Tom Theuns

TL;DR: The Virgo Consortium's EAGLE project as discussed by the authors is a suite of hydrodynamical simulations that follow the formation of galaxies and black holes in representative volumes, where thermal energy is injected into the gas, allowing winds to develop without predetermined speed or mass loading factors.

TL;DR: Observations of a quasar at a redshift of 7.3 are reported, suggesting that the neutral fraction of the intergalactic medium in front of ULAS J1120+0641 exceeded 0.1.

TL;DR: In this article, the authors present results from thirteen cosmological simulations that explore the parameter space of the "Evolution and Assembly of GaLaxies and their Environments" (EAGLE) simulation project.

TL;DR: In this paper, the authors investigate the physics driving the cosmic star formation history using the more than 50 large, cosmological, hydrodynamical simulations that together comprise the OverWhelmingly Large Simulations project.

TL;DR: In this paper, the authors performed cosmological hydrodynamic simulations to determine to what extent galaxies lose their gas due to photoheating from an ionizing background, and they found that the characteristic mass at which haloes on average have lost half of their baryons is M c ∼ 6.5 x 10 9 h -1 M ⊙ at z = 0, which corresponds to a circular velocity of 25 km s -1.