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The properties of warm dark matter haloes

, , , , , and . (2013)cite arxiv:1308.1399Comment: 20 pages, 21 Figures, Submitted to MNRAS.

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ETHOS -- an effective theory of structure formation: Predictions for the high-redshift Universe -- abundance of galaxies and reionization, , , , , , , , and . (2017)cite arxiv:1711.10497Comment: 15 pages, 8 figures, to be submitted to MNRAS. Please contact lovell@hi.is with any comments.The properties of warm dark matter haloes, , , , , and . (2013)cite arxiv:1308.1399Comment: 20 pages, 21 Figures, Submitted to MNRAS.The galaxy population in cold and warm dark matter cosmologies, , , , , , , , , and . (2016)cite arxiv:1612.04540Comment: 15 pages, 14 figures, submitted to MNRAS.The fraction of dark matter within galaxies from the IllustrisTNG simulations, , , , , , , , , and 2 other author(s). (2018)cite arxiv:1801.10170Comment: 27 pages, 14 figures, highlights: Figs. 11, 12, 13. Revised version accepted by MNRAS. Please contact lovell@hi.is with any comments.Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way, , , , , , , and . (2020)cite arxiv:2011.08865Comment: 21 pages (JCAP format), 3 appendices, 10 figures, 1 table. Comments welcome.