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nIFTy galaxy cluster simulations I: dark matter & non-radiative models, , , , , , , , , и 17 other автор(ы). (2015)cite arxiv:1503.06065Comment: 21 pages, 13 figures, 4 tables - submitted to MNRAS.nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes, , , , , , , , , и 10 other автор(ы). (2015)cite arxiv:1511.08255Comment: 17 pages (+4 page appendix), 16 figures, 2 tables; submitted to MNRAS.Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?, , и . (2020)cite arxiv:2011.12974Comment: 18 pages, 15 figures, submitted to MNRAS.Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies, , , , , , и . (2012)cite arxiv:1204.5195Comment: 13 pages, 6 figures, submitted to MNRAS.A Search for Warm/Hot Gas Filaments Between Pairs of SDSS Luminous Red Galaxies, , , , , , , и . (2017)cite arxiv:1709.05024Comment: 10 pages, 9 figures, submitted to MNRAS.The XMM Cluster Survey: The interplay between the brightest cluster galaxy and the intra-cluster medium via AGN feedback, , , , , , , , , и 9 other автор(ы). (2012)cite arxiv:1202.3787Comment: Accepted for publication in MNRAS.Bent by baryons: the low mass galaxy-halo relation, , , , , , , , , и 4 other автор(ы). (2014)cite arxiv:1404.3724Comment: 8 pages, submitted to MNRAS, comments welcome.The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology, , , и . (2016)cite arxiv:1603.02702Comment: 31 pages, 26 figures. Submitted to MNRAS.The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies, , , , , , , , , и 3 other автор(ы). (2017)cite arxiv:1703.10907Comment: 20 pages, 15 figures, submitted to MNRAS.On the road to percent accuracy V: the non-linear power spectrum beyond $Łambda$CDM with massive neutrinos and baryonic feedback, , , , , , , , , и . (2021)cite arxiv:2105.12114Comment: 11 pages, 13 figures. Download ReACT: https://github.com/nebblu/ReACT/tree/react_with_neutrinos.