Published July 2025 | Version Published
Journal Article

Characterization of a Far-Infrared Kinetic Inductance Detector Prototype for PRIMA

Abstract

The PRobe far-Infrared Mission for Astrophysics (PRIMA) is under study as a potential far-IR space mission, featuring actively cooled optics, and both imaging and spectroscopic instrumentation. To fully take advantage of the low background afforded by a cold telescope, spectroscopy with PRIMA requires detectors with a noise equivalent power (NEP) better than 1×1019 W Hz1/2. To meet this goal, we are developing large format arrays of kinetic inductance detectors (KIDs) to work across the 25–250 μm range. Here, we present the design and characterization of a single pixel prototype detector optimized for 210 μm. The KID consists of a lens-coupled aluminum inductor-absorber connected to a niobium interdigitated capacitor to form a 2 GHz resonator. We have fabricated a small array with 28 KIDs, and we measure the performance of one of these detectors with an optical loading in the 0.01–300 aW range. At low loading, the detector achieves an NEP of 9×1020 W Hz1/2 at a 10 Hz readout frequency. An extrapolation of these measurements suggests this detector may remain photon noise limited at up to 20 fW of loading, offering a high dynamic range for PRIMA observations of bright astronomical sources.

Copyright and License

© 2025, IEEE.

Acknowledgement

The authors would like to thank J. Zmuidzinas for contributing to useful discussions and providing constructive criticism of the manuscript.

Funding

  • NASA ; Grant number: 80NSSC19K0489
  • Jet Propulsion Laboratory
  • California Institute of Technology

 

Additional details

Funding

National Aeronautics and Space Administration
80NSSC19K0489
California Institute of Technology
Jet Propulsion Laboratory

Dates

Available
2025-05-12
Published online

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