Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

The co-evolution between supermassive black holes and their environment is most directly
traced by the hot atmospheres of dark matter halos. The cooling of the hot atmosphere …

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 an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …

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 …

We present a new statistical method to determine the relationship between the stellar
masses of galaxies and the masses of their host dark matter haloes over the entire cosmic …

The ATLAS3D project is a multiwavelength survey combined with a theoretical modelling
effort. The observations span from the radio to the millimetre and optical, and provide …

Black hole (BH) mergers detectable with the Laser Interferometer Gravitational-wave
Observatory (LIGO) can occur in active galactic nucleus (AGN) disks. Here we parameterize …

This paper describes the first catalogue of photometrically derived stellar mass estimates for
intermediate-redshift (z< 0.65; median z= 0.2) galaxies in the Galaxy And Mass Assembly …