Predictions from a semi-analytic model confronted with observational data

Hot gaseous halos around galaxies are mainly the realm of theoretical exploration but that will soon change

Emission maps are a crucial next step toward understanding both the baryonic distribution of the universe and the processes that mediate galaxy formation and evolution

UV, X-rays, and radio waves constrain plausible CGM models of an often overlooked type of halo

A use case for the Santa Barbara CGM Model