Future far-infrared astronomy missions will need large arrays of detectors with exceptionally low noise-equivalent power (NEP), with some mission concepts calling for thousands of detectors with NEPs below a few ×10−20 W/Hz. Though much progress has been made toward meeting this goal, such detector systems do not exist today. In this work, we present a device that offers a compelling path forward: the longitudinal proximity effect (LoPE) transition-edge sensor (TES). With a chemically-stable and mechanically-robust architecture, the LoPE TES we designed, fabricated, and characterized also exhibits unprecedented sensitivity, with a measured electrical NEP of 8×10−22 W/Hz. This represents a >100x advancement of the state-of-the-art, pushing TES detectors into the regime where they may be employed the achieve to goals of even the most ambitious large and cold future space instruments.
@article{arxiv.2012.06543,
title = {Demonstration of ultra-low noise equivalent power using a longitudinal proximity effect transition-edge sensor},
author = {Peter C. Nagler and John E. Sadleir and Edward J. Wollack},
journal= {arXiv preprint arXiv:2012.06543},
year = {2020}
}