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Assembling the Cryogenic Front-end for the ALPACA Phased Array Feed

https://doi.org/10.23919/USNC-URSI54200.2023.10289395

Vishwas, Amit; Gull, George E; Parshley, Stephen C; Cortes-Medellin, German; Campbell, Donald B; Herter, Terry L; Groppi, Christopher E; Burnett, Mitchell C; Warnick, Karl F; Jeffs, Brian D (July 2023, IEEE USNC-URSI Radio Science Meeting Proceedings)

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Cryogenic Noise-Parameter Measurements: Recent Research and a Fully Automated Measurement Application

https://doi.org/10.1109/MMM.2021.3078027

Sheldon, Alexander; Belostotski, Leonid; Mani, Hamdi; Groppi, Christopher E.; Warnick, Karl F. (August 2021, IEEE Microwave Magazine)

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Automated Noise-Parameter Measurements of Cryogenic LNAs

https://doi.org/10.1109/ARFTG52261.2021.9639993

Sheldon, Alexander; Belostotski, Leonid; Mani, Hamdi; Groppi, Christopher E.; Warnick, Karl F. (June 2021, 2021 97th ARFTG Microwave Measurement Conference (ARFTG))

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CCAT-prime: RFSoC based readout for frequency multiplexed kinetic inductance detectors

https://doi.org/10.1117/12.2629722

Sinclair, Adrian K; Stephenson, Ryan C; Roberson, Cody; Weeks, Eric L; Burgoyne, James; Huber, Anthony I; Mauskopf, Philip D; Chapman, Scott C; Austermann, Jason E; Choi, Steve K; et al (August 2022, SPIE)
Zmuidzinas, Jonas; Gao, Jian-Rong (Ed.)
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CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

https://doi.org/10.3847/1538-4365/ac9838

CCAT-Prime Collaboration; Aravena, Manuel; Austermann, Jason E.; Basu, Kaustuv; Battaglia, Nicholas; Beringue, Benjamin; Bertoldi, Frank; Bigiel, Frank; Bond, J. Richard; Breysse, Patrick C.; et al (December 2022, The Astrophysical Journal Supplement Series)

Abstract We present a detailed overview of the science goals and predictions for the Prime-Cam direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST is a wide-field, 6 m aperture submillimeter telescope being built (first light in late 2023) by an international consortium of institutions led by Cornell University and sited at more than 5600 m on Cerro Chajnantor in northern Chile. Prime-Cam is one of two instruments planned for FYST and will provide unprecedented spectroscopic and broadband measurement capabilities to address important astrophysical questions ranging from Big Bang cosmology through reionization and the formation of the first galaxies to star formation within our own Milky Way. Prime-Cam on the FYST will have a mapping speed that is over 10 times greater than existing and near-term facilities for high-redshift science and broadband polarimetric imaging at frequencies above 300 GHz. We describe details of the science program enabled by this system and our preliminary survey strategies.
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