Welcome to my website.  I am currently an Alvin Nashman Postdoctoral Fellow at Carnegie Observatories.  I use hydrodynamical (or magnetohydrodynamical) numerical simulations to study galaxy evolution across a range of environments.  This includes large-scale cosmological simulations so I can compare void to cluster galaxies and galaxy-scale idealized simulations to study how ram pressure stripping affects galaxy properties and the surrounding intracluster medium.


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