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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.

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Local Group galaxies emerge from the dark, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1412.2748Comment: 14 pages, 4 figures.Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an additional 32 pages of supplementary figures and data tables are available from http://astro.dur.ac.uk/~ams/MUSEcubes/.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.The EAGLE project: Simulating the evolution and assembly of galaxies and their environments, , , , , , , , , and 12 other author(s). (2014)cite arxiv:1407.7040Comment: Submitted to MNRAS. For images and videos, see http://eagle.strw.leidenuniv.nl/ and http://icc.dur.ac.uk/Eagle/.Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3, , , , , , , , , and 5 other author(s). (2019)cite arxiv:1904.07254Comment: Submitted to MNRAS. 23 pages, 15 figures plus appendices.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 origin of the enhanced metallicity of satellite galaxies, , , , , , , and . (2016)cite arxiv:1609.03379Comment: 22 pages, 15 figures; accepted by MNRAS.Introducing STRAUSS: A flexible sonification Python package., and . CoRR, (2023)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.