SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies

Hidehiro Kaneda; Daisuke Ishihara; Shinki Oyabu; Misato Fukagawa; Takuma Kokusho; Toyoaki Suzuki; Takuya Furuta; Takurou Tsuchikawa; Takehiko Wada; Naoki Isobe; Mitsunobu Kawada; Jungmi Kwon; Hideo Matsuhara; Koichi Nagase; Takao Nakagawa; Takafumi Ootsubo; Mitsuyoshi Yamagishi; Itsuki Sakon; Kohji Tsumura; Hiroshi Shibai

doi:10.1117/12.2313093

SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies

Hidehiro Kaneda, Daisuke Ishihara, Shinki Oyabu, Misato Fukagawa, Takuma Kokusho, Toyoaki Suzuki, Takuya Furuta, Takurou Tsuchikawa, Takehiko Wada, Naoki Isobe, Mitsunobu Kawada, Jungmi Kwon, Hideo Matsuhara, Koichi Nagase, Takao Nakagawa, Takafumi Ootsubo, Mitsuyoshi Yamagishi, Itsuki Sakon, Kohji Tsumura, Hiroshi Shibai

Creative Interdisciplinary Research Division

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Citations (Scopus)

Abstract

SMI (SPICA Mid-infrared Instrument) is one of the two focal-plane science instruments for SPICA. SMI is the Japanese led instrument proposed and managed by a nation-wide university consortium in Japan and planned to be developed in collaboration with Taiwan and the US. SMI covers the wavelength range from 12 to 36 μm with 4 separate channels: the low-resolution (R = 50-120) spectroscopy function for 17-36 μm, the broad-band (R = 5) imaging function at 34 μm, the mid-resolution (R = 1300-2300) spectroscopy function for 18-36 μm, and the high-resolution (R = 28000) spectroscopy function for 12-18 μm. In this paper, we show the results of our conceptual design and feasibility studies of SMI.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2018
Subtitle of host publication	Optical, Infrared, and Millimeter Wave
Editors	Giovanni G. Fazio, Howard A. MacEwen, Makenzie Lystrup
Publisher	SPIE
ISBN (Print)	9781510619494
DOIs	https://doi.org/10.1117/12.2313093
Publication status	Published - 2018
Event	Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave - Austin, United States Duration: 2018 Jun 10 → 2018 Jun 15

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10698
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
Country/Territory	United States
City	Austin
Period	18/6/10 → 18/6/15

Keywords

Cryogenic Telescope
Mid-infrared Instrument
SPICA
Space Infrared Telescope
Spectroscopy

ASJC Scopus subject areas

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

Access to Document

10.1117/12.2313093

Cite this

Kaneda, H., Ishihara, D., Oyabu, S., Fukagawa, M., Kokusho, T., Suzuki, T., Furuta, T., Tsuchikawa, T., Wada, T., Isobe, N., Kawada, M., Kwon, J., Matsuhara, H., Nagase, K., Nakagawa, T., Ootsubo, T., Yamagishi, M., Sakon, I., Tsumura, K., & Shibai, H. (2018). SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies. In G. G. Fazio, H. A. MacEwen, & M. Lystrup (Eds.), Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave [106980C] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10698). SPIE. https://doi.org/10.1117/12.2313093

SPICA mid-infrared instrument (SMI) : Conceptual design and feasibility studies. / Kaneda, Hidehiro; Ishihara, Daisuke; Oyabu, Shinki et al.

Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. ed. / Giovanni G. Fazio; Howard A. MacEwen; Makenzie Lystrup. SPIE, 2018. 106980C (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10698).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Kaneda, H, Ishihara, D, Oyabu, S, Fukagawa, M, Kokusho, T, Suzuki, T, Furuta, T, Tsuchikawa, T, Wada, T, Isobe, N, Kawada, M, Kwon, J, Matsuhara, H, Nagase, K, Nakagawa, T, Ootsubo, T, Yamagishi, M, Sakon, I, Tsumura, K & Shibai, H 2018, SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies. in GG Fazio, HA MacEwen & M Lystrup (eds), Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave., 106980C, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10698, SPIE, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, Austin, United States, 18/6/10. https://doi.org/10.1117/12.2313093

Kaneda H, Ishihara D, Oyabu S, Fukagawa M, Kokusho T, Suzuki T et al. SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies. In Fazio GG, MacEwen HA, Lystrup M, editors, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. SPIE. 2018. 106980C. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2313093

Kaneda, Hidehiro ; Ishihara, Daisuke ; Oyabu, Shinki et al. / SPICA mid-infrared instrument (SMI) : Conceptual design and feasibility studies. Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. editor / Giovanni G. Fazio ; Howard A. MacEwen ; Makenzie Lystrup. SPIE, 2018. (Proceedings of SPIE - The International Society for Optical Engineering).

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abstract = "SMI (SPICA Mid-infrared Instrument) is one of the two focal-plane science instruments for SPICA. SMI is the Japanese led instrument proposed and managed by a nation-wide university consortium in Japan and planned to be developed in collaboration with Taiwan and the US. SMI covers the wavelength range from 12 to 36 μm with 4 separate channels: the low-resolution (R = 50-120) spectroscopy function for 17-36 μm, the broad-band (R = 5) imaging function at 34 μm, the mid-resolution (R = 1300-2300) spectroscopy function for 18-36 μm, and the high-resolution (R = 28000) spectroscopy function for 12-18 μm. In this paper, we show the results of our conceptual design and feasibility studies of SMI.",

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AU - Furuta, Takuya

AU - Tsuchikawa, Takurou

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AU - Isobe, Naoki

AU - Kawada, Mitsunobu

AU - Kwon, Jungmi

AU - Matsuhara, Hideo

AU - Nagase, Koichi

AU - Nakagawa, Takao

AU - Ootsubo, Takafumi

AU - Yamagishi, Mitsuyoshi

AU - Sakon, Itsuki

AU - Tsumura, Kohji

AU - Shibai, Hiroshi

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ER -

SPICA mid-infrared instrument (SMI): Conceptual design and feasibility studies

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