Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …

We describe and test an updated version of radiation-hydrodynamics in the ramses code,
that includes three new features:(i) radiation pressure on gas,(ii) accurate treatment of …

The ultraviolet background (UVB) emitted by quasars and galaxies governs the ionization
and thermal state of the intergalactic medium (IGM), regulates the formation of high-redshift …

We introduce meraxes, a new, purpose-built semi-analytic galaxy formation model designed
for studying galaxy growth during reionization. meraxes is the first model of its type to …

Understanding the escape of Lyman continuum (LyC) and Lyα photons from giant molecular
clouds (GMCs) is crucial if we are to study the reionization of the universe and to interpret …

ABSTRACT SCORCH (Simulations and Constructions of the Reionization of Cosmic
Hydrogen) is a new project to study the Epoch of Reionization (EoR). In this first paper, we …

Abstract The Abundance Matching Box for the Epoch of Reionization (AMBER) is a semi-
numerical code for modeling the cosmic dawn. The new algorithm is not based on the …

We introduce a new suite of radiation-hydrodynamical simulations of galaxy formation and
reionization called Aurora. The Aurora simulations make use of a spatially adaptive radiative …

We present simulations of cosmic reionization and reheating from z= 18 to z= 5,
investigating the role of stars (emitting soft UV-photons), nuclear black holes (BHs, with …

In this work we present a new hybrid method to simulate the thermal effects of reionization in
cosmological hydrodynamical simulations. The method improves upon the standard …