I have been working in large scale structure theory from a wide range of angles, including detailing challenges in using galaxy clusters as cosmological probes, linking dark matter halo histories to observable galaxy properties, using perturbative methods to calculate galaxy and 21 cm correlation functions, and analytic and simulated estimates of bubble properties during reionization. A while back, I also worked a fair amount on validating numerous versions of the DES galaxy catalogues against observations and developed some of these tools for LSST as well, and even earlier than that I also did some strong lensing analyses. Most recently I have been interested characterizations of the cosmic web, its dynamics, and the relation of both to observable galaxy properties, using simulations and analytic approaches.