Contrary to many stereotypes about massive galaxies, observed brightest group galaxies
(BGGs) are diverse in their star formation rates, kinematic properties, and morphologies …

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

As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

We introduce the new TNG-Cluster project, an addition to the IllustrisTNG suite of
cosmological magnetohydrodynamical simulations of galaxy formation. Our objective is to …

Context. Previous studies have revealed that the estimated probability of galaxy-galaxy
strong lensing in observed galaxy clusters exceeds the expectations from the Λ cold dark …

We investigate the formation of brightest cluster galaxies (BCGs) in the TNG300
cosmological simulation of the IllustrisTNG project. Our cluster sample consists of 700 …

We introduce a new chemical enrichment and stellar feedback model into GIZMO, using the
SIMBA sub-grid models as a base. Based on the state-of-the-art chemical evolution model of …

We use a set of about 300 simulated clusters from the three hundred Project to calculate
their hydrostatic masses and evaluate the associated bias by comparing them with the true …

The distribution of baryons provides a significant way to understand the formation of galaxy
clusters by revealing the details of its internal structure and changes over time. In this paper …

Widefield surveys probe clustered scalar fields–such as galaxy counts, lensing potential, etc.–
which are sensitive to different cosmological and astrophysical processes. Constraining …