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The dust content of galaxies from z = 0 to z = 9, , и . (2016)cite arxiv:1609.08622Comment: Submitted to MNRAS.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.Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7, , , , , , , и . (2021)cite arxiv:2109.13241Comment: 28 pages, 23 figures, accepted for publication in MNRAS.Sub-mm Emission Line Deep Fields: CO and CII Luminosity Functions out to z = 6, , , , , и . (2016)cite arxiv:1602.02761Comment: 19 pages, 11 figures, 3 table, submitted to MNRAS.On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations, , , , , и . (2021)cite arxiv:2106.14904Comment: 15 pages, 8 figures, submitted to ApJ.An empirical representation of a physical model for the ISM CII, CO, and CI emission at redshift $1złeq9$, , , , , и . (2021)cite arxiv:2108.07716Comment: 15 pages, 9 figures.On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance, , , и . (2024)The effect of metal enrichment and galactic winds on galaxy formation in cosmological zoom simulations, , , , , , , , , и 2 other автор(ы). (2013)cite arxiv:1309.2946Comment: 23 pages, 16 figues, and 1 table, submitted to MNRAS.Predictions of the LCII -- SFR and CII Luminosity Function at the Epoch of Reionization, , , , , , , и . (2020)cite arxiv:2004.11912Comment: 17 pages, 13 figures, submitted to the ApJ.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2, , , , , , , , , и 28 other автор(ы). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.