Developing Environments: Formation and Quenching at Cosmic Noon Traced by the Large-scale Distribution of Gas and Galaxies
Environmental density correlates with galaxy properties in the local Universe, but how and when these trends emerge is unclear: at cosmic noon, large-scale structures are still assembling and galaxies quench rapidly for debated reasons. We study how the formation and quenching histories of massive galaxies at 1.7$<$z$<...