Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

We review the current theory of how galaxies form within the cosmological framework
provided by the cold dark matter paradigm for structure formation. Beginning with the pre …

We present the public data release of halo and galaxy catalogues extracted from the eagle
suite of cosmological hydrodynamical simulations of galaxy formation. These simulations …

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 …

We use the Illustris simulation to study the relative contributions of in situ star formation and
stellar accretion to the build-up of galaxies over an unprecedentedly wide range of masses …

We demonstrate a novel technology that combines the power of the multi-object
spectrograph with the spatial multiplex advantage of an integral field spectrograph (IFS). The …

We explore the connection between the UV luminosity functions (LFs) of high-z galaxies and
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …

We present a new algorithm for generating merger trees and halo catalogs which explicitly
ensures consistency of halo properties (mass, position, and velocity) across time steps. Our …

We measure the mass function of dark matter halos in a large set of collisionless
cosmological simulations of flat ΛCDM cosmology and investigate its evolution at z\lesssim …

Using a high-resolution hydrodynamical cosmological simulation of the formation of a
massive spheroidal galaxy we show that elliptical galaxies can be very compact and …