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Abstract: The Simons Observatory (SO), now in full science operations in Chile, will drive major advances in cosmic microwave background (CMB) science over the next decade. This talk describes the microwave-multiplexed readout that made SO’s roughly 100,000-detector deployment possible, and highlights preliminary SO collaboration results on CMB lensing that preview the observatory’s 10-year survey of large-scale structure.
Host: Laura Newburgh