CCAT-prime: a novel telescope for submillimeter astronomy
Stephen C. Parshley, J\"org Kronshage, James Blair, Terry Herter, Mike, Nolta, Gordon J. Stacey, Andrew Bazarko, Frank Bertoldi, Ricardo Bustos,, Donald B. Campbell, Scott Chapman, Nicholas Cothard, Mark Devlin, Jens Erler,, Michel Fich, Patricio A. Gallardo, Riccardo Giovanelli

TL;DR
The CCAT-prime telescope is a high-altitude, large-field, submillimeter observatory with innovative design features enabling advanced millimeter and sub-millimeter astronomical observations over a 15-year operational lifetime.
Contribution
This paper introduces the design and specifications of the novel CCAT-prime telescope, including its optics, mount, materials, and operational features, advancing submillimeter astronomy capabilities.
Findings
Unobscured optics with 8-degree field of view
Temperature-insensitive mount using Invar and CFRP
Designed for remote operation with minimal maintenance
Abstract
The CCAT-prime telescope is a 6-meter aperture, crossed-Dragone telescope, designed for millimeter and sub-millimeter wavelength observations. It will be located at an altitude of 5600 meters, just below the summit of Cerro Chajnantor in the high Atacama region of Chile. The telescope's unobscured optics deliver a field of view of almost 8 degrees over a large, flat focal plane, enabling it to accommodate current and future instrumentation fielding >100k diffraction-limited beams for wavelengths less than a millimeter. The mount is a novel design with the aluminum-tiled mirrors nested inside the telescope structure. The elevation housing has an integrated shutter that can enclose the mirrors, protecting them from inclement weather. The telescope is designed to co-host multiple instruments over its nominal 15 year lifetime. It will be operated remotely, requiring minimum maintenance and…
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