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RAMSES-CH: A New Chemodynamical Code for Cosmological Simulations

, , , , , and . (2012)cite arxiv:1202.6400Comment: Submitted to MNRAS letters,5 pages, 4 figures, comments welcome.

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RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters, , , , , and . (2015)cite arxiv:1510.00718Comment: 20 pages, 10 figures, 2 tables. Submitted to MNRAS.A three-phase amplification of the cosmic magnetic field in galaxies, , , and . Monthly Notices of the Royal Astronomical Society, (Jun 18, 2018)The short ionizing photon mean free path at z=6 in Cosmic Dawn III, a new fully-coupled radiation-hydrodynamical simulation of the Epoch of Reionization, , , , , , , , , and 6 other author(s). (2022)cite arxiv:2202.05869Comment: Submitted to MNRAS.PKDGRAV3: Beyond Trillion Particle Cosmological Simulations for the Next Era of Galaxy Surveys, , and . (2016)cite arxiv:1609.08621Comment: 13 pages, 7 figures, submitted to Computational Astrophysics and Cosmology.RAMSES-RT: Radiation hydrodynamics in the cosmological context, , , , and . (2013)cite arxiv:1304.7126Comment: 46 pages, 37 figures, submitted to MNRAS, comments are welcome.Galaxies that Shine: radiation-hydrodynamical simulations of disk galaxies, , , and . (2015)cite arxiv:1501.04632Comment: 28 pages, 26 figures, submitted to MNRAS.Dancing in the dark: galactic properties trace spin swings along the cosmic web, , , , , , , , , and 23 other author(s). (2014)cite arxiv:1402.1165Comment: 17 pages, 20 pages, submitted to MNRAS, comments are welcome, movies and pictures of the simulation can be found at this address http://horizon-AGN.projet-horizon.fr.Cosmic Dawn (CoDa): the First Radiation-Hydrodynamics Simulation of Reionization and Galaxy Formation in the Local Universe, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1511.00011Comment: 20 pages, 13 figures, submitted to MNRAS.The long lives of giant clumps and the birth of outflows in gas-rich galaxies at high redshift, , , , , , , , , and 6 other author(s). (Jul 26, 2013)A small-scale dynamo in feedback-dominated galaxies as the origin of cosmic magnetic fields. I-the kinematic phase, and . (Jun 2, 2015)