340 citations · 5.8k across the 108 of their papers we have counts for
108 papers
Insights into environmental quenching at : an enhancement of faint, low-mass passive galaxies in clusters
Harry Gully, Nina Hatch, Syeda Lammim Ahad +11
Understanding the processes that transform star-forming galaxies into quiescent ones is key to unraveling the role of environment in galaxy evolution. We present measurements of th…
Resolved UV and optical color gradients reveal environmental influence on galaxy evolution at redshift z1.6
William J. Cramer, A. G. Noble, G. Rudnick +13
The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth…
The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
Adit H. Edward, Michael L. Balogh, Yannick M. Bahe +21
We present an analysis of the galaxy stellar mass function (SMF) of 14 known protoclusters between in the COSMOS field, down to a mass limit of M$_{\odot…
The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
Caleb Gatica, Ricardo Demarco, Hervé Dole +4
A complete understanding of the mass assembly history of structures in the universe requires the study of the growth of galaxies and their supermassive black holes (SMBHs) as a fun…
Roman-Cosmic Noon: A Legacy Spectroscopic Survey of Massive Field and Protocluster Galaxies at
Gregory Rudnick, Yannick Bahé, Michael Balogh +10
Protoclusters are the densest regions in the distant universe () and are the progenitors of massive galaxy clusters () in the local universe. Th…
When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmath
Devontae C. Baxter, Michael C. Cooper, Michael L. Balogh +11
We explore models of massive () satellite quenching in massive clusters at using an MCMC framework, focusing on two primary parameters: $R_…