We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …

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 present a variation of the recently updated Munich semi-analytical galaxy formation
model, l-Galaxies, with a new gas stripping method. Extending earlier work, we directly …

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 …

We report the discovery of an extreme galaxy overdensity at z= 5.4 in the GOODS-S field
using James Webb Space Telescope (JWST)/NIRCam imaging from JADES and JEMS …

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 …

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 quantify the relative importance of environmental quenching versus pre-processing in
z∼ 1 clusters by analysing the infalling galaxy population in the outskirts of 15 galaxy …

We use photometric redshifts and statistical background subtraction to measure stellar mass
functions in galaxy group-mass (4.5− 8× 1013 M⊙) haloes at 1< z< 1.5. Groups are selected …

We investigate the stellar populations for a sample of 161 massive, mainly quiescent
galaxies at< z obs>= 0.8 with deep Keck/DEIMOS rest-frame optical spectroscopy (HALO7D …