Cameron Hummels received the PhD degree from Columbia University, New York. He is a National Science Foundation Postdoctoral fellow at Caltech, where he uses computer simulations to model how galaxies form and evolve over the age of the universe. He contributes code to the Enzo hydrodynamics simulation code, the yt visualization and analysis suite, and the Trident synthetic spectral generation tool, and he is a member of the FIRE simulation group, the AGORA simulation group, and the PI of the Tempest simulations.