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arxiv: 2404.10246 · v3 · pith:7OSPQH6Vnew · submitted 2024-04-16 · 🌌 astro-ph.IM · physics.ins-det

A 25-micron single photon sensitive kinetic inductance detector

classification 🌌 astro-ph.IM physics.ins-det
keywords opticaldetectordetectorspowerinductancekineticmicronmode
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We report measurements characterizing the performance of a kinetic inductance detector array designed for a wavelength of 25 microns and very low optical background level suitable for applications such as a far-infrared instrument on a cryogenically cooled space telescope. In a pulse counting mode of operation at low optical flux, the detectors can resolve individual 25-micron photons. In an integrating mode, the detectors remain photon noise limited over more than six orders of magnitude in absorbed power from 70 zW to 200 fW, with a limiting NEP of 4.6 x 10^-20 W/rtHz at 1 Hz. In addition, the detectors are highly stable with flat power spectra under optical load down to 1 mHz. Operational parameters of the detector are determined including the efficiency of conversion of the incident optical power into quasiparticles in the aluminum absorbing element and the quasiparticle self-recombination constant.

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