CCAT: Detector Noise Limited Performance of the RFSoC-based Readout Electronics for mm/sub-mm/far-IR KIDs

Bibliographic Details
Title: CCAT: Detector Noise Limited Performance of the RFSoC-based Readout Electronics for mm/sub-mm/far-IR KIDs
Authors: Sinclair, Adrian K., Burgoyne, James, Huber, Anthony I., Murphy, Colin, Choi, Steve K., Duell, Cody J., Huber, Zachary B., Li, Yaqiong, Chapman, Scott C., Niemack, Michael D., Nikola, Thomas, Vavagiakis, Eve M., Walker, Samantha, Wheeler, Jordan D., Austermann, Jason, Lin, Lawrence, Xie, Ruixuan, Zou, Bugao, Mauskopf, Philip D.
Publication Year: 2024
Collection: Astrophysics
Physics (Other)
Subject Terms: Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
More Details: The Fred Young Submillimeter Telescope (FYST), on Cerro Chajnantor in the Atacama desert of Chile, will conduct wide-field and small deep-field surveys of the sky with more than 100,000 detectors on the Prime-Cam instrument. Kinetic inductance detectors (KIDs) were chosen as the primary sensor technology for their high density focal plane packing. Additionally, they benefit from low cost, ease of fabrication, and simplified cryogenic readout, which are all beneficial for successful deployment at scale. The cryogenic multiplexing complexity is pulled out of the cryostat and is instead pushed into the digital signal processing of the room temperature electronics. Using the Xilinx Radio Frequency System on a Chip (RFSoC), a highly multiplexed KID readout was developed for the first light Prime-Cam and commissioning Mod-Cam instruments. We report on the performance of the RFSoC-based readout with multiple detector arrays in various cryogenic setups. Specifically we demonstrate detector noise limited performance of the RFSoC-based readout under the expected optical loading conditions.
Comment: draft submitted to SPIE
Document Type: Working Paper
Access URL: http://arxiv.org/abs/2406.14892
Accession Number: edsarx.2406.14892
Database: arXiv
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