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Revision as of 13:01, 29 July 2020

Astrophysics of High-Redshift Galaxies and Clusters Lindsey Bleem and Anthony Gonzalez

CMB-S4 will detect high redshift dusty galaxies out to z~9; protoclusters out to z~5 ; and massive galaxy clusters out to z~2. In this session we will discuss how CMB-S4 can shed light on the evolution from high-redshift dusty galaxies to protoclusters to galaxy clusters and highlight the insights and advances that studies of these discrete objects will bring to the field of astrophysics.