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The EAGLE project: Simulating the evolution and assembly of galaxies and their environments

J. Schaye, R. Crain, R. Bower, M. Furlong, M. Schaller, T. Theuns, C. Vecchia, C. Frenk, I. McCarthy, J. Helly, A. Jenkins, Y. Rosas-Guevara, S. White, M. Baes, C. Booth, P. Camps, J. Navarro, Y. Qu, A. Rahmati, T. Sawala, P. Thomas, и J. Trayford. (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/.

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Friedrich Matthieu

Matthieu Hammer

Matthieu Felsinger

Matthieu Saubanère

Matthieu Barukinamwo

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EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxiesE. Altamura, S. Kay, R. Bower, M. Schaller, Y. Bahé, J. Schaye, J. Borrow, и I. Towler. (2022)cite arxiv:2210.09978.Colours and luminosities of z=0.1 simulated galaxies in the EAGLE simulationsJ. Trayford, T. Theuns, R. Bower, J. Schaye, M. Furlong, M. Schaller, C. Frenk, R. Crain, C. Vecchia, и I. McCarthy. (2015)cite arxiv:1504.04374Comment: 20 pages, 7 figures, submitted to MNRAS.SWIFT: task-based hydrodynamics and gravity for cosmological simulationsT. Theuns, A. Chalk, M. Schaller, и P. Gonnet. (2015)cite arxiv:1508.00115Comment: Proceedings of the EASC 2015 conference, Edinburgh, UK, April 21-23, 2015.It's not easy being green: The evolution of galaxy colour in the EAGLE simulationJ. Trayford, T. Theuns, R. Bower, R. Crain, C. Lagos, M. Schaller, и J. Schaye. (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 effect of baryons on the inner density profiles of rich clustersM. Schaller, C. Frenk, R. Bower, T. Theuns, J. Trayford, R. Crain, M. Furlong, J. Schaye, C. Vecchia, и I. McCarthy. (2014)cite arxiv:1409.8297Comment: 13 pages, 7 figures, submitted to MNRAS.The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an endR. Bower, J. Schaye, C. Frenk, T. Theuns, M. Schaller, R. Crain, и S. McAlpine. (2016)cite arxiv:1607.07445Comment: 15 pages, 8 figures.A Hybrid MPI+Threads Approach to Particle Group Finding Using Union-Find.J. Willis, M. Schaller, P. Gonnet, and J. Helly. PARCO, volume 36 of Advances in Parallel Computing, page 263-274. IOS Press, (2019)A machine learning approach to mapping baryons onto dark matter halos using the EAGLE and C-EAGLE simulationsC. Lovell, S. Wilkins, P. Thomas, M. Schaller, C. Baugh, G. Fabbian, and Y. Bahé. (2021)cite arxiv:2106.04980Comment: 15 pages, 13 figures, submitted to MNRAS. Comments welcome!.The properties of "dark" ŁambdaCDM halos in the Local GroupA. Benítez-Llambay, J. Navarro, C. Frenk, T. Sawala, K. Oman, A. Fattahi, M. Schaller, J. Schaye, R. Crain, and T. Theuns. (2016)cite arxiv:1609.01301Comment: Submitted to MNRAS. Comments are welcome.The Hydrangea simulations: galaxy formation in and around massive clustersY. Bahé, D. Barnes, C. Vecchia, S. Kay, S. White, I. McCarthy, J. Schaye, R. Bower, R. Crain, T. Theuns and 5 other author(s). (2017)cite arxiv:1703.10610Comment: 22 pages, 15 figures (18 pages, 14 figures without appendices); submitted to MNRAS.