Searches for the galaxies associated with low-metallicity circumgalactic clouds reveal one population of clouds associated with galactic halos and another population that appears to be more distant from detectable galaxies

Using synthetic spectroscopy to gain insight into the phase and kinematics of multiphase CGM gas

A joint approach combining observations and simulations helps to distinguish inflowing filaments from outflowing clumps

Accretion mode may determine galaxy morphology.

A novel analytic model for a galactic wind peppered with embedded cold clouds

Understanding the CGM in the context of large scale environment

A demonstration of Enhanced Halo Resolution