Major progress has been achieved in recent years in mapping the properties of passively-
evolving, early-type galaxies (ETG) from the local universe all the way to redshift∼ 2. Here …

The epoch of galaxy assembly from 2⩽ z⩽ 4 marks a critical stage during the evolution of
today's galaxy population. During this period, the star-formation activity in the Universe was …

Deriving the expansion history of the Universe is a major goal of modern cosmology. To
date, the most accurate measurements have been obtained with Type Ia Supernovae (SNe) …

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 …

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 …

We present global structural parameter measurements of 109,533 unique, H F160W-
selected objects from the CANDELS multi-cycle treasury program. Sérsic model fits for these …

Using a compilation of 25 studies from the literature, we investigate the evolution of the star-
forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out …

The stellar masses, mean ages, metallicities, and star formation histories of galaxies are
now commonly estimated via stellar population synthesis (SPS) techniques. SPS relies on …

Recent observations of the distant Universe suggest that much of the stellar mass of bright
galaxies was already in place at z> 1. This presents a challenge for models of galaxy …

Distant star-forming galaxies show a correlation between their star formation rates (SFRs)
and stellar masses, and this has deep implications for galaxy formation. Here, we present a …