A New Window into the Baryon Cycle at Cosmic Noon with Line Intensity Mapping: Forecasts for auto- and cross-correlations in [CII]-158$\mu$m, HI 21 cm, CO${}_{J+1\to J}$, and H$\alpha$ galaxies

Shubh Agrawal, James E. Aguirre, Justin S. Bracks +24

Across the peak of cosmic star formation at $z\sim 1-2$, inflow, processing, and feedback drive rapid changes in the spatial distribution and chemical composition of baryons in gala…