ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies (S 4 G) is a deep 3.6 and 4.5
μm imaging survey of 2352 nearby (< 40 Mpc) galaxies. We describe the S 4 G data analysis …

In Paper I of this series we introduced a volume-limited parent sample of 871 galaxies from
which we extracted the ATLAS3D sample of 260 early-type galaxies (ETGs). In Papers II and …

We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled
independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey …

We analyse the relationships between galaxy morphology, colour, environment and stellar
mass using data for over 105 objects from Galaxy Zoo, the largest sample of visually …

Gravitational lensing by clusters of galaxies offers a powerful probe of their structure and
mass distribution. Several research groups have developed techniques independently to …

In this paper, we investigate environment-driven gas depletion in satellite galaxies, taking
full advantage of the atomic hydrogen (H i) spectral stacking technique to quantify the gas …

We use HST/WFC3 imaging from the CANDELS Multi-Cycle Treasury Survey, in conjunction
with the Sloan Digital Sky Survey, to explore the evolution of galactic structure for galaxies …

It has long been regarded as difficult if not impossible for a cosmological model to account
simultaneously for the galaxy luminosity, mass, and velocity distributions. We revisit this …

We measure the mass functions for generically red and blue galaxies, using az< 0.12
sample of log M*> 8.7 field galaxies from the Galaxy And Mass Assembly (GAMA) survey …

We analyse the environmental dependence of galaxy morphology and colour with two-point
clustering statistics, using data from the Galaxy Zoo, the largest sample of visually classified …