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

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

doi:10.1117/12.2313093

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

DOI 被引用文献2件参考文献18件

書誌事項

公開日: 2018-07-12

資源種別: journal article

DOI

10.1117/12.2313093

公開者: SPIE

説明

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.

収録刊行物

Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave

Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave 10698 11-, 2018-07-12

SPIE

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

書誌事項

説明

収録刊行物

被引用文献 (2)*注記

参考文献 (18)*注記

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

書誌事項

説明

収録刊行物

被引用文献 (2)*注記

参考文献 (18)*注記

関連プロジェクト

詳細情報 詳細情報について

書き出し

問題の指摘

詳細情報詳細情報について