I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations
of galaxy formation performed with the arepo code and updated models for feedback …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …

We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …

We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …

We present a robust method to constrain average galaxy star formation rates (SFRs), star
formation histories (SFHs), and the intracluster light (ICL) as a function of halo mass. Our …

We present a new comprehensive model of the physics of galaxy formation designed for
large-scale hydrodynamical simulations of structure formation using the moving-mesh code …

We present measurements of the stellar mass functions (SMFs) of star-forming and
quiescent galaxies to z= 4 using a sample of 95,675 K s-selected galaxies in the …

The evolution of the number density of galaxies in the universe, and thus also the total
number of galaxies, is a fundamental question with implications for a host of astrophysical …