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 …

We present an extended suite of the Auriga cosmological gravo-magnetohydrodynamical
'zoom-in'simulations of 40 Milky Way-mass haloes and 26 dwarf galaxy–mass haloes run …

At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …

This is a golden age for galaxy formation: Existing and especially new telescopes are
providing observations that challenge and illuminate rapidly improving theory and …

We present a detailed study of the cosmic star formation history over 90 per cent of cosmic
time (0≲ z≲ 4), using deep, radio continuum observations that probe star formation activity …

The recent launch of JWST has ushered in a new era of high-redshift astronomy by
providing detailed insights into the gas and stellar populations of galaxies in the epoch of …

Observations of local star-forming galaxies (SFGs) show a tight correlation between their
singly ionized carbon line luminosity () and star formation rate (SFR), suggesting that may be …

The feedback loop between the galaxies producing the background radiation field for
reionization and their growth is crucial, particularly for low-mass haloes. Despite this, the …

Arkenstone is a new model for multiphase, stellar feedback-driven galactic winds designed
for inclusion in coarse resolution cosmological simulations. In this first paper of a series, we …

Cosmological simulations serve as invaluable tools for understanding the Universe.
However, the technical complexity and substantial computational resources required to …