Fibre-Multi-Object Spectrograph (FMOS) for Subaru telescope

Masahiko Kimura, Toshinori Maihara, Kouji Ohta, Fumihide Iwamuro, Shigeru Eto, Masafumi Iino, Daisaku Mochida, Takanori Shima, Hiroshi Karoji, Jun'ichi Noumaru, Masayuki Akiyama, Jurek Brezeski, Peter Gillingham, Anna Moore, Greg Smith, Gavin B. Dalton, Ian Tosh, Graham Murray, David Robertson, Naoyuki Tamura

Research output: Contribution to journalConference article

24 Citations (Scopus)

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 fibre positioners, and the near-infrared spectrograph, etc.

Original languageEnglish
Pages (from-to)974-984
Number of pages11
JournalProceedings of SPIE - The International Society for Optical Engineering
Volume4841
Issue number2
DOIs
Publication statusPublished - 2002
EventInstrument Design and Performance for Optical/Infrared Ground-based Telescopes - waikoloa, HI, United States
Duration: 2002 Aug 252002 Aug 28

Keywords

  • Large telescope
  • Multi-object spectrograph
  • Near-infrared
  • OH suppression
  • Optical fibre
  • VPH grating

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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  • Cite this

    Kimura, M., Maihara, T., Ohta, K., Iwamuro, F., Eto, S., Iino, M., Mochida, D., Shima, T., Karoji, H., Noumaru, J., Akiyama, M., Brezeski, J., Gillingham, P., Moore, A., Smith, G., Dalton, G. B., Tosh, I., Murray, G., Robertson, D., & Tamura, N. (2002). Fibre-Multi-Object Spectrograph (FMOS) for Subaru telescope. Proceedings of SPIE - The International Society for Optical Engineering, 4841(2), 974-984. https://doi.org/10.1117/12.461208