@inproceedings{oai:jaxa.repo.nii.ac.jp:00003012,
 author = {真喜屋, 龍 and 戸谷, 友則 and 小林, 正和 and 長島, 雅裕 and 竹内, 努 and Makiya, Ryu and Totani, Tomonori and Kobayashi, Masakazu A. R. and Nagashima, Masahiro and Takeuchi, Tsutomu},
 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, Understanding the galaxy dust emission is very important to obtain a full picture of galaxy formation, since it contains rich information about hidden star formation activity, physical properties of interstellar dust, and their role in galaxy formation. From the analysis of infrared spectral energy distribution (SED) of local galaxies which were observed by AKARI, we have found that a dust temperature averaged over the entire galaxy is strongly correlated with total infrared surface brightness, rather than total infrared luminosity. Combining this correlation with our cosmological galaxy formation model, we have computed dust SED of mock galaxies. By using this model, we present can theoretical predictions on the evolution of dusty universe., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027035, レポート番号: JAXA-SP-17-010E},
 pages = {153--155},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Semi-analytic Model of Galaxy Formation in the Infrared: Predictions for SPICA},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}