Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …

The transformation of cold neutral intergalactic hydrogen into a highly ionized warm plasma
marks the end of the cosmic dark ages and the beginning of the age of galaxies. The details …

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

We present morphologies of galaxies at z≳ 9 resolved by JWST/NIRCam 2–5 μm imaging.
Our sample consists of 22 galaxy candidates identified by stringent dropout and photo-z …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

We measure escape fractions, f esc, of ionizing radiation from galaxies in the sphinx suite of
cosmological radiation-hydrodynamical simulations of reionization, resolving haloes with …

We present the results from a new search for candidate galaxies at z≈ 8.5–11 discovered
over the 850 arcmin 2 area probed by the Cosmic Assembly Near-Infrared Deep …

We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy
formation (available at http://flathub. flatironinstitute. org/fire) from the Feedback In Realistic …

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 …

We present the sphinx suite of cosmological adaptive mesh refinement simulations, the first
radiation-hydrodynamical simulations to simultaneously capture large-scale reionization …