Satellite galaxies in groups and clusters are more likely to have low star formation rates
(SFRs) and lie on the 'red sequence'than central ('field') galaxies. Using galaxy group/cluster …

Exploiting the data from the GAs Stripping Phenomena in galaxies with MUSE (GASP)
program, we compare the integrated star formation rate–mass relation (SFR–M*) relation of …

The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a
telescope under development by a consortium of 17 countries. The SKA will be 50 times …

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 …

We investigate the effect of ram-pressure from the intracluster medium on the stripping of H i
gas in galaxies in a massive, relaxed, X-ray bright, galaxy cluster at z= 0.2 from the Blind …

We describe and discuss the selection procedure and statistical properties of the galaxy
sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy …

We use publicly available galaxy merger trees, obtained applying semi-analytic techniques
to a large high-resolution cosmological simulation, to study the environmental history of …

In the local Universe, galaxies in groups and clusters contain less gas and are less likely to
be forming stars than their field counterparts. This effect is not limited to the central …

We use the galaxy stellar mass and halo merger tree information from the semi-analytic
model galaxy catalogue of Font et al. to examine the accretion of galaxies into a large …

Galaxies that are being stripped of their gas can sometimes be recognized from their optical
appearance. Extreme examples of stripped galaxies are the so-called" jellyfish galaxies" that …