Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

The environments of galaxy clusters that underwent a recent (≤ 3 Gyr) major merger are
harsher than those of dynamically relaxed clusters due to the global hydrodynamical …

Golovich et al. present an optical imaging and spectroscopic survey of 29 radio relic merging
galaxy clusters. In this paper, we study this survey to identify substructure and quantify the …

We present a study of the orbits, environments, and morphologies of 13 ram-pressure
stripped galaxies in the massive, intermediate redshift (z∼ 0.3− 0.4) galaxy clusters A2744 …

To understand the formation and growth of supermassive black holes (SMBHs) and their
coevolution with host galaxies, it is essential to know the impact of environment on the …

We present initial results from the Subaru Strategic Program (SSP) with Hyper Suprime-Cam
(HSC) on a comprehensive survey of emission-line galaxies at z< 1.5 based on narrowband …

We report CFHT/SITELLE imaging Fourier Transform Spectrograph observations of the
brightest cluster galaxy (BCG) of galaxy cluster Abell 2390 at z= 0.228. The BCG displays a …

We use a complete set of deep narrow-band imaging data for 384 galaxies gathered during
the Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) to derive the first …

Studies of star formation in various galaxy cluster mergers have reached apparently
contradictory conclusions regarding whether mergers stimulate star formation, quench it, or …

We investigate dust-unbiased star formation rates (SFRs) as a function of the environment in
20 massive clusters () between 0.15<< 0.35 using radio luminosities (L 1.4 GHz) from the …