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Absorption Line Spectroscopy of Gravitationally-Lensed Galaxies: Further Evidence for an Increased Escape Fraction of Ionizing Photons at High Redshift, , , , и . (2016)cite arxiv:1606.05309Comment: 13 pages, 9 figures.Lyman-alpha and CIII Emission in z=7-9 Galaxies: Accelerated Reionization Around Luminous Star Forming Systems?, , , , , , , , , и 2 other автор(ы). (2016)cite arxiv:1606.01304Comment: Submitted to MNRAS, 13 pages, 8 figures.Limit theorems for maximum likelihood estimators in the Curie-Weiss-Potts model, и . Stochastic Processes and their Applications, 40 (2): 251--288 (марта 1992)The Assembly History of Disk Galaxies: I - The Tully-Fisher Relation to z~1.3 from Deep Exposures with DEIMOS, , , , и . (2011)cite arxiv:1102.3911 Comment: 19 pages, 10 figures, submitted to ApJ.Connecting the Gamma Ray Burst Rate and the Cosmic Star Formation History: Implications for Reionization and Galaxy Evolution, и . (2011)cite arxiv:1109.0990 Comment: Submitted to ApJ.The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies, , , и . (2020)cite arxiv:2005.11078Comment: 12 pages, 9 figures, 3 tables, submitted to the Astrophysical Journal.The role of galaxies and AGN in reionising the IGM -- III : IGM-galaxy cross-correlations at z~6 from 8 quasar fields with DEIMOS and MUSE, , , , , , , , и . (2019)cite arxiv:1912.04314Comment: Submitted to MNRAS. 17 pages, 18 figures, 3 tables + appendices. Key results: Figs. 6,13,14.The Lyman Continuum Escape Survey: Connecting Time-Dependent OIII and OII Line Emission with Lyman Continuum Escape Fraction in Simulations of Galaxy Formation, , , , , , и . (2020)cite arxiv:2010.00592Comment: 12 pages, 5 figures, submitted to ApJL on September 15, 2020.Dust in the reionization era: ALMA observations of a $z$=8.38 Galaxy, , , , , , , , и . (2017)cite arxiv:1703.02039Comment: Accepted for publication in ApJL.The Origin and Evolution of Metallicity Gradients: Probing the Mode of Mass Assembly at z=2, , , и . (2012)cite arxiv:1207.4489Comment: Submitted to ApJ.