@inproceedings{oai:jaxa.repo.nii.ac.jp:00003148,
 author = {正垣, 綾乃 and 松浦, 周二 and 大井, 渚 and 後藤, 友嗣 and 松原, 英雄 and 村田, 一心 and 高木, 俊暢 and 大塚, 拓也 and Malkan, Matthew and 中禮, 沙也加 and Shogaki, Ayano and Matsuura, Shuji and Oi, Nagisa and Goto, Tomotsugu and Matsuhara, Hideo and Murata, Kazumi and Takagi, Toshinobu and Otsuka, Takuya and Malkan, Matthew and Churei, Sayaka},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life},
 month = {Mar},
 note = {第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京, The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan, We analyzed 553 spectra of infrared sources in the AKARI NEP deep field observed with Keck/DEIMOS in 2011. In previous work, we conducted a spectroscopic diagnostics of the sources based on relative line fluxes without the absolute flux calibration, and the analysis was not done for all detected sources due to a technical reason. In this work, we present a preliminary report on measurement of absolute line flux for all detected sources. For the flux calibration of the DEIMOS spectra, we adopted the photometric (r- or i-band) flux to determine the scaling factor of the average flux in the blue or red channel of DEIMOS. As a result of our analysis, we obtained emission spectra of 304 galaxies showing hydrogen recombination lines and forbidden lines of heavy elements, e.g., brackets O III brackets line., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026074, レポート番号: JAXA-SP-17-009E},
 pages = {367--370},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Line flux measurement of infrared galaxies in the AKARI NEP field with Keck/DEIMOS},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}