Near-infrared and Mid-infrared Spectroscopy with the Infrared Camera (IRC) for AKARI
Youichi Ohyama (1), Takashi Onaka (2), Hideo Matsuhara (1), Takehiko, Wada (1), Woojung Kim (1), Naofumi Fujishiro (3), Kazunori Uemizu (1), Itsuki, Sakon (2), Martin Cohen (4), Miho Ishigaki (5), Daisuke Ishihara (2),, Yoshifusa Ita (1), Hirokazu Kataza (1)

TL;DR
The IRC instrument on the AKARI satellite offers unique low-resolution, wide-field infrared spectroscopy capabilities in space, enabling sensitive surveys in the near- and mid-infrared ranges.
Contribution
This paper details the specifications and in-orbit performance of the IRC spectrograph, highlighting its unique space-based wide-field spectroscopic capabilities.
Findings
Successful in-orbit operation of IRC spectrograph
Achieved sensitive wide-field infrared spectroscopy
Demonstrated performance aligns with specifications
Abstract
The Infrared Camera (IRC) is one of the two instruments on board the AKARI satellite. In addition to deep imaging from 1.8-26.5um for the pointed observation mode of the AKARI, it has a spectroscopic capability in its spectral range. By replacing the imaging filters by transmission-type dispersers on the filter wheels, it provides low-resolution (lambda/d_lambda ~ 20-120) spectroscopy with slits or in a wide imaging field-of-view (approximately 10'X10'). The IRC spectroscopic mode is unique in space infrared missions in that it has the capability to perform sensitive wide-field spectroscopic surveys in the near- and mid-infrared wavelength ranges. This paper describes specifications of the IRC spectrograph and its in-orbit performance.
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