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The effect of baryons on the inner density profiles of rich clusters, , , , , , , , , and . (2014)cite arxiv:1409.8297Comment: 13 pages, 7 figures, submitted to MNRAS.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulations, , , , , , , , , and . (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.It's not easy being green: The evolution of galaxy colour in the EAGLE simulation, , , , , , and . (2016)cite arxiv:1601.07907Comment: 15 pages, 10 figures. Submitted to MNRAS. All comments welcome. Larger version of Fig. 1 included in source. For the animated evolution of the EAGLE intrinsic u-r CMD (with central and satellite galaxies coloured red and blue respectively) see http://community.dur.ac.uk/j.w.trayford/media/CMD_evolution_EAGLE.mp4.The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end, , , , , , and . (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.SWIFT: task-based hydrodynamics and gravity for cosmological simulations., , , and . CoRR, (2015)A machine learning approach to mapping baryons onto dark matter halos using the EAGLE and C-EAGLE simulations, , , , , , and . (2021)cite arxiv:2106.04980Comment: 15 pages, 13 figures, submitted to MNRAS. Comments welcome!.EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, , , , , , , and . (2022)cite arxiv:2210.09978.A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find., , , and . PARCO, volume 36 of Advances in Parallel Computing, page 263-274. IOS Press, (2019)The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation, , , , , , and . (2015)cite arxiv:1503.05553Comment: 24 pages, 20 figures; submitted to MNRAS.The origin of the $\alpha$-enhancement of massive galaxies, , , , , and . (2016)cite arxiv:1603.05653Comment: 5 pages, 3 figures, submitted to MNRAS Letters.