| Autor: |
Itsuki Sakon, Takao Nakagawa, Hiroshi Shibai, Naoki Isobe, Takuma Kokusho, Mitsunobu Kawada, Kohji Tsumura, Mitsuyoshi Yamagishi, Takuya Furuta, Daisuke Ishihara, Takafumi Ootsubo, Hideo Matsuhara, Koichi Nagase, Misato Fukagawa, Takehiko Wada, Jungmi Kwon, Shinki Oyabu, Hidehiro Kaneda, Takurou Tsuchikawa, Toyoaki Suzuki |
| Rok vydání: |
2018 |
| Předmět: |
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| Zdroj: |
Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. |
| Popis: |
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. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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