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Cooled scientific instrument assembly onboard SPICA

Authors :
Shinji Mitani
M. Kawada
G. Crone
Takao Nakagawa
Toshihiko Yamawaki
Hideo Matsuhara
Hiroyuki Sugita
K. Isaak
Y. Sato
Yasuhiro Kawakatsu
Hiroshi Murakami
A. Heske
Keisuke Shinozaki
Source :
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave.
Publication Year :
2012
Publisher :
SPIE, 2012.

Abstract

The Space Infrared Telescope for Cosmology and Astrophysi cs (SPICA) is a 3.2m cooled (below 6K) telescope mission which covers mid- and far-IR waveband with unprecedented sensitivity. An overview of recent design updates of the Scientific Instrument Assembly (SIA), composed of the telescope assembly and the instrument optical bench equipped with Focal Plane Instruments (FPIs) are presented. The FPI international science and engineering review is on-going to determine the FPI suite onboard SPICA: at present the mandatory instruments and functions to perform the unique science objectives of the SPICA mission are now consolidated. The final decision on the composition of the FPI suite is expected in early 2013. Through the activities in the current pre-project phase, several key technical issues which impact directly on the instrumentsÂ’ performances and the science requirements and the observing efficiency have been identified, and extensive works are underway both at instrument and spacecraft level to reso lve these issues and to enable the confirmation of the SPICA FPI suite. Keywords: SPICA, space telescope, Joule-T homson cooler , infrared astronomy

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
Accession number :
edsair.doi...........896871037df95c460a2ed456486fec96
Full Text :
https://doi.org/10.1117/12.926984