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arxiv: 1406.4010 · v2 · submitted 2014-06-16 · 🌌 astro-ph.IM · cond-mat.supr-con

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Photon-noise limited sensitivity in titanium nitride kinetic inductance detectors

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classification 🌌 astro-ph.IM cond-mat.supr-con
keywords noisedetectorsinductancekineticlimitedphoton-noisesensitivitytemperature
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We demonstrate photon-noise limited performance at sub-millimeter wavelengths in feedhorn-coupled, microwave kinetic inductance detectors (MKIDs) made of a TiN/Ti/TiN trilayer superconducting film, tuned to have a transition temperature of 1.4~K. Micro-machining of the silicon-on-insulator wafer backside creates a quarter-wavelength backshort optimized for efficient coupling at 250~\micron. Using frequency read out and when viewing a variable temperature blackbody source, we measure device noise consistent with photon noise when the incident optical power is $>$~0.5~pW, corresponding to noise equivalent powers $>$~3$\times 10^{-17}$ W/$\sqrt{\mathrm{Hz}}$. This sensitivity makes these devices suitable for broadband photometric applications at these wavelengths.

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