Poster + Paper
31 August 2022 Monolithic amplifier and current biasing for SQUID readout: AwaXe_v4
Si Chen, Damien Prêle, Manuel Gonzalez, Jean Mesquida, Bernard Courty, Didier Charrier, Jean Lesrel, Sylvie Blin, Guy Monier
Author Affiliations +
Conference Poster
Abstract
The X-IFU is one of the two instruments of the ESA ATHENA mission, offering an unprecedented high spectral resolution. In the detection and readout chain of the X-IFU, the first warm stage is the WFEE subsystem. It mainly includes low-noise amplifiers and current sources to read out and bias cryogenic stages. Based on the development of four previous versions of the ASICs dedicated to the WFEE, a new version has been recently developed to transfer analogue functions to a thinner SiGe technology node of 130 nm. This paper updates the development of this new ASIC.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Si Chen, Damien Prêle, Manuel Gonzalez, Jean Mesquida, Bernard Courty, Didier Charrier, Jean Lesrel, Sylvie Blin, and Guy Monier "Monolithic amplifier and current biasing for SQUID readout: AwaXe_v4", Proc. SPIE 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, 121813Z (31 August 2022); https://doi.org/10.1117/12.2629890
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KEYWORDS
Transistors

Amplifiers

X-ray telescopes

X-ray detectors

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