@inproceedings{oai:jaxa.repo.nii.ac.jp:00003147, author = {Kim, Seong Jin and Jeong, Woong-Seob and Lee, Hyung Mok and 後藤, 友嗣 and Pearson, Chris and Shim, Hyunjin and 松原, 英雄 and The AKARI NEP Team and Kim, Seong Jin and Jeong, Woong-Seob and Lee, Hyung Mok and Goto, Tomotsugu and Pearson, Chris and Shim, Hyunjin and Matsuhara, Hideo and The AKARI NEP Team}, 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 study infrared properties of star-forming (SF) galaxies selected by 250 micrometers band detection of the Herschel/SPIRE survey on the entire North Ecliptic Pole (NEP) field of AKARI. We matched SPIRE sources with the spectroscopic survey data and combined with those in the AKARI NEP-Wide catalogue covering from optical to 24 micrometers band. We selected around 250 star-forming galaxies and carried out spectral energy distribution (SED) fit analysis to derive physical quantities. Our SED-fit is based on the continuous near- to mid-IR coverage by 9 photometric bands as well as reliable constraint on far-IR peak by Herschel. Our sample galaxies have prominent mid-IR PAH features and majority of them are LIRG type population in the low-z (less than 0.9). Although they do not seem to form a tight concentration along the galaxy main-sequence due to a wide range of redshift (z is greater than 0.0 and less than 0.9) and various morphological types, they show the downsizing evolutionary pattern toward the present epoch., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026073, レポート番号: JAXA-SP-17-009E}, pages = {363--365}, publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)}, title = {Herschel 250 micrometers detected star-forming (SF) galaxies over the North Ecliptic Pole (NEP) Wide field of AKARI}, volume = {JAXA-SP-17-009E}, year = {2018} }