Oyabu, S.; Yamamura, I.; Alfageme, C.; Barthel, P.; Cassatella, A.; Cohen, M.; Cox, N.; Figueredo, E.; Fujiwara, H.; Ikeda, N.; Ishihara, D.; Jeong, W.-S.; Kataza, H.; Kester, Do; Lee, H. M.; Makiuti, S.; Mueller, T. G.; Nakagawa, T.; Takita, S.; Oh, S. H.; Oliver, S.; Pearson, C.; Rahman, N.; Rowan-Robinson, M.; Salama, A.; Savage, R.; Serjeant, S.; White, G. J. and Yamauchi, C.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1117/12.856931|
|Google Scholar:||Look up in Google Scholar|
Bright source catalogues based on the new mid- and far-infrared all-sky survey by the infrared astronomical satellite AKARI were released into the public domain in March 2010. The mid-infrared catalogue contains more than 870 thousand sources observed at 9 and 18 µm, and the far-infrared catalogue provides information of about 427 thousand sources at 65, 90, 140, and 160 µm. The AKARI catalogues will take over the IRAS catalogues and will become one of the most important catalogues in astronomy. We present the characteristics of the AKARI infrared source catalogues as well as current activity for the future versions.
|Item Type:||Conference Item|
|Copyright Holders:||2010 SPIE|
|Academic Unit/School:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||07 Jan 2011 15:32|
|Last Modified:||28 Nov 2016 14:15|
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