Sanders, J. S. High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;
Walker, S. A., Sanders, J. S., & Fabian, A. C. (2018). What fraction of the density fluctuations in the Perseus cluster core is due to gas sloshing rather than AGN feedback? Monthly Notices of the Royal Astronomical Society, 481(2), 1718-1725. doi:10.1093/mnras/sty2390.