activity
20242026
collaborators

7 papers

astro-ph.IM2026

CCAT: Design and Characterization of the 350 GHz Instrument Module

Ben Keller, Jordan Wheeler, Cody J. Duell +24

The CCAT Collaboration's Prime-Cam instrument will soon be deployed to the Fred Young Submillimeter Telescope (FYST) in Chile's Atacama Desert. Featuring prominently in Prime-Cam's…

astro-ph.IM2026

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

Eliza Gazda, Quintin Meyers, James R. Burgoyne +18

The Prime-Cam instrument on the Fred Young Submillimeter Telescope (FYST) at the CCAT Observatory will conduct sensitive millimeter to submillimeter surveys for a range of astrophy…

astro-ph.IM2026

CCAT: Mod-Cam Readout Overview and Flexible Stripline Performance

Ben Keller, Rodrigo Freundt, James R. Burgoyne +14

The CCAT Observatory's primary science instrument, Prime-Cam, is nearing readiness for deployment to the Fred Young Submillimeter Telescope (FYST) in the Atacama Desert in northern…

astro-ph.IM2026

CCAT: Magnetic Sensitivity Measurements of Kinetic Inductance Detectors

Benjamin J. Vaughan, Yuhan Wang, Cody J. Duell +16

The CCAT Observatory is a ground-based submillimeter to millimeter experiment located on Cerro Chajnantor in the Atacama Desert, at an altitude of 5,600 meters. CCAT features the 6…

astro-ph.IM2025

CCAT: Design, Implementation, and Testing of a System to Read Out over 10,000 280 GHz KIDs using RFSoC Electronics

Darshan A. Patel, Yuhan Wang, Cody J. Duell +28

Over the past decade, kinetic inductance detectors (KIDs) have emerged as a viable superconducting technology for astrophysics at millimeter and submillimeter wavelengths. KIDs spa…

astro-ph.IM2025

CCAT: Mod-Cam Cryogenic Performance and its Impact on 280 GHz KID Array Noise

Lawrence T. Lin, Eve M. Vavagiakis, Jason E. Austermann +27

The CCAT Observatory's Fred Young Submillimeter Telescope (FYST) is designed to observe submillimeter astronomical signals with high precision, using receivers fielding state-of-th…