@article{oai:jaxa.repo.nii.ac.jp:00036686,
 author = {尾中, 敬 and 藤田, 眞之 and 石原, 大助 and 片坐, 宏一 and Kim, Woojung and 前田, 一平 and 松原, 英雄 and 松本, 敏男 and 村上, 浩 and 根岸, 武利 and 大坪, 貴文 and 武山, 芸英 and 上水, 和典 and 上野, 宗孝 and 和田, 武彦 and 度會, 英教 and Onaka, Takashi and Fujita, Saneyuki and Ishihara, Daisuke and Kataza, Hirokazu and Kim, Woojung and Maeda, Ippei and Matsuhara, Hideo and Matsumoto, Toshio and Murakami, Hiroshi and Negishi, Taketoshi and Ootsubo, Takafumi and Takeyama, Norihide and Uemizu, Kazunori and Ueno, Munetaka and Wada, Takehiko and Watarai, Hidenori},
 journal = {The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission},
 month = {Dec},
 note = {The Infrared Camera (IRC) is one of the focal-plane instruments on board ASTRO-F(also called as the Infrared Imaging Surveyor; IRIS) and will make imaging and low-resolutionspectroscopy observations over a wide spectral range in the near- to mid-infrared from 2 - 26μm.The IRC will be operated in the pointed observation mode of ASTRO-F to make deep photometricand spectroscopic surveys of wide field-of-views. It will provide a significant database for studiesof the formation and evolution of galaxies, properties of brown dwarfs, evolution of planetarysystems, and processes of star formation. The IRC comprises three channels: NIR (2 - 5μm),MIR-S (5 - 12μm) and MIR-L (12 - 26μm), and employs state-of-the-art large format arraydetectors. The NIR channel uses a 512×412 InSb array and the MIR channels adopt 256×256Si:As impurity band conduction (IBC) arrays. Each channel has a field-of-view of 10′×10′with anearly diffraction-limited spatial resolution. The NIR and MIR-S channels simultaneously observethe same field on the sky, while the MIR-L observes the sky about 200 away from the NIR/MIR-Sposition. The design overview and current development status of the IRC are presented., 資料番号: SA4597792000},
 pages = {281--288},
 title = {Infrared Camera (IRC) onboard ASTRO-F (IRIS)},
 volume = {14},
 year = {2000}
}