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Conceptual design of the detection chain for the X-IFU on Athena

Authors :
W. Bertrand Doriese
Hervé Geoffray
Malcom Durkin
A. Argan
Stephen J. Smith
Joe Adams
Yann Parot
Bert Joost van Leeuwen
Simon R. Bandler
Jan-Willem den Herder
Frank Brachet
Claudio Macculi
Brian Jackson
M. Barbera
Didier Barret
James A. Chervenak
Damien Prêle
L. Ravera
Carl D. Reintsema
Ruud W. M. Hoogeveen
Jan van der Kuur
Joel N. Ullom
Henk van Weers
Luigi Piro
Mikko Kirivanta
Aurélien Ledot
Source :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray.
Publication Year :
2020
Publisher :
SPIE, 2020.

Abstract

CNES (French Space Agency) is in charge of the development of the X-IFU instrument for Athena. The main sensor array detection chain sub-system of the X-IFU instrument is one of the major sub-subsystem of the instrument, as the main contributor to the performance. This sub-system involves major partners of the X-IFU instrument, e.g GFSC, SRON, VTT, APC, and IRAP. The purpose of this paper is to present the baseline of the definition of the X-IFU detection chain in the frame at end of phase A/beginning of phase B. The readout is based on Time Domain Multiplexing (TDM). There are strong design issues which couple the different sub-components of the detection chain (the main sensor array, the cold electronics stages, and the warm electronics). The detection chain environment (thermal, mechanical and EMI/EMC environment) also requires a transverse analysis. This paper focuses on those aspects while providing design description of the sub-components of the detection chain.

Details

Database :
OpenAIRE
Journal :
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Accession number :
edsair.doi...........e4e51083c36880fe96bd60c21dd7aee3