154 citations · 2k across the 43 of their papers we have counts for
10 papers · 1 filter
Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
Gandhali D. Joshi, Laura C. Parker, James Wadsley
We investigate mass segregation in group and cluster environments by identifying galaxy analogues in high-resolution dark matter simulations. Subhalos identified by the AHF and ROC…
Do group dynamics play a role in the evolution of member galaxies?
Annie Hou, Laura C. Parker, Michael L. Balogh +8
We examine galaxy groups from the present epoch to z = 1 to explore the impact of group dynamics on galaxy evolution. We use group catalagues from the Sloan Digital Sky Survey (SDS…
Efficient satellite quenching at z~1 from the GEEC2 spectroscopic survey of galaxy groups
Angus Mok, Michael L. Balogh, Sean L. McGee +9
We present deep GMOS-S spectroscopy for 11 galaxy groups at 0.8<z<1.0, for galaxies with r_{AB}<24.75. Our sample is highly complete (>66%) for eight of the eleven groups. Using an…
Exploring the Diversity of Groups at 0.1<z<0.8 with X-ray and Optically Selected Samples
Jennifer L. Connelly, David J. Wilman, Alexis Finoguenov +8
We present the global group properties of two samples of galaxy groups containing 39 high quality X-ray selected systems and 38 optically (spectroscopically) selected systems in co…
Substructure in the Most Massive GEEC Groups: Field-like Populations in Dynamically Active Groups
Annie Hou, Laura C. Parker, David J. Wilman +6
The presence of substructure in galaxy groups and clusters is believed to be a sign of recent galaxy accretion and can be used not only to probe the assembly history of these struc…
The Nature of Star Formation at 24 microns in the Group Environment at 0.3 < z < 0.55
K. Tyler, G. H. Rieke, D. J. Wilman +7
Galaxy star formation rates (SFRs) are sensitive to the local environment; for example, the high-density regions at the cores of dense clusters are known to suppress star formation…