Poster + Paper
31 August 2022 CCAT-prime: optical and cryogenic design of the 850 GHz module for Prime-Cam
Anthony I. Huber, Scott C. Chapman, Adrian K. Sinclair, Locke D. Spencer, Jason E. Austermann, Steve K. Choi, Jesslyn Devina, Patricio A. Gallardo, Doug Henke, Zachary B. Huber, Ben Keller, Yaqiong Li, Lawrence T. Lin, Mike Niemack, Kayla M. Rossi, Eve M. Vavagiakis, Jordan D. Wheeler
Author Affiliations +
Conference Poster
Abstract
Prime-Cam is a first-generation instrument for the Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) Facility. The 850 GHz module for Prime-Cam will probe the highest frequency of all the instrument modules. We describe the parameter space of the 850 GHz optical system between the Fλ spacing, beam size, pixel sensitivity, and detector count. We present the optimization of an optical design for the 850 GHz instrument module for CCAT-prime. We further describe the development of the cryogenic RF chain design to accommodate 30 readout lines to read 41,400 kinetic inductance detectors (KIDs) within the cryogenic testbed.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Anthony I. Huber, Scott C. Chapman, Adrian K. Sinclair, Locke D. Spencer, Jason E. Austermann, Steve K. Choi, Jesslyn Devina, Patricio A. Gallardo, Doug Henke, Zachary B. Huber, Ben Keller, Yaqiong Li, Lawrence T. Lin, Mike Niemack, Kayla M. Rossi, Eve M. Vavagiakis, and Jordan D. Wheeler "CCAT-prime: optical and cryogenic design of the 850 GHz module for Prime-Cam", Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 121901D (31 August 2022); https://doi.org/10.1117/12.2630370
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KEYWORDS
Sensors

Cryogenics

Optical design

Lenses

Attenuators

Detector arrays

Monochromatic aberrations

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