The cosmic microwave background and how we measure it (3/9)

by Kam Arnold (Univ. of California San Diego (US))




Kam Arnold's research focuses on the measurement of the intensity and polarization of the Cosmic Microwave Background (CMB). He is currently working on deploying new instruments to a 17,000 ft Chilean telescope site, and developing technology for a future space mission. Further description of his research can be found at cosmology.ucsd.edu.

Javier Duarte is inviting you to a scheduled Zoom meeting.

Topic: Physics 191
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