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 …

Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …

Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …

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 …

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 …

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 …

Context. The processes responsible for galaxy evolution in different environments as a
function of galaxy mass remain heavily debated. Rich galaxy clusters are ideal laboratories …

We present Hubble multi-wavelength photometric catalogs, including (up to) 17 filters with
the Advanced Camera for Surveys and Wide Field Camera 3 from the ultra-violet to near …

Using a sample of four galaxy clusters at 1.35< z< 1.65 and 10 galaxy clusters at 0.85< z<
1.35, we measure the environmental quenching timescale, t Q, corresponding to the time …