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

Weak galaxy lensing surveys have consistently reported a lower amplitude for the matter
fluctuation spectrum, as measured by the S 8 parameter, than expected in the ΛCDM …

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

We present the first analysis of cosmic shear measured in DES Y3 that employs the entire
range of angular scales in the data. To achieve this, we built upon recent advances in the …

The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. is a …

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 …

Upcoming large-scale structure surveys will measure the matter power spectrum to
approximately per cent level accuracy with the aim of searching for evidence for new physics …

We use the small scales of the Dark Energy Survey (DES) Year-3 cosmic shear
measurements, which are excluded from the DES Year-3 cosmological analysis, to constrain …

We present a full forward-modeled w CDM analysis of the KiDS-1000 weak lensing maps
using graph-convolutional neural networks (GCNN). Utilizing the cosmogrid, a novel …

Feedback from active galactic nuclei and stellar processes changes the matter distribution
on small scales, leading to significant systematic uncertainty in weak lensing constraints on …