CISCO: Cooled Infrared Spectrograph and Camera for OHS on the Subaru   Telescope
  This paper describes a Cooled Infrared Spectrograph and Camera for OHS (CISCO), mounted on the Nasmyth focus of the Subaru telescope. It is primarily designed as a back-end camera of the OH-Airglow Suppressor (OHS), and is also used as an independent, general-purpose near-infrared camera/spectrograph. CISCO is based on a single 1024x1024 format HgCdTe HAWAII array detector, and is capable of either wide-field imaging of 1.8'x1.8' field-of-view or low-resolution spectroscopy from 0.9 to 2.4 um. The limiting magnitudes measured during test observations were found to be J=23.5mag and K'=22.4mag (imaging, 1" aperture, S/N=5, 1 hr exposure). 
K. Motohara (1,2,3), F. Iwamuro (3), T. Maihara (3,4), S. Oya (3,5),   H. Tsukamoto (3), M. Imanishi (3,6), H. Terada (2,3),...