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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.

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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.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.DUSTiER (DUST in the Epoch of Reionization): dusty galaxies in cosmological radiation-hydrodynamical simulations of the Epoch of Reionization with RAMSES-CUDATON, , , , , , and . (2022)cite arxiv:2204.03949Comment: submitted to MNRAS, 1st report received: under revision Have partially addressed referee's concerns, namely that the model predicts high dust masses and redder bright galaxies than expected, by discussing this aspect around the relevant results. Work is being carried out to present a clearer parameter exploration of the dust model.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.