Abstract
The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision Science Program. The X-IFU consists of a large array of TES microcalorimeters that will operate at ~ 50 mK inside a sophisticated cryostat. A set of thin filters, highly transparent to X-rays, will be mounted on the cryostat thermal shields in order to attenuate the IR radiative load, to attenuate RF electromagnetic interferences, and to protect the detector from contamination. In this paper, we present the current thermal filters design, describe the filter samples developed/procured so far, and present preliminary results from the ongoing characterization tests.
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References
D. Barret et al., Proc. SPIE 9905, 99052F-1 (2016). https://doi.org/10.1117/12.223243
X. Barcons et al., J. Phys: Conf. Ser. 610, 1 (2015). https://doi.org/10.1088/1742-6596/610/1/012008
K. Nandra et al. (2013). arXiv preprint arXiv:1306.2307
M. Barbera et al., Proc. SPIE 9144, 91445U (2014). https://doi.org/10.1117/12.2057403
M. Barbera et al., J. Low Temp. Phys. 184, 706–711 (2016). https://doi.org/10.1007/s10909-016-1501-4
Statement of Work – Appendix 1 to the European Space Agency ITT AO/1-8786/16/NL/BJ entitled “Large area high-performance optical filter for X-ray instrumentation”
A. Ciaravella et al., Astrophys. J. (2018). https://doi.org/10.3847/1538-4357/aab9a3
Acknowledgements
The research leading to these results has received funding from ASI (Italian Space Agency) through the Contract No. 2015-046-R.0 and from the European Union’s Horizon 2020 Program under the AHEAD Project (Grant Agreement No. 654215). We acknowledge fruitful discussions and support by LUXEL corp.
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Barbera, M., Lo Cicero, U., Sciortino, L. et al. Preliminary Mechanical Characterization of Thermal Filters for the X-IFU Instrument on Athena. J Low Temp Phys 193, 793–798 (2018). https://doi.org/10.1007/s10909-018-1942-z
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DOI: https://doi.org/10.1007/s10909-018-1942-z