We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …

The distribution of chemical elements in the hot intracluster medium (ICM) retains valuable
information about the enrichment and star formation histories of galaxy clusters, and on the …

We present cosmological hydrodynamical simulations of galaxy clusters aimed at studying
the process of metal enrichment of the intra-cluster medium (ICM). These simulations have …

We present results from the semi-analytic model of galaxy formation sagapplied on the
MultiDark simulation MDPL2. sag features an updated supernova (SN) feedback scheme …

Context. Observationally, the quenching of star-forming galaxies appears to depend both on
their mass and environment. The exact cause of the environmental dependence is still …

We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution
of galaxies by using a combination of a cosmological N-body simulation of the concordance …

The success of H i intensity mapping is largely dependent on how well 21-cm foreground
contamination can be controlled. In order to progress our understanding further, we present …

In this study, we modify the semi-analytic model galacticus in order to accurately reproduce
the observed properties of dwarf galaxies in the Milky Way. We find that reproducing …

We investigate the consequences of applying different star formation laws in the galaxy
formation model galform. Three broad star formation laws are implemented: the empirical …

In this work, we combine the semi-analytic model of galaxy formation and evolution sag with
the 102 relaxed simulated galaxy clusters from the three hundred project, and we study the …