Paper
16 August 2000 Fiber multi-object spectrograph (FMOS) for the Subaru Telescope
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Abstract
Design concept of the fiber multi-object spectrograph (FMOS) for Subaru Telescope together with innovative ideas of optical and structural components is presented. Main features are; i) wide field coverage of 30 arcmin in diameter, ii) 400 target multiplicity, iii) 0.9 to 1.8 micrometers near-IR wavelengths, and iv) OH-airglow suppression capability. The instrument is proposed to be built under the Japan-UK-Australia international collaboration scheme.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Toshinori Maihara, Kouji Ohta, Naoyuki Tamura, Hiroshi Ohtani, Masayuki Akiyama, Junichi Noumaru, Norio Kaifu, Hiroshi Karoji, Masanori Iye, Gavin B. Dalton, Ian Robert Parry, David J. Robertson, Ray M. Sharples, Deqing Ren, Jeremy R. Allington-Smith, Keith Taylor, and Peter R. Gillingham "Fiber multi-object spectrograph (FMOS) for the Subaru Telescope", Proc. SPIE 4008, Optical and IR Telescope Instrumentation and Detectors, (16 August 2000); https://doi.org/10.1117/12.395429
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Cited by 37 scholarly publications.
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KEYWORDS
Spectrographs

Optical spheres

Telescopes

Mirrors

Near infrared

Astronomical imaging

Spectroscopy

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