@inproceedings{oai:jaxa.repo.nii.ac.jp:00003070,
 author = {Packham, Chris and 本田, 充彦 and 岡本, 美子 and The MICHI team and Packham, Chris and Honda, Mitsuhiko and Okamoto, Yoshiko and The MICHI team},
 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, We discuss the key science drivers for a mid-IR instrument for the 30 m TMT, taking advantage of the spatial and spectral resolution afforded by the large aperture of the TMT., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027093, レポート番号: JAXA-SP-17-010E},
 pages = {419--421},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Key Science Drivers for MICHI: A MIR Instrument Concept for the TMT},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}