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First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\geq5$, , , , , , , и . (2022)cite arxiv:2203.12627.The Lyman-continuum photon production efficiency in the high-redshift Universe, , , , , , и . (2015)cite arxiv:1512.03214Comment: 4 pages, 2 figures, submitted to MNRAS. Comments welcome.First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Evolution, , , , , , и . (2020)cite arxiv:2004.07283Comment: 20 pages, 19 figures, submitted to MNRAS. Comments welcome!.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , и 54 other автор(ы). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.Extreme Value Statistics of the Halo and Stellar Mass Distributions at High Redshift: are JWST Results in Tension with ŁambdaCDM?, , , , и . (2022)cite arxiv:2208.10479Comment: 10 pages, 7 figures, submitted to MNRAS, comments welcome!.VLT/XSHOOTER & Subaru/MOIRCS Spectroscopy of HUDF-YD3: No Evidence for Lyman-alpha Emission at z=8.55, , , , , , , и . (2013)cite arxiv:1301.4477Comment: Accepted for publication in MNRAS.Luminosity function of OII emission-line galaxies in the MassiveBlack-II simulation, , , , , , и . (2015)cite arxiv:1508.05106Comment: 12 pages, 13 figures, 3 tables, accepted for publication in MNRAS.Inferred H\alpha Flux as a Star-Formation Rate Indicator at z ~ 4-5: Implications for Dust Properties, Burstiness, and the z = 4-8 Star-Formation-Rate Functions, , , , , и . (2015)cite arxiv:1511.08808Comment: 19 pages, 11 figures, 9 tables, submitted to ApJ.Characterising and Identifying Galaxy Protoclusters, , и . (2017)cite arxiv:1710.02148Comment: 19 pages, 16 figures, submitted to MNRAS.Spectroscopy of z ~ 7 candidate galaxies: Using Lyman-alpha to constrain the neutral fraction of hydrogen in the high-redshift universe, , , , , , и . (2013)cite arxiv:1311.0057Comment: submitted to MNRAS.