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Damped Ly\alpha Absorption Systems in Semi-Analytic Models with Multiphase Gas

, , , , , , and . (2013)cite arxiv:1308.2598Comment: 27 pages, 15 figures, submitted to MNRAS.

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Damped Ly\alpha Absorption Systems in Semi-Analytic Models with Multiphase Gas, , , , , , and . (2013)cite arxiv:1308.2598Comment: 27 pages, 15 figures, submitted to MNRAS.The Terahertz Intensity Mapper (TIM): a Next-Generation Experiment for Galaxy Evolution Studies, , , , , , , , , and 15 other author(s). (2020)cite arxiv:2009.14340Comment: 8 pages, 5 figures, published in the 30th International Symposium on Space THz Technology (ISSTT2019), Gothenburg, Sweden, April 15-17, 2019.Sub-mm Emission Line Deep Fields: CO and CII Luminosity Functions out to z = 6, , , , , and . (2016)cite arxiv:1602.02761Comment: 19 pages, 11 figures, 3 table, submitted to MNRAS.ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using CI and CO, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1703.05764Comment: Accepted for publication in A&A.The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift, , , , , , , , , and 2 other author(s). (2022)cite arxiv:2201.03564Comment: 25 pages, 15 figures. Accepted for publication in ApJ.On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations, , , , , and . (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 $1złeq9$, , , , , and . (2021)cite arxiv:2108.07716Comment: 15 pages, 9 figures.Predictions of the LCII -- SFR and CII Luminosity Function at the Epoch of Reionization, , , , , , , and . (2020)cite arxiv:2004.11912Comment: 17 pages, 13 figures, submitted to the ApJ.To See or Not to See a $z\sim13$ Galaxy? That is the Question, , , , , , , , , and . (2022)cite arxiv:2210.03754Comment: Submitted to A&A, 9 pages, 6 figures,.The dust content of galaxies from z = 0 to z = 9, , and . (2016)cite arxiv:1609.08622Comment: Submitted to MNRAS.