Transition edge sensor arrays for future FIR space missions

We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in <i>one</i> direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 104 pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.

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Publication Details

Published
2024-08-16
DOI
https://doi.org/10.1117/12.3019128
Citations
1
Primary Topic
Superconducting and THz Device Technology
Type
article
Field-Weighted Citation Impact
0.33
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article

Transition edge sensor arrays for future FIR space missions

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1 citations
Superconducting and THz Device Technology
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Transition edge sensor arrays for future FIR space missions

Johannes Staguhn, Stephen F. Maher, Archana Devasia, Ari-David Brown, Shannon M. Duff, Malcolm Durkin, Kevin L. Denis, Peter C. Nagler, Elmer H. Sharp, W. B. Doriese, Suzanne T. Staggs, Vilem Mikula, Edward J. Wollack, Jason Glenn, Mike J. DiPirro, Felipe A. Colazo Petit, B. Harrop, D. J. Fixsen
article en
1 citations

Abstract

We have obtained NASA funding to build and demonstrate Transition Edge Sensor (TES) based kilopixel arrays with the properties that match the requirements for cryogenic far-infrared space missions: the arrays are very closely tileable in <i>one</i> direction and have only a moderate gap in the other direction. This array architecture can meet the sampling- and pixel number requirement of ~ 104 pixels. Many details of the architecture have already been demonstrated individually, and the detector board will be optimized for the use of the latest cryogenic bump bonded NIST 2-D time domain SQUID readout multiplexers with a high density fanout scheme. Additionally, we use flex-lines that are very similar to those developed at Princeton University for the ACT project. We already have a pixel design that exceeds the continuum sensitivity requirements for a cryogenic space mission.

Goddard Space Flight Center (US), National Institute of Standards and Technology (US), Johns Hopkins University (US), Princeton University (US), Science Systems and Applications (United States) (US), University of Maryland, College Park (US)
Affordable and clean energy
Openalex Percentile: Top 35%
Superconducting and THz Device Technology
0.33
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