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Spatial Mapping of Kilopixel Kinetic Inductance Detector Arrays for PRIMA

MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY XII, PT 1(2024)

CALTECH

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Abstract
We present a characterization of the mapping from resonant frequency to spatial position for a kilopixel kinetic inductance detector (KID) array developed for the Probe far-Infrared Mission for Astrophysics (PRIMA). This work targets the longest wavelength band of PRIMA's FIRESS spectrometer, which in total spans 24 to 235 mu m. Light emitting diodes arrayed to match repeating unit cells of 16 KIDs first discriminate among unit cells. Within each unit cell, frequencies are widely spaced, so positions are discriminated by theoretical predictions of the relative frequency spacing between detectors based on KID geometries. With this mapping, we analyze board features to improve the accuracy of modeling PRIMA KIDs and inform future fabrication runs.
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Key words
Kinetic Inductance Detectors,Far-Infrared,PRIMA,Multiplexed readout,Radio frequency system on a chip,RFSoC
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