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The Prime-Cam receiver on the Fred Young Submillimeter Telescope for theCCAT-prime project aims to address important astrophysical and cosmologicalquestions with sensitive broadband, polarimetric, and spectroscopicmeasurements. The primary frequency bands in development include 280, 350, and850 GHz for the polarization-sensitive broadband channels and 210--420 GHz forthe spectrometers. Microwave kinetic inductance detectors (MKIDs) are a naturalchoice of detector technology for the simplicity in multiplexed readout neededfor large format arrays at these high frequencies. We present here the initiallab characterization of the feedhorn-coupled 280 GHz polarimetric MKID array,and outline the plans for the subsequent MKID arrays and the development of thetestbed to characterize them.

CCAT-prime: Characterization of the First 280 GHz MKID Array for Prime-Cam