Paper
28 June 2006 FMOS: the fiber multiple-object spectrograph IV: current status of OHS-based spectrograph
Fumihide Iwamuro, Toshinori Maihara, Kouji Ohta, Shigeru Eto, Michinari Sakai, Masayuki Akiyama, Masahiko Kimura, Naoyuki Tamura, Junichi Noumaru, Hiroshi Karoji, Gavin B. Dolton, Ian J. Lewis, Ian A. J. Tosh, Graham J. Murray, Nigel A. Dipper, David J. Robertoson, Peter R. Gillingham, Scott Smedley, Greg A. Smith, Gabriella Frost
Author Affiliations +
Abstract
The Fiber Multiple-Object Spectrograph for Subaru Telescope (FMOS) is quite large instrument composed of the prime focus unit, the fiber bundle unit, and the two infrared spectrographs. Among these units, a part of the prime focus unit and one of the spectrograph were transported from Kyoto University to the Subaru Observatory in the middle of 2005. We present the optical and the mechanical components of the spectrograph, which was reassembled on the new floor of the Subaru dome. We also show the preliminary results of the optical alignment and the cooling test of the instrument at the summit of Mauna Kea.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Fumihide Iwamuro, Toshinori Maihara, Kouji Ohta, Shigeru Eto, Michinari Sakai, Masayuki Akiyama, Masahiko Kimura, Naoyuki Tamura, Junichi Noumaru, Hiroshi Karoji, Gavin B. Dolton, Ian J. Lewis, Ian A. J. Tosh, Graham J. Murray, Nigel A. Dipper, David J. Robertoson, Peter R. Gillingham, Scott Smedley, Greg A. Smith, and Gabriella Frost "FMOS: the fiber multiple-object spectrograph IV: current status of OHS-based spectrograph", Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62691B (28 June 2006); https://doi.org/10.1117/12.671006
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Cited by 7 scholarly publications.
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KEYWORDS
Spectrographs

Mirrors

Sensors

Cameras

Infrared radiation

Actuators

Optical alignment

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