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CCAT-prime: RFSoC Based Readout for Frequency Multiplexed Kinetic Inductance Detectors

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arxiv 2208.07465 v1 pith:5H2G35AH submitted 2022-08-15 astro-ph.IM physics.ins-det

classification astro-ph.IMphysics.ins-det
keywords readoutdesigndetectorsfrequencyinstrumentrfsocbandwidthfirmware
verification ladder T0 review T1 audit T2 compute T3 formal
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The Prime-Cam instrument on the Fred Young Submillimeter Telescope (FYST) is expected to be the largest deployment of millimeter and submillimeter sensitive kinetic inductance detectors to date. To read out these arrays efficiently, a microwave frequency multiplexed readout has been designed to run on the Xilinx Radio Frequency System on a Chip (RFSoC). The RFSoC has dramatically improved every category of size, weight, power, cost, and bandwidth over the previous generation readout systems. We describe a baseline firmware design which can read out four independent RF networks each with 500 MHz of bandwidth and 1000 detectors for ~30 W. The overall readout architecture is a combination of hardware, gateware/firmware, software, and network design. The requirements of the readout are driven by the 850 GHz instrument module of the 7-module Prime-Cam instrument. These requirements along with other constraints which have led to critical design choices are highlighted. Preliminary measurements of the system phase noise and dynamic range are presented.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. CCAT: Optical Responsivity, Noise, and Readout Optimization of KIDs for Prime-Cam

    astro-ph.IM 2025-10 conditional novelty 5.0 of 10

    Cold-load tests of 280 GHz TiN and Al KIDs for Prime-Cam show NEP degrades up to 2x with only ~0.2 pW of optical loading drift and depends strongly on readout tone power and placement.

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