UCSD

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

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

US/Pacific
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Description

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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