作者: Bruce Swinyard , Takao Nakagawa , None
DOI: 10.1007/S10686-008-9090-0
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摘要: The Space Infrared telescope for Cosmology and Astrophysics (SPICA) is planned to be the next space astronomy mission observing in infrared. launched 2017 will feature a 3.5 m cooled 30 microns wavelength). We describe scientific advances that made possible by this large increase sensitivity give details of mission, spacecraft focal plane conceptual design.