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CCAT:弗雷德·杨亚毫米波望远镜的Prime-Cam仪器——概述与现状

CCAT: The Prime-Cam Instrument for the Fred Young Submillimeter Telescope -- Overview and Status

Eve M. Vavagiakis, Yuhan Wang, Lawrence T. Lin, Manuel Aravena, Jason E. Austermann, Frank Bertoldi, James Burgoyne, Victoria Butler, Scott Chapman, Steve K. Choi, Dongwoo Chung, Abigail Crites, Ankur Dev, Cody J. Duell, Michel Fich, Laura Fissel, Rodrigo G. Freundt, Eliza Gazda, Anthony I. Huber, Doug Johnstone, Ben Keller, Paul Malachuk, Alicia Middleton, Jenna Moore, Michael D. Niemack, Thomas Nikola, Yoko Okada, Darshan A. Patel, Tilak M. Patel, Dominik A. Riechers, Douglas Scott, Gordon J. Stacey, Benjamin J. Vaughan, Samantha Walker, Ruixuan, Xie

arXiv 2608.25111首次发表:更新:

AI 中文总结

本文介绍了为智利在建FYST研制的Prime-Cam仪器的设计、测试与部署进展,该仪器将大幅提升亚毫米波段测绘能力,计划2026年末集成后开展早期科学观测以探索宇宙相关问题。

AI 中文摘要

Prime-Cam是CCAT天文台6米口径弗雷德·杨亚毫米波望远镜(FYST)的第一代科学仪器,该望远镜正在智利阿塔卡马沙漠查南托山海拔5600米处建造。Prime-Cam在亚毫米波段的测绘速度将比现有设备高10倍以上,可在1.4-0.3毫米(220-850吉赫兹)波段实现前所未有的宽带和光谱测量。当完全配置时,Prime-Cam将在7个独立优化的仪器模块中部署超过10万个动力学电感探测器。CCAT合作组将借助Prime-Cam解决一系列科学目标,从大爆炸宇宙学到宇宙时间内的星系演化和恒星形成。Prime-Cam计划于2026年末集成到FYST中,随后利用280和350吉赫兹仪器模块开展为期一年的早期科学观测。我们讨论了直径1.8米的Prime-Cam接收机和280吉赫兹仪器模块的设计与实验室测试情况,并提供了部署状态和早期科学计划的最新进展。

英文摘要

Prime-Cam is a first-generation science instrument for the CCAT Observatory's six-meter aperture Fred Young Submillimeter Telescope (FYST), under construction at an elevation of 5600 m on Cerro Chajnantor in Chile's Atacama Desert. Prime-Cam will deliver over ten times greater mapping speed at submillimeter wavelengths than current facilities for unprecedented broadband and spectroscopic measurements in windows between 1.4 -- 0.3 mm (220 -- 850 GHz). When fully populated, Prime-Cam will field over 100,000 kinetic inductance detectors across seven independently optimized instrument modules. With Prime-Cam, the CCAT Collaboration will address a suite of science goals, from Big Bang cosmology, to galaxy evolution and star formation over cosmic time. Prime-Cam is scheduled for integration in FYST in late 2026, followed by a year of early science observations with the 280 and 350 GHz instrument modules. We discuss the design and in-lab testing of the 1.8-m diameter Prime-Cam receiver and 280 GHz instrument module, and give an update on deployment status and early science plans.

Comments24 pages, 9 figures, as submitted to SPIE Astronomical Telescopes + Instrumentation

Journal refProc. SPIE 14156, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XIII, 1415604 (20 Aug 2026)

DOI:10.1117/12.3105297

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