@inproceedings{oai:jaxa.repo.nii.ac.jp:00003113,
 author = {諸隈, 佳菜 and 山村, 一誠 and MorokumaMatsui, Kana and Yamamura, Issei},
 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 compare the all-sky AKARI/Far-Infrared Surveyor (FIS) Bright Source Catalogue (BSC) Version 2 with the Herschel/ Photodetector Array Camera and Spectrometer (PACS) Point Source Catalogue (PSC), in order to investigate condition for correct matching. We define a ''fake''-match rate based on the AKARI-Herschel flux ratio and study the dependence of this rate on the source density of the region (Ndens), AKARI-Herschel separation (D), Galactic latitude (absolute value of b), and the AKARI flux. We find that the 'fake'-match rate depends on Ndens, D, and absolute value of b and not strongly on the AKARI flux where the sources with smaller Ndens and D and larger absolute value of b result in lower ''fake''-match rate. In our analysis, if we limit the AKARI sources with FQUAL= 3, Ndens = 0 and absolute value of b greater than 30 degrees, and adopt a searching radius of less than 10 arcsec, the source is likely to be matched with an appropriate counterpart in a catalogue of astronomical data whose position accuracy is better than that of the AKARI catalogue., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026039, レポート番号: JAXA-SP-17-009E},
 pages = {231--234},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Evaluation of The AKARI/FIS Bright Source Catalogue Vers.2: Comparison with the Herschel/PACS Point Source Catalogue},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}