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The large-scale environment from cosmological simulations I: The baryonic cosmic web

, , , , , , , and . (2017)cite arxiv:1708.02302Comment: 13 pages, 8 figures, submitted to MNRAS.

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A warm mode of gas accretion on forming galaxies, , , , , and . (2012)cite arxiv:1202.5212Comment: 6 pages, 3 figures, accepted for publication in ApJL.Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1510.04277Comment: 18 pages, 12 figures. Comments welcome.Temperature Structure of the Intra-Cluster Medium from SPH and AMR simulations, , , , , , , , , and 1 other author(s). (Jun 17, 2014)Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium, , , , , and . (2022)cite arxiv:2202.00974Comment: 14 pages, 8 figures.The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D, , , , , , and . (2014)cite arxiv:1412.6105Comment: 12 pages, 10 figures, submitted to MNRAS.Turbulence driven by structure formation in the circum-galactic medium, , and . (2013)cite arxiv:1304.3465Comment: 14 pages, 17 figures, MNRAS, accepted.On the impact of baryons on the halo mass function, bias, and cluster cosmology, , , , , , and . (2020)cite arxiv:2009.01775Comment: 22 pages, 17 figures; comments are welcome.Shall numerical astrophysics step into the era of Exascale computing?, , , , , , , and . CoRR, (2019)nIFTy galaxy cluster simulations I: dark matter & non-radiative models, , , , , , , , , and 17 other author(s). (2015)cite arxiv:1503.06065Comment: 21 pages, 13 figures, 4 tables - submitted to MNRAS.The large-scale environment from cosmological simulations I: The baryonic cosmic web, , , , , , , and . (2017)cite arxiv:1708.02302Comment: 13 pages, 8 figures, submitted to MNRAS.