This blog is a space¬†for me to polish off ideas and make code public. I’ll try to fill it with useful content related to data¬†science projects, astrophysics, my job search, and programming. For now, here’s a density-weighted projection of the gas in one of my simulated galaxies a few hundred million years after the big bang:

]1 The simulated gas around a young galaxy (circled), 750 million years after the big bang. The filamentary gas structure and violent fragmentation are prominent features of simulations at this epoch.