Mr. Sven Visser Profile

Sven Visser

at SRON Netherlands Institute for Space Research

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Author

Publications (3)

Proceedings Article | 17 August 2024 Presentation

PRIMA: demonstration of a high-efficiency 25-45 μm Linear Variable Filter for PRIMAger

Willem Jellema, Marcel Bruijn, Kenichiro Nagayoshi, Marcel Ridder, Nathalie Gorter, Martin Eggens, Erik van der Meer, Robert Huisman, Sven Visser, Sander van Loon, Sanghati Roy, Laure Ciesla, Denis Burgarella, Marc Sauvage, C. Darren Dowell, Jason Glenn

Proceedings Volume PC13102, PC1310210 (2024) https://doi.org/10.1117/12.3020634

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Proceedings Article | 13 December 2020 Poster

Optimizing normal resistance of an x-ray transition edge sensor for frequency domain multiplexing

Kenichiro Nagayoshi, Martin de Wit, Luciano Gottardi, Marcel Ridder, Sven Visser, Emanuele Taralli, Hiroki Akamatsu, Marcel Bruijn, Jian-Rong Gao, Ruud W. Hoogeveen, Jan-Willem den Herder

Proceedings Volume 11444, 114444C (2020) https://doi.org/10.1117/12.2562782

KEYWORDS: X-rays, Sensors, Space observatories, Superconductors, X-ray imaging, Spectral resolution, Fused deposition modeling, Resistance, Space telescopes, Spectroscopy

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Athena is an ESA-led space telescope to be launched in the early 2030s. The X-ray Integral Field Unit (X-IFU) on board of the Athena mission is an X-ray imaging spectrometer, sensitive to 0.2-12 keV X-rays. The main sensor of the X-IFU is an array of ~3200 closely-packed superconducting transition-edge sensor (TES) microcalorimeters with X-ray absorbers. The X-IFU provides a breakthrough spectral resolution of 2.5 eV (full width at half maximum; FWHM) at 6 keV, which enables us to access unrevealed properties of the hot gases that are formed at every level of the hierarchical structure of the universe. At SRON, we are developing Frequency Division Multiplexing (FDM) readout with SQUID amplifiers as a baseline technology for the X-IFU. In the FDM system, the microcalorimeter pixels are AC-biased at different frequencies from 1 to 5 MHz. Therefore, it is crucial to minimize frequency-dependent phenomena because it causes non-linearity effects in the detector response and degrades the spectral resolution. Theoretical analyses have shown that this non-linearity is caused by weak-link behavior, induced by superconducting leads and can be mitigated by increasing the normal resistance of the TES. We are also developing TES arrays based on a superconducting Ti/Au bi-layer with an Au absorber as a sensor backup technology for the X-IFU. We have recently fabricated TES calorimeters with large variation of normal resistance from 25 to 150 mΩ by changing the width and aspect ratio of the bi-layer. The TESes with 117 and 150 mΩ have shown a promising spectral performance of below 2 eV (FWHM) at 6 keV. However, we still see that the detector response is affected by the weak-link behavior, especially at high frequency regime. In this paper, we briefly summarize our results with a focus on the spectral performance and the detector responsivity for each TES design. We also present our recent works on fabrication related to a superconducting wiring process, which would be useful for further reduction of the weak-link effects.

Proceedings Article | 13 December 2020 Presentation

Frequency domain multiplexing technology of transition-edge sensors for x-ray astronomy

Hiroki Akamatsu, Davide Vaccaro, Luciano Gottardi, Jan van der Kuur, Cor de Vries, Simon Bandler, Marcel Bruijn, James Chervenak, Matteo D'Andrea, Jian-Rong Gao, Jan-Willem den Herder, Ruud W. Hoogeveen, Mikko Kiviranta, Anton van der Linden, Brian Jackson, Antoine Miniussi, Kenichiro Nagayoshi, Kevin Ravensberg, Marcel Ridder, Kazuhiro Sakai, Stephen Smith, Emanuele Taralli, Sven Visser, Nicholas Wakeham, Martin de Wit

Proceedings Volume 11444, 114440Y (2020) https://doi.org/10.1117/12.2561271

KEYWORDS: Multiplexing, Sensors, Fused deposition modeling, Sensor technology, X-ray astronomy, X-rays, Resonators, Observatories, Quantum efficiency, Spectral resolution

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