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SPICA Mid-infrared Instrument (SMI): technical concepts and scientific capabilities

Authors :
Hiroshi Shibai
Itsuki Sakon
Mitsuyoshi Yamagishi
Kohji Tsumura
Hideo Matsuhara
Hidehiro Kaneda
Takehiko Wada
Mitsunobu Kawada
Taro Matsuo
Kentaroh Asano
Daisuke Ishihara
Naoki Isobe
Toyoaki Suzuki
Shinki Oyabu
Takao Nakagawa
Source :
SPIE Proceedings.
Publication Year :
2016
Publisher :
SPIE, 2016.

Abstract

SMI (SPICA Mid-infrared Instrument) is one of the two focal-plane scientific instruments planned for new SPICA, and the Japanese instrument proposed and managed by a university consortium in Japan. SMI covers the wavelength range of 12 to 36 μm, using the following three spectroscopic channels with unprecedentedly high sensitivities: low-resolution spectroscopy (LRS; R = 50 - 120, 17 - 36 μm), mid-resolution spectroscopy (MRS; R = 1300 - 2300, 18 - 36 μm), and high-resolution spectroscopy (HRS; R = 28000, 12 - 18 μm). The key functions of these channels are high-speed dustband mapping with LRS, high-sensitivity multi-purpose spectral mapping with MRS, and high-resolution molecular-gas spectroscopy with HRS. This paper describes the technical concept and scientific capabilities of SMI.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi...........0afcb4f919296c1bb1757c055bc89a06
Full Text :
https://doi.org/10.1117/12.2232442