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Proceedings Paper

CISCO: cooled infrared spectrograph and camera for OHS
Author(s): Kentaro Motohara; Toshinori Maihara; Fumihide Iwamuro; Shin Oya; Masatoshi Imanishi; Hiroshi Terada; Miwa Goto; Jun Ichi Iwai; Hirohisa Tanabe; Hiroyuki Tuskamoto; Kazuhiro Sekiguchi
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Paper Abstract

CISCO is an IR camera and spectrograph based on a single 1024 X 1024 HgCdTe array detector, which has been developed as a back-end spectrograph of OHS. It is also designed to be mounted on the Cassegrain or Nasmyth focus directly as an independent instrument. In addition to the normal imaging and spectroscopy modes, CISCO has a slitless prism spectroscopy mode at resolving power of approximately 30. This mode is primarily aimed at detecting the H(alpha) emission line of forming galaxy at z equals 2.05-2.65. The development of CISCO is in near completion, showing results of test observations carried out using a 1.5m telescope.

Paper Details

Date Published: 21 August 1998
PDF: 9 pages
Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); doi: 10.1117/12.317328
Show Author Affiliations
Kentaro Motohara, Kyoto Univ. (Japan)
Toshinori Maihara, Kyoto Univ. (Japan)
Fumihide Iwamuro, Kyoto Univ. (Japan)
Shin Oya, Kyoto Univ. (Japan)
Masatoshi Imanishi, Kyoto Univ. (Japan)
Hiroshi Terada, Kyoto Univ. (Japan)
Miwa Goto, Kyoto Univ. (Japan)
Jun Ichi Iwai, Kyoto Univ. (Japan)
Hirohisa Tanabe, Kyoto Univ. (Japan)
Hiroyuki Tuskamoto, Nikon Corp. (Japan)
Kazuhiro Sekiguchi, National Astronomical Observatory of Japan (United States)


Published in SPIE Proceedings Vol. 3354:
Infrared Astronomical Instrumentation
Albert M. Fowler, Editor(s)

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