Kam Arnold

基本信息

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职业迁徙

个人简介

Kam's research focuses on measurement of the intensity and polarization of the Cosmic Microwave Background (CMB). His future plans include developing technology for the next generation of detectors/telescopes.

研究兴趣

论文共 155 篇作者统计合作学者相似作者

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The Simons Observatory: Large Diameter and Large Load-Capacity Superconducting Magnetic Bearing for a Millimeter-Wave Polarization Modulator

Daichi Sasaki, Junna Sugiyama,Kyohei Yamada, Bryce Bixler,Yuki Sakurai,Kam Arnold,Bradley R. Johnson,Akito Kusaka

arxiv（2025）

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Erratum: "the Simons Observatory: Cryogenic Half Wave Plate Rotation Mechanism for the Small Aperture Telescopes" [rev. Sci. Instrum. 95, 024504 (2024)]

K Yamada, B Bixler, Y Sakurai,P C Ashton, J Sugiyama,K Arnold, J Begin,L Corbett, S Day-Weiss,N Galitzki,C A Hill,B R Johnson, B Jost,A Kusaka,B J Koopman, J Lashner,A T Lee,A Mangu, H Nishino, L A Page, M J Randall, D Sasaki, X Song, J Spisak, T Tsan, Y Wang,P A Williams

The Review of scientific instruments（2025）

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The Simons Observatory: Validation of Reconstructed Power Spectra from Simulated Filtered Maps for the Small Aperture Telescope Survey