Showing 21–40 of 40 results
/ Date/ Name
May 12, 2020The globular cluster system mass-halo mass relation in the E-MOSAICS simulationsMay 11, 2020Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulationsJun 28, 2017Constraining cosmology with the velocity function of low-mass galaxiesJun 6, 2024Spherinator and HiPSter: Representation Learning for Unbiased Knowledge Discovery from SimulationsJul 14, 2022Monochromatic globular clusters as a critical test of formation models for the dark matter deficient galaxies NGC1052-DF2 and NGC1052-DF4Oct 2, 2022Globular cluster metallicity distributions in the E-MOSAICS simulationsNov 29, 2021NGC5846-UDG1: A galaxy formed mostly by star formation in massive, extremely dense clumps of gasFeb 28, 2020Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulationsNov 5, 2012The Self-Similarity of the Circumgalactic Medium with Galaxy Virial Mass: Implications for Cold-Mode AccretionDec 21, 2025EuroHPC SPACE CoE: Redesigning Scalable Parallel Astrophysical Codes for ExascaleJan 20, 2021What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxiesJun 14, 2021Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulationsJul 5, 2023On the origin of globular clusters in a hierarchical UniverseOct 2, 2023HI discs of L$_{\ast}$ galaxies as probes of the baryonic physics of galaxy evolutionMay 3, 2012Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 GalaxyJun 9, 2014Halo Mass Dependence of HI and OVI Absorption: Evidence for Differential KinematicsSep 2, 2014Direct Insights into Observational Absorption Line Analysis Methods of the Circumgalactic Medium Using Cosmological SimulationsJun 2, 2015An Extreme Metallicity, Large-Scale Outflow from a Star-Forming Galaxy at z ~ 0.4Nov 28, 2016Hints against the cold and collisionless nature of dark matter from the galaxy velocity functionMay 7, 2025Machine Learning Workflow for Morphological Classification of Galaxies