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The infall of dwarf satellite galaxies are influenced by their host’s massive accretions
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Modelling the orbital histories of satellites of Milky Way-mass galaxies: testing static host potentials against cosmological simulations
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On the segregation of dark matter substructure
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emerge – an empirical model for the formation of galaxies since z ∼ 10
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A profile in FIRE: resolving the radial distributions of satellite galaxies in the Local Group with simulations
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Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
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ELVES II: Globular Clusters and Nuclear Star Clusters of Dwarf Galaxies: the Importance of Environment
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Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set
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ELVES. III. Environmental Quenching by Milky Way–mass Hosts
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Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way
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NeutralUniverseMachine: An Empirical Model for the Evolution of H i and H2 Gas in the Universe
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ELVES. IV. The Satellite Stellar-to-halo Mass Relation Beyond the Milky Way
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Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
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Microgalaxies in LCDM
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symfind : Addressing the Fragility of Subhalo Finders and Revealing the Durability of Subhalos
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Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia–Sausage–Enceladus Analogs
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The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way–mass Galaxies
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The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way–mass Galaxies
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Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation
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The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
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Atomic Gas Scaling Relations of Star-forming Galaxies at z ≈ 1
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A Self-interacting Dark Matter Solution to the Extreme Diversity of Low-mass Halo Properties
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