@inproceedings{oai:jaxa.repo.nii.ac.jp:00003097,
 author = {Zhang, Jin and 尾中, 敬 and 左近, 樹 and 臼井, 文彦 and 下西, 隆 and 板, 良房 and Zhang, Jin and Onaka, Takashi and Sakon, Itsuki and Usui, Fumihiko and Shimonishi, Takashi and Ita, Yoshifusa},
 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 performed the data reduction of the AKARI Phase 3 near-infrared spectroscopy (2-5.5 micrometers with prism) of the LMC, which covers almost the same regions as in Phase 1&2 (in the order of 10 deg(exp 2)). A new spectroscopic catalog which includes approximately 350 contamination free (approximately 200 new) sources and approximately 1200 not heavily contaminated (approximately 700 new) sources is created. The time intervals between Phase 1&2 observations and the corresponding Phase 3 observations are more than 200 days, allowing us to analyze the spectroscopic variabilities of YSOs and carbon stars. In this paper, we report the details of the current version of the Phase 3 spectroscopic catalog as well as some of the results so far obtained., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026023, レポート番号: JAXA-SP-17-009E},
 pages = {143--146},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {The AKARI Phase 3 Near-infrared Spectroscopic Catalog of the Large Magellanic Cloud and the Stellar Spectroscopic Variability},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}