@inproceedings{oai:jaxa.repo.nii.ac.jp:00003042,
 author = {高見, 道弘 and Goicoechea, Javier R. and 塩谷, 圭吾 and 猿楽, 祐樹 and SPICA Science Working Group and Takami, Michihiro and Goicoechea, Javier R. and Enya, Keigo and Sarugaku, Yuki and SPICA Science Working Group},
 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 will be a powerful facility to help us understand the formation and evolution of our solar system and exoplanetary systems in 2020's. The wavelength coverage (5-210 micrometers) is optimal for observations of key targets including exoplanets, protoplanetary and debris disks, and solar system small bodies. At this coverage SPICA will offer several dramatic advantages, including extremely high sensitivity and excellent image quality with a cooled (approximately 6 K) monolithic 3-m class mirror telescope, a variety of capabilities for spectroscopy and spectro-imaging, and an unprecedented high spectral resolution for mid-infrared spectroscopy free from telluric absorption and emission. We briefly summarize our discussions for possible science impacts on the above targets and research topics., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027065, レポート番号: JAXA-SP-17-010E},
 pages = {299--305},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Studies of Exoplanets and Solar Systems with SPICA: An Overview},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}