
2018-03-09
会議概要(会議名, 開催地, 会期, 主催者等)(英)
SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan
抄録(英)
FPC-S is a back up of the fine guidance camera, but is usable for the scientific observation. FPC-S is optimized to observe the spectrum and fluctuation of near-infrared background. One of main scientific targets is to search for the light of first stars of the universe and to delineate the star formation history and structure evolution during the dark age of the universe. The expected performance and its scientific significance is presented.
内容記述
著者人数: 11名
形態: カラー図版あり
内容記述(英)
Number of authors: 11
Physical characteristics: Original contains color illustrations