Proceedings Paper
FIS: far-infrared surveyor on board ASTRO-F (IRIS)| Format | Member Price | Non-Member Price |
|---|---|---|
| $17.00 | $21.00 |
Paper Abstract
The ASTRO-F project is currently in its final stage of proto-model, which is constructed same as flight-model. Since instrument goals of the Far-Infrared Surveyor (FIS) are unprecedented achievement of high sensitivity and high spatial resolution in far-infrared wavelength, the proto- model stage is important to prove the performance as the flight instrument. We mainly present here the latest optical, thermal, and mechanical properties of the proto- model of the FIS.
Paper Details
Date Published: 28 July 2000
PDF: 12 pages
Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); doi: 10.1117/12.393984
Published in SPIE Proceedings Vol. 4013:
UV, Optical, and IR Space Telescopes and Instruments
James B. Breckinridge; Peter Jakobsen, Editor(s)
PDF: 12 pages
Proc. SPIE 4013, UV, Optical, and IR Space Telescopes and Instruments, (28 July 2000); doi: 10.1117/12.393984
Show Author Affiliations
Hidenori Takahashi, Nagoya Univ. and Japan Science and Technology Corp. (Japan)
Hiroshi Shibai, Nagoya Univ. (Japan)
Mitsunobu Kawada, Nagoya Univ. (Japan)
Takanori Hirao, Nagoya Univ. (Japan)
Toyoki Watabe, Nagoya Univ. (Japan)
Yasushi Tsuduku, Nagoya Univ. (Japan)
Hirohisa Nagata, Nagoya Univ. (Japan)
Hiroshi Utsuno, Nagoya Univ. (Japan)
Yasushi Hibi, Nagoya Univ. (Japan)
Shinya Hirooka, Nagoya Univ. (Japan)
Takao Nakagawa, Institute of Space and Astronautical Science (Japan)
Hiroshi Shibai, Nagoya Univ. (Japan)
Mitsunobu Kawada, Nagoya Univ. (Japan)
Takanori Hirao, Nagoya Univ. (Japan)
Toyoki Watabe, Nagoya Univ. (Japan)
Yasushi Tsuduku, Nagoya Univ. (Japan)
Hirohisa Nagata, Nagoya Univ. (Japan)
Hiroshi Utsuno, Nagoya Univ. (Japan)
Yasushi Hibi, Nagoya Univ. (Japan)
Shinya Hirooka, Nagoya Univ. (Japan)
Takao Nakagawa, Institute of Space and Astronautical Science (Japan)
Hidehiro Kaneda, Institute of Space and Astronautical Science (Japan)
Shuji Matsuura, Institute of Space and Astronautical Science (Japan)
Tsuneo Kii, Institute of Space and Astronautical Science (Japan)
Shin'ichiro Makiuti, Institute of Space and Astronautical Science (Japan)
Yoshihiko Okamura, Institute of Space and Astronautical Science (Japan)
Yasuo Doi, Univ. of Tokyo (Japan)
Hiroshi Matsuo, National Astronomical Observatory of Japan (Japan)
Norihisa Hiromoto, Communications Research Lab. (Japan)
Mikio Fujiwara, Communications Research Lab. (Japan)
Manabu Noda, Nagoya City Science Museum (Japan)
Shuji Matsuura, Institute of Space and Astronautical Science (Japan)
Tsuneo Kii, Institute of Space and Astronautical Science (Japan)
Shin'ichiro Makiuti, Institute of Space and Astronautical Science (Japan)
Yoshihiko Okamura, Institute of Space and Astronautical Science (Japan)
Yasuo Doi, Univ. of Tokyo (Japan)
Hiroshi Matsuo, National Astronomical Observatory of Japan (Japan)
Norihisa Hiromoto, Communications Research Lab. (Japan)
Mikio Fujiwara, Communications Research Lab. (Japan)
Manabu Noda, Nagoya City Science Museum (Japan)
Published in SPIE Proceedings Vol. 4013:
UV, Optical, and IR Space Telescopes and Instruments
James B. Breckinridge; Peter Jakobsen, Editor(s)
© SPIE. Terms of Use
