Dark-ages, Reionization And Galaxy-formation Observables Numerical Simulation


Meraxes is a brand new semi-analytic galaxy formation model, specially designed for studying galaxy formation during the Epoch of Reionisation. Meraxes includes a fully temporally and spatially coupled treatment of reionisation and is built upon the Tiamat N-body simulations which possesses both sufficient volume and mass resolution to study reionisation structure as well as the temporal resolution needed to resolve the galaxy and star formation physics relevant to early galaxy formation.