The Fiber Multi-Object Spectrograph (FMOS) for the Subaru Telescope

Masahiko Kimura; Toshinori Maihara; Kouji Ohta; Fumihide Iwamuro; Sigeru Eto; Masafumi Lino; Daisaku Mochida; Takanori Shima; Hiroshi Karoji; Junichi Noumaru; Masayuki Akiyama; Jurek Brzeski; Peter R. Gillingham; Anna Marie Moore; Greg Smith; Gavin B. Dalton; Ian A. Tosh; Graham J. Murray; David J. Robertson; Naoyuki Tamura

doi:10.1117/12.461208

7 March 2003 Fibre-Multi-Object Spectrograph (FMOS) for Subaru Telescope

Masahiko Kimura, Toshinori Maihara, Kouji Ohta, Fumihide Iwamuro, Sigeru Eto, Masafumi Lino, Daisaku Mochida, Takanori Shima, Hiroshi Karoji, Junichi Noumaru, Masayuki Akiyama, Jurek Brzeski, Peter R. Gillingham, Anna Marie Moore, Greg Smith, Gavin B. Dalton, Ian A. Tosh, Graham J. Murray, David J. Robertson, Naoyuki Tamura

Author Affiliations +

Proceedings Volume 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes; (2003) https://doi.org/10.1117/12.461208
Event: Astronomical Telescopes and Instrumentation, 2002, Waikoloa, Hawai'i, United States

Abstract

The Fibre Multi-Object Spectrograph (FMOS) is a second-generation common-use instrument of the Subaru telescope. Under an international collaboration scheme of Japan, UK, and Australia, a realistic design of FMOS has been already in completion, and the fabrications of hardware components have been in progress. We present the overall design details together with the special features of FMOS subsystems, such as the prime focus corrector, the prime focus mechanical unit including fiber positioners, and the near-infrared spectrograph, etc.

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Masahiko Kimura, Toshinori Maihara, Kouji Ohta, Fumihide Iwamuro, Sigeru Eto, Masafumi Lino, Daisaku Mochida, Takanori Shima, Hiroshi Karoji, Junichi Noumaru, Masayuki Akiyama, Jurek Brzeski, Peter R. Gillingham, Anna Marie Moore, Greg Smith, Gavin B. Dalton, Ian A. Tosh, Graham J. Murray, David J. Robertson, and Naoyuki Tamura "Fibre-Multi-Object Spectrograph (FMOS) for Subaru Telescope", Proc. SPIE 4841, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, (7 March 2003); https://doi.org/10.1117/12.461208

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