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EMMA: an AMR cosmological simulation code with radiative transfer

, , and . (2015)cite arxiv:1508.07888Comment: Accepted for publication in MNRAS, 28 pages, 27 figures.

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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.RAMSES-RT: Radiation hydrodynamics in the cosmological context, , , , and . (2013)cite arxiv:1304.7126Comment: 46 pages, 37 figures, submitted to MNRAS, comments are welcome.A deep learning model to emulate simulations of cosmic reionization, , , , , , and . (2019)cite arxiv:1905.06958Comment: 11 pages, 8 figures, submitted to MNRAS.The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models, , , , , , , , and . (2021)cite arxiv:2105.02250Comment: 18 pages, 11 figures, 4 tables. Submitted to MNRAS, comments welcome.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.Rethinking the Accessibility of Digital Content with Perceptual Supplementation System through the Lens of an Ethics of Care., , , and . IxD&A, (2018)Perceptive Supplementation for an Access to Graphical Interfaces., , , , , and . HCI (5), volume 4554 of Lecture Notes in Computer Science, page 841-850. Springer, (2007)Constraining the second half of reionization with the Lyman-$\beta$ forest, , , , and . (2019)cite arxiv:1912.05582Comment: 10 pages, 8 figures, 1 table. 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.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.