Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope

Masahiko Kimura; Toshinori Maihara; Fumihide Iwamuro; Masayuki Akiyama; Naoyuki Tamura; Gavin B. Dalton; Naruhisa Takato; Philip Tait; Kouji Ohta; Shigeru Eto; Daisaku Mochida; Brian Elms; Kaori Kawate; Tomio Kurakami; Yuuki Moritani; Junichi Noumaru; Norio Ohshima; Masanao Sumiyoshi; Kiyoto Yabe; Jurek Brzeski; Tony Farrell; Gabriella Frost; Peter R. Gillingham; Roger Haynes; Anna M. Moore; Rolf Muller; Scott Smedley; Greg Smith; David G. Bonfield; Charles B. Brooks; Alan R. Holmes; Emma Curtis Lake; Hanshin Lee; Ian J. Lewis; Tim R. Froud; Ian A. Tosh; Guy F. Woodhouse; Colin Blackburn; Robert Content; Nigel Dipper; Graham Murray; Ray Sharples; David J. Robertson

Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope

Masahiko Kimura, Toshinori Maihara, Fumihide Iwamuro, Masayuki Akiyama, Naoyuki Tamura, Gavin B. Dalton, Naruhisa Takato, Philip Tait, Kouji Ohta, Shigeru Eto, Daisaku Mochida, Brian Elms, Kaori Kawate, Tomio Kurakami, Yuuki Moritani, Junichi Noumaru, Norio Ohshima, Masanao Sumiyoshi, Kiyoto Yabe, Jurek BrzeskiTony Farrell, Gabriella Frost, Peter R. Gillingham, Roger Haynes, Anna M. Moore, Rolf Muller, Scott Smedley, Greg Smith, David G. Bonfield, Charles B. Brooks, Alan R. Holmes, Emma Curtis Lake, Hanshin Lee, Ian J. Lewis, Tim R. Froud, Ian A. Tosh, Guy F. Woodhouse, Colin Blackburn, Robert Content, Nigel Dipper, Graham Murray, Ray Sharples, David J. Robertson

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101 Citations (Scopus)

Abstract

Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2 prime-focus of the Subaru Telescope. The field coverage of 30' diameter is achieved using a new 3-element corrector optimized in the near-infrared (0.9-1.8 mu m) wavelength range. Due to limited space at the prime-focus, we have had to develop a novel fibre positioner, called "Echidna", together with two OH-airglow suppressed spectrographs. FMOS consists of three subsystems: the prime focus unit for IR, the fibre positioning system/connector units, and the two spectrographs. After full systems integration, FMOS was installed on the telescope in late 2007. Many aspects of the performance were checked through various test and engineering observations. In this paper, we present the optical and mechanical components of FMOS, and show the results of our on-sky engineering observations to date.

Original language	English
Pages (from-to)	1135-1147
Number of pages	13
Journal	Publications of the Astronomical Society of Japan
Volume	62
Issue number	5
Publication status	Published - 2010

Keywords

cosmology: observations
instrumentation: spectrographs
surveys
telescopes: Subaru
OH-AIRGLOW SUPPRESSOR
ECHIDNA
POSITIONER
PROJECT

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Kimura, M., Maihara, T., Iwamuro, F., Akiyama, M., Tamura, N., Dalton, G. B., Takato, N., Tait, P., Ohta, K., Eto, S., Mochida, D., Elms, B., Kawate, K., Kurakami, T., Moritani, Y., Noumaru, J., Ohshima, N., Sumiyoshi, M., Yabe, K., ... Robertson, D. J. (2010). Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope. Publications of the Astronomical Society of Japan, 62(5), 1135-1147. http://pasj.asj.or.jp/#past

@article{94c3346637a740d09c28f20740b63a5e,

title = "Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope",

abstract = "Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2 prime-focus of the Subaru Telescope. The field coverage of 30' diameter is achieved using a new 3-element corrector optimized in the near-infrared (0.9-1.8 mu m) wavelength range. Due to limited space at the prime-focus, we have had to develop a novel fibre positioner, called {"}Echidna{"}, together with two OH-airglow suppressed spectrographs. FMOS consists of three subsystems: the prime focus unit for IR, the fibre positioning system/connector units, and the two spectrographs. After full systems integration, FMOS was installed on the telescope in late 2007. Many aspects of the performance were checked through various test and engineering observations. In this paper, we present the optical and mechanical components of FMOS, and show the results of our on-sky engineering observations to date.",

keywords = "cosmology: observations, instrumentation: spectrographs, surveys, telescopes: Subaru, OH-AIRGLOW SUPPRESSOR, ECHIDNA, POSITIONER, PROJECT",

author = "Masahiko Kimura and Toshinori Maihara and Fumihide Iwamuro and Masayuki Akiyama and Naoyuki Tamura and Dalton, {Gavin B.} and Naruhisa Takato and Philip Tait and Kouji Ohta and Shigeru Eto and Daisaku Mochida and Brian Elms and Kaori Kawate and Tomio Kurakami and Yuuki Moritani and Junichi Noumaru and Norio Ohshima and Masanao Sumiyoshi and Kiyoto Yabe and Jurek Brzeski and Tony Farrell and Gabriella Frost and Gillingham, {Peter R.} and Roger Haynes and Moore, {Anna M.} and Rolf Muller and Scott Smedley and Greg Smith and Bonfield, {David G.} and Brooks, {Charles B.} and Holmes, {Alan R.} and Lake, {Emma Curtis} and Hanshin Lee and Lewis, {Ian J.} and Froud, {Tim R.} and Tosh, {Ian A.} and Woodhouse, {Guy F.} and Colin Blackburn and Robert Content and Nigel Dipper and Graham Murray and Ray Sharples and Robertson, {David J.}",

year = "2010",

language = "English",

volume = "62",

pages = "1135--1147",

journal = "Publications of the Astronomical Society of Japan",

issn = "0004-6264",

publisher = "Astronomical Society of Japan",

number = "5",

}

Kimura, M, Maihara, T, Iwamuro, F, Akiyama, M, Tamura, N, Dalton, GB, Takato, N, Tait, P, Ohta, K, Eto, S, Mochida, D, Elms, B, Kawate, K, Kurakami, T, Moritani, Y, Noumaru, J, Ohshima, N, Sumiyoshi, M, Yabe, K, Brzeski, J, Farrell, T, Frost, G, Gillingham, PR, Haynes, R, Moore, AM, Muller, R, Smedley, S, Smith, G, Bonfield, DG, Brooks, CB, Holmes, AR, Lake, EC, Lee, H, Lewis, IJ, Froud, TR, Tosh, IA, Woodhouse, GF, Blackburn, C, Content, R, Dipper, N, Murray, G, Sharples, R & Robertson, DJ 2010, 'Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope', Publications of the Astronomical Society of Japan, vol. 62, no. 5, pp. 1135-1147. <http://pasj.asj.or.jp/#past>

TY - JOUR

T1 - Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope

AU - Kimura, Masahiko

AU - Maihara, Toshinori

AU - Iwamuro, Fumihide

AU - Akiyama, Masayuki

AU - Tamura, Naoyuki

AU - Dalton, Gavin B.

AU - Takato, Naruhisa

AU - Tait, Philip

AU - Ohta, Kouji

AU - Eto, Shigeru

AU - Mochida, Daisaku

AU - Elms, Brian

AU - Kawate, Kaori

AU - Kurakami, Tomio

AU - Moritani, Yuuki

AU - Noumaru, Junichi

AU - Ohshima, Norio

AU - Sumiyoshi, Masanao

AU - Yabe, Kiyoto

AU - Brzeski, Jurek

AU - Farrell, Tony

AU - Frost, Gabriella

AU - Gillingham, Peter R.

AU - Haynes, Roger

AU - Moore, Anna M.

AU - Muller, Rolf

AU - Smedley, Scott

AU - Smith, Greg

AU - Bonfield, David G.

AU - Brooks, Charles B.

AU - Holmes, Alan R.

AU - Lake, Emma Curtis

AU - Lee, Hanshin

AU - Lewis, Ian J.

AU - Froud, Tim R.

AU - Tosh, Ian A.

AU - Woodhouse, Guy F.

AU - Blackburn, Colin

AU - Content, Robert

AU - Dipper, Nigel

AU - Murray, Graham

AU - Sharples, Ray

AU - Robertson, David J.

PY - 2010

Y1 - 2010

N2 - Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2 prime-focus of the Subaru Telescope. The field coverage of 30' diameter is achieved using a new 3-element corrector optimized in the near-infrared (0.9-1.8 mu m) wavelength range. Due to limited space at the prime-focus, we have had to develop a novel fibre positioner, called "Echidna", together with two OH-airglow suppressed spectrographs. FMOS consists of three subsystems: the prime focus unit for IR, the fibre positioning system/connector units, and the two spectrographs. After full systems integration, FMOS was installed on the telescope in late 2007. Many aspects of the performance were checked through various test and engineering observations. In this paper, we present the optical and mechanical components of FMOS, and show the results of our on-sky engineering observations to date.

AB - Fibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2 prime-focus of the Subaru Telescope. The field coverage of 30' diameter is achieved using a new 3-element corrector optimized in the near-infrared (0.9-1.8 mu m) wavelength range. Due to limited space at the prime-focus, we have had to develop a novel fibre positioner, called "Echidna", together with two OH-airglow suppressed spectrographs. FMOS consists of three subsystems: the prime focus unit for IR, the fibre positioning system/connector units, and the two spectrographs. After full systems integration, FMOS was installed on the telescope in late 2007. Many aspects of the performance were checked through various test and engineering observations. In this paper, we present the optical and mechanical components of FMOS, and show the results of our on-sky engineering observations to date.

KW - cosmology: observations

KW - instrumentation: spectrographs

KW - surveys

KW - telescopes: Subaru

KW - OH-AIRGLOW SUPPRESSOR

KW - ECHIDNA

KW - POSITIONER

KW - PROJECT

M3 - Article

SN - 0004-6264

VL - 62

SP - 1135

EP - 1147

JO - Publications of the Astronomical Society of Japan

JF - Publications of the Astronomical Society of Japan

IS - 5

ER -

Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope

Abstract

Keywords

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