@inproceedings{oai:jaxa.repo.nii.ac.jp:00002997,
 author = {早津, 夏己 and 吉田, 直紀 and 松田, 有一 and Hayatsu, Natsuki and Yoshida, Naoki and Matsuda, Yuichi},
 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 present a forecast for detection of high-redshift star-forming galaxies using SPICA-SAFARI and ALMA Band 10-11. We use the outputs of large cosmological simulations of galaxy formation to calculate the fluxes of infrared and far-infrared emission lines ([O III]88.3 μm, [O III] 51.8 μm, [N III]57.2 μm and [C II]158 μm). To this end, we assume empirical relations between the line fluxes and the star formation rate or far-infrared luminoisities. We consider a large survey programme with a 2′× 2′ field-of-view and the limiting flux densities of greater than 21 and greater than 32 μJy (5σ). Our models predicts that there are 604 plus or minus59 galaxies to be detected by such a survey. The number of [C II] emitters with L[C II] less than 10(exp 9)solar luminosity is expected to be 543 plus or minus 52., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027020, レポート番号: JAXA-SP-17-010E},
 pages = {95--97},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Distribution of IR and Submillimeter Line Emitting Galaxies in Cosmological Simulations},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}