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The Infrared Astronomical Mission AKARI

Hiroshi Murakami, Hajime Baba, P. D. Barthel, David L. Clements, Martin Cohen, Yasuo Doi, Keigo Enya, E. Figuerêdo, Naofumi Fujishiro, Hideaki Fujiwara, Mikio Fujiwara, Pedro García-Lario, Tomotsugu Goto, Sunao Hasegawa, Yasunori Hibi, T. Hirao, Norihisa Hiromoto, Seung Soo Hong, Koji Imai, Miho N. Ishigaki, Masateru Ishiguro, Daisuke Ishihara, Yoshifusa Ita, Woong-Seob Jeong, K. S. Jeong, Hidehiro Kaneda, Hirokazu Kataza, Mitsunobu Kawada, Toshihide Kawai, Akiko Kawamura

📄 Abstract

Abstract AKARI, the first Japanese satellite dedicated to infrared astronomy, was launched on 2006 February 21, and started observations in May of the same year. AKARI has a 68.5 cm cooled telescope, together with two focal-plane instruments, which survey the sky in six wavelength bands from mid–to far-infrared. The instruments also have a capability for imaging and spectroscopy in the wavelength range 2-180$mu$m in the pointed observation mode, occasionally inserted into a continuous survey operation. The in-orbit cryogen lifetime is expected to be one and a half years. The All-Sky Survey will cover more than 90% of the whole sky with a higher spatial resolution and a wider wavelength coverage than that of the previous IRAS all-sky survey. Point-source catalogues of the All-Sky Survey will be released to the astronomical community. Pointed observations will be used for deep surveys of selected sky areas and systematic observations of important astronomical targets. These will become an additional future heritage of this mission.

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