Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …

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 present a model for the evolution of the galaxy ultraviolet (UV) luminosity function (LF)
across cosmic time where star formation is linked to the assembly of dark matter halos under …

We study star cluster formation in a low-metallicity environment using three-dimensional
hydrodynamic simulations. Starting from a turbulent cloud core, we follow the formation and …

In recent years, the discovery of massive quasars at has provided a striking challenge to our
understanding of the origin and growth of supermassive black holes in the early Universe …

ABSTRACT The James Webb Space Telescope (JWST) is expected to observe galaxies at
z> 10 that are presently inaccessible. Here, we use a self-consistent empirical model, the …

Reionization in the early Universe is likely driven by dwarf galaxies. Using cosmological
radiation-hydrodynamic simulations, we study star formation and the escape of Lyman …

We study star cluster formation at low metallicities of Z/Z⊙= 10− 4–10− 1 using three-
dimensional hydrodynamics simulations. Particular emphasis is put on how the stellar mass …

The detection of quasars at z> 6 unveils the presence of supermassive black holes of a few
billion solar masses. The rapid formation process of these extreme objects remains a …

ABSTRACT We implemented Population III (Pop. III) star formation in mini-haloes within the
Meraxes semi-analytic galaxy formation and reionization model, run on top of a N-body …