Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

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 …

The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

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 …

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 …

Much of our knowledge of galaxies comes from analysing the radiation emitted by their stars,
which depends on the present number of each type of star in the galaxy. The present …

The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analog of
large star-formation events in the distant universe. We determined the recent formation …

We use the energy-balance code magphys to determine stellar and dust masses, and dust
corrected star formation rates for over 200 000 GAMA galaxies, 170 000 G10-COSMOS …

The era of the James Webb Space Telescope ushers stellar population models into
uncharted territories, particularly at the high-redshift frontier. In a companion paper, we apply …