System performance of a cryogenic test-bed for the time-division multiplexing readout for the NewAthena X-ray Integral Field Unit

The X-ray Integral Field Unit (X-IFU) is an instrument of European Space Agency’s future NewAthena space observatory, with the goal to provide high-energy resolution (<4 eV at X-ray energies up to 7 keV) and high-spatial resolution (9 in.) spectroscopic imaging over the X-ray energy range from 200 eV to 12 keV, by means of an array of ∼1500 transition-edge sensors (TESs) read out via superconducting quantum interference device time-division multiplexing (TDM). A TDM-based laboratory test bed has been assembled at Netherlands Institute for Space Research, hosting an array of 75×75 μm2 TESs that are read out via 2-column × 32-row TDM. A system component that is critical to high-performance operation is the wiring harness that connects the room-temperature electronics to the cryogenic readout componentry. We report here on our characterization of such a test bed, whose harness has a length close to what was envisioned for X-IFU, which allowed us to achieve a co-added energy resolution at a level of 2.7-eV full width half maximum at 6 keV via 32-row readout. In addition, we provide an outlook on the integration of TDM readout into the X-IFU focal plane assembly development model.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2024-12-10
DOI
https://doi.org/10.1117/1.jatis.10.4.046002
Primary Topic
Superconducting and THz Device Technology
Type
article
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article

System performance of a cryogenic test-bed for the time-division multiplexing readout for the NewAthena X-ray Integral Field Unit

Tobias Vos, Brian J. Jackson, Stephen J. Smith, S. R. Bandler et al.
Journal of Astronomical Telescopes Instruments and Systems
Superconducting and THz Device Technology
article

System performance of a cryogenic test-bed for the time-division multiplexing readout for the NewAthena X-ray Integral Field Unit

Tobias Vos, Brian J. Jackson, Stephen J. Smith, S. R. Bandler, A. Simionescu, Malcolm Durkin, K. Ravensberg, J. van der Kuur, D. A. Bennett, W. B. Doriese, Kazuhiro Sakai, E. Taralli, Jan-Willem A. den Herder, Martin de Wit, Joel N. Ullom, Paul van der Hulst, J. R. Adams, Nicholas A. Wakeham, J. R. Gao, P. Khosropanah, D. Vaccaro, Carl D. Reintsema, James A. Chervenak, Luciano Gottardi, Peter Roelfsema, J. Gard
article en

Abstract

The X-ray Integral Field Unit (X-IFU) is an instrument of European Space Agency’s future NewAthena space observatory, with the goal to provide high-energy resolution (<4 eV at X-ray energies up to 7 keV) and high-spatial resolution (9 in.) spectroscopic imaging over the X-ray energy range from 200 eV to 12 keV, by means of an array of ∼1500 transition-edge sensors (TESs) read out via superconducting quantum interference device time-division multiplexing (TDM). A TDM-based laboratory test bed has been assembled at Netherlands Institute for Space Research, hosting an array of 75×75 μm2 TESs that are read out via 2-column × 32-row TDM. A system component that is critical to high-performance operation is the wiring harness that connects the room-temperature electronics to the cryogenic readout componentry. We report here on our characterization of such a test bed, whose harness has a length close to what was envisioned for X-IFU, which allowed us to achieve a co-added energy resolution at a level of 2.7-eV full width half maximum at 6 keV via 32-row readout. In addition, we provide an outlook on the integration of TDM readout into the X-IFU focal plane assembly development model.

Journal of Astronomical Telescopes Instruments and SystemsVol. 10(04)
Goddard Space Flight Center (US), National Institute of Standards and Technology (US), University of Colorado Boulder (US), Dutch Research Council (NL), Space Research Organisation Netherlands (NL), University of Maryland, Baltimore County (US), University of Amsterdam (NL)
Climate action
Openalex Percentile: Top 84%
Superconducting and THz Device Technology
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