Si Chen,1 Damien Prêle,1 Manuel Gonzalez,1 Jean Mesquida,1 Bernard Courty,1 Michael Punch,1 Luis Horacio Arnaldi,1 Bao That Minh Ton,1 Jean Lesrelhttps://orcid.org/0000-0002-3599-94701
1Univ. Paris Cité, CNRS, Astroparticule et Cosmologie (France)
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This paper gives a review of the ASIC design evolutions of the WFEE in the context of the ATHENA mission. The development follows the evolutions of the X-IFU instrument detection chain and secures the ASIC technology access continuity by using an ST SiGe 130 nm technology instead of the previous use of an AMS SiGe 350 nm node. First ASIC prototypes based on this ST 130 nm SiGe technology have been developed to answer these technical challenges and meet the new requirements. This paper will give a brief review of these ASICs dedicated to the WFEE.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Si Chen,Damien Prêle,Manuel Gonzalez,Jean Mesquida,Bernard Courty,Michael Punch,Luis Horacio Arnaldi,Bao That Minh Ton , andJean Lesrel
"ASIC design evolution of ATHENA X-IFU warm front-end electronics", Proc. SPIE 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, 130934J (21 August 2024); https://doi.org/10.1117/12.3020115
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Si Chen, Damien Prêle, Manuel Gonzalez, Jean Mesquida, Bernard Courty, Michael Punch, Luis Horacio Arnaldi, Bao That Minh Ton , Jean Lesrel, "ASIC design evolution of ATHENA X-IFU warm front-end electronics," Proc. SPIE 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, 130934J (21 August 2024); https://doi.org/10.1117/12.3020115