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 …

Most diffuse baryons, including the circumgalactic medium (CGM) surrounding galaxies and
the intergalactic medium (IGM) in the cosmic web, remain unmeasured and unconstrained …

We quantify the cosmological spread of baryons relative to their initial neighbouring dark
matter distribution using thousands of state-of-the-art simulations from the Cosmology and …

Extracting information from the total matter power spectrum with the precision needed for
upcoming cosmological surveys requires unraveling the complex effects of galaxy formation …

We explore the role of galactic feedback on the low-redshift Lyα (Lyα) forest (z≲ 2) statistics
and its potential to alter the thermal state of the intergalactic medium. Using the Cosmology …

ABSTRACT Sunyaev–Zel'dovich (SZ) measurements can dramatically improve our
understanding of the intergalactic medium and the role of feedback processes in galaxy …

Recent work has pointed out the potential existence of a tight relation between the
cosmological parameter Ω m, at fixed Ω b, and the properties of individual galaxies in state …

Galaxy cluster mass functions are a function of cosmology, but mass is not a direct
observable, and systematic errors abound in all its observable proxies. Mass-free inference …

We present a new suite of over 1500 cosmological N-body simulations with varied warm
dark matter (WDM) models ranging from 2.5 to 30 keV. We use these simulations to train …

We discover analytic equations that can infer the value of Ω m from the positions and velocity
moduli of halo and galaxy catalogs. The equations are derived by combining a tailored …