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Evolution of the cosmic web
The cosmic web is the largest scale manifestation of the anisotropic gravitational collapse of matter. It represents the transitional stage between linear and non-linear structures and containsExpand
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The total satellite population of the Milky Way.
The total number and luminosity function of the population of dwarf galaxies of the Milky Way (MW) provide important constraints on the nature of the dark matter and on the astrophysics of galaxyExpand
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Tracing the cosmic web
The cosmic web is one of the most striking features of the distribution of galaxies and dark matter on the largest scales in the Universe. It is composed of dense regions packed full of galaxies,Expand
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Milky Way mass constraints from the Galactic satellite gap
We use the distribution of maximum circular velocities, Vmax, of satellites in the Milky Way (MW) to constrain the virial mass, M200, of the Galactic halo under an assumed prior of a Λ cold darkExpand
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Planes of satellite galaxies: when exceptions are the rule
The detection of planar structures within the satellite systems of both the Milky Way (MW) and Andromeda (M31) has been reported as being in stark contradiction to the predictions of the standardExpand
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NEXUS: Tracing the cosmic web connection
We introduce the NEXUS algorithm for the identification of cosmic web environments: clusters, filaments, walls and voids. This is a multiscale and automatic morphological analysis tool thatExpand
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The Copernicus Complexio: a high-resolution view of the small-scale Universe
We introduce Copernicus Complexio (COCO), a high-resolution cosmological N-body simulation of structure formation in the ΛCDM model. COCO follows an approximately spherical region of radius ∼17.4 h−1Expand
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The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web
We investigate the alignment of haloes with the filaments of the cosmic web using an un-precedently large sample of dark matter haloes taken from the P-Millennium Lambda cold dark matter cosmologicalExpand
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The mass of the Milky Way from satellite dynamics
We present and apply a method to infer the mass of the Milky Way (MW) by comparing the dynamics of MW satellites to those of model satellites in the EAGLE cosmological hydrodynamics simulations. A Expand
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Subhalo statistics of galactic haloes: beyond the resolution limit
We study the substructure population of Milky Way (MW)-mass haloes in the Λ cold dark matter (ΛCDM) cosmology using a novel procedure to extrapolate subhalo number statistics beyond the resolutionExpand
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