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Reionization time of the Local Group and Local-Group-like halo pairs

, , , , , , , , , and . (2022)cite arxiv:2207.13102Comment: Accepted for publication in MNRAS, 11 pages, 5 figures.

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A deep learning model to emulate simulations of cosmic reionization, , , , , , and . (2019)cite arxiv:1905.06958Comment: 11 pages, 8 figures, submitted to MNRAS.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.Lyman-alpha opacities at z=4-6 require low mass, radiatively-suppressed galaxies to drive cosmic reionization, , , , , , and . (2021)cite arxiv:2105.01663Comment: 9 pages, 6 figures, subbmitted to MNRAS.Scattering of Ly\alpha Photons through the Reionizing Intergalactic Medium: I. Spectral Energy Distribution, , , , , , , , , and . (2022)cite arxiv:2202.06277Comment: 16 pages, 12 figures, Submitted to ApJ.Topology of Reionisation times: concepts, measurements and comparisons to gaussian random field predictions, , , and . (2022)cite arxiv:2209.11608Comment: 20 pages, 19 figures, 3 tables. Submitted to Astronomy & Astrophysics.LyC escape from SPHINX galaxies in the Epoch of Reionization, , , , , , , , , and . (2022)cite arxiv:2207.03232Comment: 20 figures, 21 pages plus appendices. Accepted for publication in MNRAS.Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation, , , , , , , , , and 3 other author(s). (2020)cite arxiv:2004.14496Comment: 13 pages, 12 figures.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.Galactic ionising photon budget during the Epoch ofReionisation in the Cosmic Dawn II simulation, , , , , , , , , and 3 other author(s). (2020)cite arxiv:2001.07785Comment: Submitted to MNRAS.Crucial Factors of Ly\alpha Transmission in the Reionizing Intergalactic Medium: Infall Motion, HII Bubble Size, and Self-shielded Systems, , , , , , , , , and . (2021)cite arxiv:2105.10770Comment: 15 pages, 11 figures, 4 tables, submitted to ApJ.