@inproceedings{oai:jaxa.repo.nii.ac.jp:00003050,
 author = {小谷, 隆行 and 塩谷, 圭吾 and 金田, 英宏 and 松尾, 太郎 and 生駒, 大洋 and 伊藤, 洋一 and 井田, 茂 and 櫨, 香奈恵 and 大薮, 進喜 and 石原, 大助 and 空華, 智子 and 本田, 充彦 and 井上, 昭雄 and 長沢, 真樹子 and 高見, 道弘 and 深川, 美里 and 山下, 卓也 and 成田, 憲保 and 田村, 元秀 and 尾関, 真二 and 竹内, 菜未 and 中川, 貴雄 and 松原, 英雄 and 片坐, 宏一 and 川田, 光伸 and 和田, 武彦 and 津村, 耕司 and 磯部, 直樹 and 三田, 誠 and 小松, 敬治 and 内田, 英樹 and 巳谷, 真司 and 坂井, 真一郎 and 猿楽, 祐樹 and 有松, 亘 and 垰, 千尋 and Kotani, Takayuki and Enya, Keigo and Kaneda, Hidehiro and Matsuo, Taro and Ikoma, Masahiro and Ito, Yoichi and Ida, Shigeru and Haze, Kanae and Oyabu, Shinki and Ishihara, Daisuke and Sorahana, Satoko and Honda, Mitsuhiko and Inoue, Akio K. and Nagasawa, Makiko and Takami, Michihiro and Fukagawa, Misato and Yamashita, Takuya and Narita, Norio and Tamura, Motohide and Oseki, Shinji and Takeuchi, Nami and Nakagawa, Takao and Matsuhara, Hideo and Kataza, Hirokazu and Kawada, Mitsunobu and Wada, Takehiko and Tsumura, Koji and Isobe, Naoki and Mita, Makoto and Komatsu, Keiji and Uchida, Hideki and Mitani, Shinji and Sakai, Shinichiro and Sarugaku, Yuki and Arimatsu, Ko and Tao, Chihiro},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {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, SPICA Coronagraph Instrument (SCI) is an instrument dedicated for direct detection and characterization of exoplanets and also for other science that needs a high-contrast imaging and spectroscopic capability in the near to mid-infrared wavelengths. We will present the major science cases for exoplanets from the instrument proposal of SCI. Thanks to the high-contrast imaging and spectroscopic capability, we will be able to tackle the various problems on the exoplanet science. SCI will give us the unique opportunity to observationally understand the formation process of Jovian planets, which is still poorly understood, by measuring temperatures of young Jovian planets. Spectroscopy of planet atmospheres will enable us to reveal the chemical compositions by measuring the abundances of various important molecules such as CO, CH4, NH3, H2O, H2 etc. We will also access to the structure of Jovian atmosphere, for example the existence of thermal inversion which is known for our Solar system planets. Furthermore, the direct detection of icy giants around early-type stars with SCI will open a new window to investigate these enigmatic planets., 著者名の誤記: T. KOMATSU, 著者人数: 57名, 形態: カラー図版あり, The clerical error of an author's name: T. KOMATSU, Number of authors: 57, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027073, レポート番号: JAXA-SP-17-010E},
 pages = {339--342},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Exoplanet Science with the SPICA Coronagraph Instrument},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}