We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

We use the age–metallicity distribution of 96 Galactic globular clusters (GCs) to infer the
formation and assembly history of the Milky Way (MW), culminating in the reconstruction of …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

We present the extended GALEX Arecibo SDSS Survey (xGASS), a gas fraction-limited
census of the atomic hydrogen (H i) gas content of 1179 galaxies selected only by stellar …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

The coevolution of galaxies and their metal content serves as an important test for galaxy
feedback models. We analyse the distribution and evolution of metals within the IllustrisTNG …

Abstract We introduce the MOdelling Star cluster population Assembly In Cosmological
Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models …

We introduce the Cluster-EAGLE (c-eagle) simulation project, a set of cosmological
hydrodynamical zoom simulations of the formation of 30 galaxy clusters in the mass range of …

Current and upcoming radio telescopes will map the spatial distribution of cosmic neutral
hydrogen (H i) through its 21 cm emission. In order to extract the maximum information from …