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 …

We have constructed merger trees for galaxies in the Illustris simulation by directly tracking
the baryonic content of subhaloes. These merger trees are used to calculate the galaxy …

Abstract The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary
spectroscopic surveys of low redshift galaxies. Covering an area of∼ 286 deg2 (split among …

Galaxy mergers are expected to have a significant role in the mass assembly of galaxies in
the early universe, but there are very few observational constraints on the merger history of …

Euclid is a space-based survey mission from the European Space Agency designed to
understand the origin of the Universe's accelerating expansion. It will use cosmological …

We present new determinations of the stellar-to-halo mass relation (SHMR) at z= 0–10 that
match the evolution of the galaxy stellar mass function, the star formation rate (SFR)–M …

Calculating the galaxy merger rate requires both a census of galaxies identified as merger
candidates and a cosmologically averaged" observability" timescale< T obs (z)> for …

Using multiwavelength surveys of active galactic nuclei (AGNs) across a wide range of
bolometric luminosities (10 43< L bol (erg s− 1)< 5× 10 46) and redshifts (0< z< 3), we find a …

The presence of extremely compact galaxies at z∼ 2 and their subsequent growth in
physical size has been the cause of much puzzlement. We revisit the question using deep …

We analyse the mass assembly of central galaxies in the Evolution and Assembly of
Galaxies and their Environments (EAGLE) hydrodynamical simulations. We build merger …