Elijah Kane,1 Chris Albert,1 Nicholas Cothard,2 Steven Hailey-Dunsheath,1 Pierre Echternach,3 Logan Foote,1 Reinier M. Janssenhttps://orcid.org/0000-0001-9122-9668,3 Henry (Rick) LeDuc,3 Lun-Jun (Simon) Liu,1 Hien Nguyen,3 Jason Glenn,2 Charles (Matt) Bradford,3 Jonas Zmuidzinas1
1California Institute of Technology (United States) 2NASA Goddard Space Flight Ctr. (United States) 3Jet Propulsion Lab. (United States)
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The Probe far-Infrared Mission for Astrophysics (PRIMA) is a proposed space observatory which will use arrays of thousands of kinetic inductance detectors (KIDs) to perform low- and moderate-resolution spectroscopy throughout the far-infrared. The detectors must have noise equivalent powers (NEPs) at or below 1×10−19 W Hz−1/2 to be subdominant to noise from sky backgrounds and thermal noise from PRIMA’s cryogenically cooled primary mirror. Using a Radio Frequency System on a Chip for multitone readout, we measure the NEPs of detectors on a flight-like array designed to observe at a wavelength of 210 μm. We find that 92% of the KIDs measured have an NEP below 1 × 10−19 W Hz−1/2 at a noise frequency of 10 Hz.
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Elijah Kane, Chris Albert, Nicholas Cothard, Steven Hailey-Dunsheath, Pierre Echternach, Logan Foote, Reinier M. Janssen, Henry (Rick) LeDuc, Lun-Jun (Simon) Liu, Hien Nguyen, Jason Glenn, Charles (Matt) Bradford, Jonas Zmuidzinas, "Development of an ultra-sensitive 210-micron array of KIDs for far-IR astronomy," Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131021K (16 August 2024); https://doi.org/10.1117/12.3020346