Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

Galactic winds shape the stellar, gas, and metal content of galaxies. To quantify their impact,
we must understand their physics. We review potential wind-driving mechanisms and …

We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

We introduce the public version of the cosmological magnetohydrodynamical moving-mesh
simulation code A repo. This version contains a finite-volume magnetohydrodynamics …

The early release science results from JWST have yielded an unexpected abundance of
high-redshift luminous galaxies that seems to be in tension with current theories of galaxy …

We present new determinations of the rest-UV luminosity functions (LFs) at z= 2–9 to
extremely low luminosities (>− 14 mag) from a sample of> 2500 lensed galaxies found …

The star formation rate (SFR) in galactic disks depends on both the quantity of the available
interstellar medium (ISM) gas and its physical state. Conversely, the ISM's physical state …

The high-redshift intergalactic medium (IGM) and the primeval galaxy population are rapidly
becoming the new frontier of extragalactic astronomy. We investigate the IGM properties and …

ABSTRACT We present STARFORGE (STAR FORmation in Gaseous Environments): a new
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …

The visibility of high-redshift Lyman-alpha emitting galaxies (LAEs) provides important
constraints on galaxy formation processes and the Epoch of Reionization (EoR). However …