Showing 1–20 of 20 results
/ Date/ Name
Feb 1, 2022Higher-order initial conditions with massive neutrinosMar 9, 2020Setting the Stage: Structures from Gaussian Random FieldsMar 31, 2017The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxiesJul 13, 2015The APOSTLE project: Local Group kinematic mass constraints and simulation candidate selectionJul 8, 2015The COpernicus COmplexio: Statistical Properties of Warm Dark Matter HaloesMay 24, 2015The Copernicus Complexio: a high-resolution view of the small-scale UniverseDec 8, 2014Local Group galaxies emerge from the darkSep 30, 2014Baryon effects on the internal structure of LCDM halos in the EAGLE simulationsSep 2, 2014Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relationsJul 25, 2014The EAGLE project: Simulating the evolution and assembly of galaxies and their environmentsJun 24, 2014The chosen few: the low mass halos that host faint galaxiesMay 20, 2014Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matterApr 14, 2014Bent by baryons: the low mass galaxy-halo relationJun 25, 2013A new way of setting the phases for cosmological multi-scale Gaussian initial conditionsJun 24, 2013Panphasia: a user guideSep 13, 2012Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark MatterOct 29, 2010A Halo Expansion (HEX) Technique for Approximating Simulated Dark Matter HaloesOct 1, 2009Second-order Lagrangian perturbation theory initial conditions for resimulationsMar 18, 2009Resolving Cosmic Structure Formation with the Millennium-II SimulationOct 19, 2006The baryon fraction of LambdaCDM haloes