@inproceedings{oai:jaxa.repo.nii.ac.jp:00003149,
 author = {Kim, Helen K. and Malkan, Matthew A. and 大井, 渚 and Burgarella, Denis and Buat, Veronique and 高木, 俊暢 and 松原, 英雄 and Kim, Helen K. and Malkan, Matthew A. and Oi, Nagisa and Burgarella, Denis and Buat, Veronique and Takagi, Toshinobu and Matsuhara, Hideo},
 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 present follow-up optical DEIMOS/Keck-II spectra of in the order of 180 galaxies (median z in the order of 0.7) in the AKARI NEP-Deep field. The spectroscopic redshifts (z(sub spec)) agree well with photometric redshifts (z(sub phot)) at z less than 1, with mean absolute value of z approximately equal to 0.07, but the photometric redshifts are systematically too high at z greater than 1. One Seyfert 1.9 and one Seyfert 2 were identified from their emission lines, but no LINERs were found, in contrast to Kartaltepe et al. (2015), 84% of our objects are classified to be along the star-forming, HII sequence. At a given stellar mass, gas phase metallicities were found to be 0.1-0.2 dex lower than the local SDSS relation, but consistent with the relation found by Zahid et al. (2011) at z in the order of 0.8. Gas reddenings were derived from Balmer emission line ratios. In the majority of cases, the corresponding extinction at H alpha is in the order of 1 mag, typical of normal spiral galaxies. Star formation rates (SFRs) were estimated from the luminosities of either brackets O II brackets lambda 3727 or H alpha, and agreed reasonably (50% scatter). In galaxies with equivalent width EW(H alpha) of 10 angstroms or less, the broadband spectral energy distribution (SED) fitting significantly overestimates the SFR., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026075, レポート番号: JAXA-SP-17-009E},
 pages = {371--374},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {DEIMOS Spectroscopy of Star-Forming Galaxies in the AKARI North Ecliptic Pole-Deep Field},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}