Paper
6 July 2018 The performance of the ATHENA X-ray Integral Field Unit
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Abstract
The X-ray Integral Field Unit (X-IFU) is a next generation microcalorimeter planned for launch onboard the Athena observatory. Operating a matrix of 3840 superconducting Transition Edge Sensors at 90 mK, it will provide unprecedented spectro-imaging capabilities (2.5 eV resolution, for a field of view of 5’) in the soft X-ray band (0.2 up to 12 keV), enabling breakthrough science. The definition of the instrument evolved along the phase A study and we present here an overview of its predicted performances and their modeling, illustrating how the design of the X-IFU meets its top-level scientific requirements. This article notably covers the energy resolution, count-rate capability, quantum efficiency and non X-ray background levels, highlighting their main drivers.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Philippe Peille, Roland den Hartog, Claudio Macculi, Marco Barbera, Simone Lotti, Edoardo Cucchetti, Christian Kirsch, Thomas Dauser, Joern Wilms, Simon R. Bandler, Stephen J. Smith, Brian Jackson, Hervé Geoffray, Jean-Michel Mesnager, François Pajot, Didier Barret, Thien Lam-Trong, Jan-Willem den Herder, and Luigi Piro "The performance of the ATHENA X-ray Integral Field Unit", Proc. SPIE 10699, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, 106994K (6 July 2018); https://doi.org/10.1117/12.2313720
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Cited by 3 scholarly publications.
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KEYWORDS
X-rays

Sensors

Quantum efficiency

Mirrors

Optical filters

Image resolution

Contamination

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