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Development of the 220/270 GHz Receiver of BICEP Array

By Bicep/keck Collaboration and others at
LogoStanford University
and
LogoCardiff University
Measurements of B-mode polarization in the CMB sourced from primordial gravitational waves would provide information on the energy scale of inflation and its potential form. To achieve these goals, one must carefully characterize the Galactic foregrounds, which can be distinguished from the CMB by conducting measurements at multiple frequencies. BICEP... Show more
September 3, 2024
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Development of the 220/270 GHz Receiver of BICEP Array
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