24 July 2014 ATHENA X-IFU detector cooling chain
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Abstract
The TES (Transition Edge Sensors) micro-calorimeter detector technology in the X-IFU instrument for ATHENA (Astrophyics of the Hot and Energetic universe - Europe’s next generation X-ray observatory ATHENA) will require cooling down to 50 mK, and a stable and quiet Electro-Magnetic and micro-vibrations environment. In order to achieve this temperature and environment, a cooling chain integrated in a compact cryostat with an optimized electromagnetic environment has to be developed. Critical technology developments are covered, such as mechanical cryocoolers, support structures, radiative and EMC shields, micro-vibrations reduction, and others.
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M. B. C. Branco, M. B. C. Branco, I. Charles, I. Charles, J. Butterworth, J. Butterworth, } "ATHENA X-IFU detector cooling chain", Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91445V (24 July 2014); doi: 10.1117/12.2056427; https://doi.org/10.1117/12.2056427
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