Development of the WFEE subsystem for the X-IFU instrument of the ATHENA Space Observatory

Si Chen; Damien Prêle; Cyril Beillimaz; Fabrice Voisin; Kuo Kwan Chan; Philippe Laurent; Andrea Goldwurm

doi:10.1117/12.2312710

6 July 2018 Development of the WFEE subsystem for the X-IFU instrument of the ATHENA Space Observatory

Si Chen, Damien Prêle, Cyril Beillimaz, Fabrice Voisin, Kuo Kwan Chan, Philippe Laurent, Andrea Goldwurm

Author Affiliations +

Proceedings Volume 10699, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray; 106994P (2018) https://doi.org/10.1117/12.2312710
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States

Abstract

The X-IFU is one of the two instruments of the ESA ATHENA space mission, at present in feasibility phase (phase A). It is an X-Ray spectral imager designed to have an unprecedented 2.5 eV spectral resolution at 6 keV. In the readout chain of the X-IFU, the first stage working at room temperature is the WFEE subsystem, currently being developed at APC laboratory. It will include low-noise amplifiers, current sources, RS485/I²C digital interfaces and housekeeping elements. A first ASIC dedicated to this subsystem has been designed and tested. The basic functions of the main components of the WFEE and its radiation-hardened abilities have been evaluated. According to the measurement results, a second ASIC is being developed, aiming to comply with the WFEE requirements in the X-IFU readout chain.

Citation Download Citation

Si Chen, Damien Prêle, Cyril Beillimaz, Fabrice Voisin, Kuo Kwan Chan, Philippe Laurent, and Andrea Goldwurm "Development of the WFEE subsystem for the X-IFU instrument of the ATHENA Space Observatory", Proc. SPIE 10699, Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray, 106994P (6 July 2018); https://doi.org/10.1117/12.2312710

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