Characterization of High Aspect-Ratio TiAu TES X-ray Microcalorimeter Array Under AC Bias

Journal Article (2019)
Author(s)

E. Taralli (SRON–Netherlands Institute for Space Research)

L Gottardi (SRON–Netherlands Institute for Space Research)

K. Nagayoshi (SRON–Netherlands Institute for Space Research)

M Ridder (SRON–Netherlands Institute for Space Research)

S Visser (SRON–Netherlands Institute for Space Research)

Pourya Khosropanah (SRON–Netherlands Institute for Space Research)

H. Akamatsu (SRON–Netherlands Institute for Space Research)

J van der Kuur (SRON–Netherlands Institute for Space Research)

M. Bruijn (SRON–Netherlands Institute for Space Research)

J.R. Gao (TU Delft - QN/Gao Lab, SRON–Netherlands Institute for Space Research)

Research Group
QN/Gao Lab
DOI related publication
https://doi.org/10.1007/s10909-019-02254-y
More Info
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Publication Year
2019
Language
English
Research Group
QN/Gao Lab
Issue number
1-2
Volume number
199
Pages (from-to)
80-87

Abstract

We are developing X-ray microcalorimeters as a backup option for the baseline detectors in the X-IFU instrument on board the ATHENA space mission led by ESA and to be launched in the early 2030s. 5 × 5 mixed arrays with TiAu transition-edge sensor (TES), which have different high aspect ratios and thus high resistances, have been designed and fabricated to meet the energy resolution requirement of the X-IFU instrument. Such arrays can also be used to optimize the performance of the frequency domain multiplexing (FDM) readout and lead to the final steps for the fabrication of a large detector array. In this work, we present the experimental results from tens of the devices with an aspect ratio (length-to-width) ranging from 1-to-1 up to 6-to-1, measured in a single-pixel mode with a FDM readout system developed at SRON/VTT. We observed a nominal energy resolution of about 2.5 eV at 5.9 keV at bias frequencies ranging from 1 to 5 MHz. These detectors are proving to be the best TES microcalorimeters ever reported in Europe, intending to meet the requirements of the X-IFU instrument, but also those of other future challenging X-ray space missions, fundamental physics experiments, plasma characterization and material analysis.

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