Mark Vogelsberger

TL;DR: The Illustris Project as mentioned in this paper is a series of large-scale hydrodynamical simulations of galaxy formation, which includes primordial and metal-line cooling with self-shielding corrections, stellar evolution, stellar feedback, gas recycling, chemical enrichment, supermassive black hole growth, and feedback from active galactic nuclei.

TL;DR: In this article, the authors performed the largest ever particle simulation of a Milky Way sized dark matter halo, and presented the most comprehensive convergence study for an individual dark mass halo carried out thus far.

TL;DR: In this paper, the authors performed the largest ever particle simulation of a Milky Way-sized dark matter halo, and presented the most comprehensive convergence study for an individual dark matter Halo carried out thus far.

TL;DR: A simulation that starts 12 million years after the Big Bang, and traces 13 billion years of cosmic evolution with 12 billion resolution elements in a cube of 106.5 megaparsecs a side yields a reasonable population of ellipticals and spirals, reproduces the observed distribution of galaxies in clusters and characteristics of hydrogen on large scales, and at the same time matches the ‘metal’ and hydrogen content of galaxies on small scales.

TL;DR: In this article, an updated physical model to simulate the formation and evolution of galaxies in cosmological, large-scale gravity+magnetohydrodynamical simulations with the moving mesh code AREPO is introduced.