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 …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11
galaxy clusters at 1.0< z< 1.4 drawn from the Gemini Observations of Galaxies in Rich Early …

The miniJPAS survey has observed∼ 1 deg 2 of the AEGIS field with 60 bands (spectral
resolution of R∼ 60) in order to demonstrate the scientific potential of the Javalambre …

We study the star formation histories (SFHs) and mass-weighted ages of 331 UVJ-selected
quiescent galaxies in 11 galaxy clusters and in the field at 1< z< 1.5 from the Gemini …

At redshifts of z≲ 1.3, early-type galaxies (ETGs) and passive galaxies are mainly found in
dense environments, such as galaxy clusters. However, it remains unclear whether these …

We present results on the environmental dependence of the star-forming galaxy main
sequence in 11 galaxy cluster fields at 1.0< z< 1.5 from the Gemini Observations of Galaxies …

We measure the rate of environmentally driven star formation quenching in galaxies at z∼ 1,
using eleven massive () galaxy clusters spanning a redshift range 1.0< z< 1.4 from the …

Recent observations have shown that the environmental quenching of galaxies at z∼ 1 is
qualitatively different to that in the local Universe. However, the physical origin of these …

We model satellite quenching at z∼ 1 by combining 14 massive (1013.8< M halo/M⊙<
1015) clusters at 0.8< z< 1.3 from the GOGREEN and GCLASS surveys with accretion …