Poster + Paper
16 August 2024 Development of an ultra-sensitive 210-micron array of KIDs for far-IR astronomy
Author Affiliations +
Conference Poster
Abstract
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.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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, and 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
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KEYWORDS
Sensors

Black bodies

Histograms

Resonators

Detector arrays

Inductance

Background noise

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