369 citations · 3k across the 56 of their papers we have counts for
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The cosmic globular cluster formation history in the E-MOSAICS simulations
Philipp S. Joschko, J. M. Diederik Kruijssen, Sebastian Trujillo-Gomez +4
We present a comprehensive analysis of globular cluster (GC) formation and evolution across the Mpc volume of the E-MOSAICS galaxy formation simulations. Defining GCs as…
Comparing E-MOSAICS predictions of high-redshift proto-globular clusters with JWST observations in lensed galaxies
Joel Pfeffer, Duncan A. Forbes, Aaron J. Romanowsky +8
High-resolution imaging and strong gravitational lensing of high-redshift galaxies have enabled the detection of compact sources with properties similar to nearby massive star clus…
The PIPER Survey. II. The Globular Cluster Systems of Low Surface Brightness Galaxies in the Perseus Cluster
Steven R. Janssens, Duncan A. Forbes, Aaron J. Romanowsky +7
We present Hubble Space Telescope ACS/WFC and WFC3/UVIS imaging for a sample of 50 low surface brightness (LSB) galaxies in the 10 M Perseus cluster, which w…
The formation and disruption of globular cluster populations in simulations of present-day galaxies with controlled assembly histories
Oliver Newton, Jonathan J. Davies, Joel Pfeffer +4
Globular clusters (GCs) are sensitive tracers of galaxy assembly histories but interpreting the information they encode is challenging because mergers are thought to promote both t…
Origin of the correlation between stellar kinematics and globular cluster system richness in ultra-diffuse galaxies
Joel Pfeffer, Steven R. Janssens, Maria Luisa Buzzo +9
Observational surveys have found that the dynamical masses of ultra-diffuse galaxies (UDGs) correlate with the richness of their globular cluster (GC) system. This could be explain…
Constraining the stellar populations of ultra-diffuse galaxies in the MATLAS survey using spectral energy distribution fitting
Maria Luisa Buzzo, Duncan A. Forbes, Thomas H. Jarrett +12
We use spectral energy distribution (SED) fitting to place constraints on the stellar populations of 59 ultra-diffuse galaxies (UDGs) in the low-to-moderate density fields of the M…