@inproceedings{oai:jaxa.repo.nii.ac.jp:00002995,
 author = {斎藤, 智樹 and 江上, 英一 and 小林, 正和 and 和田, 武彦 and 中島, 王彦 and 清水, 一紘 and 井上, 昭雄 and Saito, Tomoki and Egami, Eiichi and Kobayashi, Masakazu A. R. and Wada, Takehiko and Nakajima, Kimihiko and Shimizu, Ikkoh and Inoue, Akio K.},
 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 propose a narrowband imaging survey of star-forming galaxies at re-ionisation era. The survey will exploit the widefield imaging capability of SPICA/MCS by using narrowband filter to detect H emission from the redshift 7 less than or equal to z less than or equal to 10. We estimated the feasibility of this survey, showing that the number of detectable sources highly depends on the IMF of the stellar population. Since the age constraints are fairly strong at such high redshifts, and extremely young star-forming galaxies are presumably less dusty, the survey should give the first direct and meaningful constraints on the IMF of population III (popIII) star formation., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027018, レポート番号: JAXA-SP-17-010E},
 pages = {87--89},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Probing the Stellar Contents of Star-Forming Galaxies at Re-Ionisation Era},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}