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 …
JM Helton, F Sun, C Woodrum… - The Astrophysical …, 2024 - iopscience.iop.org
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 …
E Kukstas, ML Balogh, IG McCarthy… - Monthly Notices of …, 2023 - academic.oup.com
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 …
S Tacchella, C Conroy, SM Faber… - The Astrophysical …, 2022 - iopscience.iop.org
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 …