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 …

ABSTRACT We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …

Radio jets and the lobes they inflate are common in cool-core clusters and are known to play
a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is …

We study the formation of the first galaxies in overdense regions modelled by the
FORmation and EVolution of galaxies in Extremely overdense Regions motivated by SSA22 …

To fully take advantage of the data provided by large-scale structure surveys, we need to
quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei …

We study weak gravitational lensing convergence maps produced from the MillenniumTNG
simulations by direct projection of the mass distribution on the past backwards lightcone of a …

For decades, the boundary of cosmic filaments has been a subject of debate. In this work,
we determine the physically motivated radii of filaments by constructing stacked galaxy …

We perform a structural decomposition of galaxies identified in three cosmological
hydrodynamical simulations by applying Gaussian mixture models (GMMs) to the kinematics …

ABSTRACT JWST has revealed a large population of accreting black holes (BHs) in the
early Universe. Recent work has shown that even after accounting for possible systematic …

It is well established that maximizing the information extracted from upcoming and ongoing
stage-IV weak-lensing surveys requires higher order summary statistics that complement the …