Black holes: The next generation—repeated mergers in dense star clusters and their gravitational-wave propertiesCarl L. Rodriguez, Claire S. Ye, M. Zevin et al.|Physical review. D/Physical review. D.|2019Cited by 339
Post-Newtonian dynamics in dense star clusters: Formation, masses, and merger rates of highly-eccentric black hole binariesCarl L. Rodriguez, M. Zevin, Pau Amaro‐Seoane et al.|Physical review. D/Physical review. D.|2018Cited by 270
(untitled)Katelyn Breivik, Frederic A. Rasio, Shane L. Larson et al.|Research at the University of Copenhagen (University of Copenhagen)|0Cited by 233
Modeling Dense Star Clusters in the Milky Way and beyond with the Cluster Monte Carlo CodeCarl L. Rodriguez, Frederic A. Rasio, Newlin C. Weatherford et al.|The Astrophysical Journal Supplement Series|2022Cited by 103
Compact Object Modeling in the Globular Cluster 47 TucanaeClaire S. Ye, Frederic A. Rasio, Kyle Kremer et al.|The Astrophysical Journal|2022Cited by 29