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Setting the Stage: Structures from Gaussian Random Fields

, , , , , , and . (2020)cite arxiv:2003.04321Comment: 18 pages, 22 figures, submitted to MNRAS.

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The Hydrangea simulations: galaxy formation in and around massive clusters, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.The statistics of Λ CDM halo concentrations, , , , , , , , and . Monthly Notices of the Royal Astronomical Society, 381 (4): 1450--1462 (November 2007)Bent by baryons: the low mass galaxy-halo relation, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1404.3724Comment: 8 pages, submitted to MNRAS, comments welcome.Local Group galaxies emerge from the dark, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1412.2748Comment: 14 pages, 4 figures.Cosmic cookery: making a stereoscopic 3D animated movie, , , , , , , , and . 6055, page 605505--605505-12. (2006)The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1703.10907Comment: 20 pages, 15 figures, submitted to MNRAS.Indra: a Public Computationally-Accessible Suite of Cosmological $N$-body Simulations, , , , , , and . (2021)cite arxiv:2101.03631Comment: Submitted to MNRAS. Indra is available on SciServer at http://sciserver.org.Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way, , , , , , , and . (2020)cite arxiv:2011.08865Comment: 21 pages (JCAP format), 3 appendices, 10 figures, 1 table. Comments welcome.Universality in the structure of dark matter haloes over twenty orders of magnitude in halo mass, , , , , , and . (2019)cite arxiv:1911.09720Comment: 35 pages, 8 figures, submitted.Setting the Stage: Structures from Gaussian Random Fields, , , , , , and . (2020)cite arxiv:2003.04321Comment: 18 pages, 22 figures, submitted to MNRAS.