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 study of galaxy protoclusters is beginning to fill in unknown details of the important
phase of the assembly of clusters and cluster galaxies. This review describes the current …

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

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 …

The spectra of high-redshift (z≳ 6) quasars contain valuable information on the progression
of the Epoch of Reionization. At redshifts z< 6, the observed Lyman-series forest shows that …

We present a new flexible Bayesian framework for directly inferring the fraction of neutral
hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR, z∼ 6 …

We investigate constraints on cosmic reionization extracted from the Planck cosmic
microwave background (CMB) data. We combine the Planck CMB anisotropy data in …

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

We present the grackle chemistry and cooling library for astrophysical simulations and
models. grackle provides a treatment of non-equilibrium primordial chemistry and cooling for …

Abstract Recently, the Hydrogen Epoch of Reionization Array (HERA) has produced the
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …