@inproceedings{oai:jaxa.repo.nii.ac.jp:00003006,
 author = {大山, 陽一 and 和田, 武彦 and Foucaud, Sebastien and 左近, 樹 and 片坐, 宏一 and Ohyama, Youichi and Wada, Takehiko and Foucaud, Sebastien and Sakon, Itsuki and Kataza, Hirokazu},
 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, The wide field camera of MCS onboard SPICA will have an unique capability of slit-less grism spectroscopy survey. It utilizes wide (5′ × 5′) field of view (FOV), and spectra of all sources within the FOV would be acquired at once with grisms mounted on filter wheels, covering 5-38 μm in total. We simulate the slit-less spectroscopy images of a realistic deep universe with galaxies populated according to their luminosity function in order to examine detectability of galaxies as a function of their luminosity and redshift while quantitatively assessing source overlapping problem., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027029, レポート番号: JAXA-SP-17-010E},
 pages = {129--131},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Perspective on Extra-Galactic Studies with MCS WFC Slit-less Spectroscopy Survey},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}