Brien, Thomas, Ade, Peter A. R. ![]() ![]() ![]() |
Abstract
We present a study of a cold-electron bolometer operating at 350 mK with a twin-slot antenna coupling radiation at 160 GHz. The detector’s absorbing element consists of degenerately-doped strained silicon and has Schottky contacts to superconducting aluminium leads. These contacts allow for direct electron cooling of the absorber to below the phonon temperature, enabling the cold-electron bolometer to achieve much faster time constants (τ < 1 μs) compared to conventional bolometric detectors while not sacrificing sensitivity. We measure both the dark and optically-loaded noise of the detector via a novel method of cross-correlating the outputs of two amplifiers in order to measure noise below the amplifier noise level. From this we measure the photon-noise limited noise-equivalent power of the detector to be 6.6×10^−17 W/rtHz when observing a 77-Kelvin source.
Item Type: | Conference or Workshop Item (Paper) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Funders: | STFC, EPSRC, Academy of Finland |
Date of Acceptance: | 14 September 2015 |
Last Modified: | 11 Jan 2023 17:10 |
URI: | https://orca.cardiff.ac.uk/id/eprint/90786 |
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