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On the influence of physical galaxy properties on Lyman-alpha escape in star-forming galaxies

, , , , , , , and . (2013)cite arxiv:1308.6577Comment: 17 pages. Accepted for publication.

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The ALPINE-ALMA C II survey: the luminosity function of serendipitous C II line emitters at $z5$, , , , , , , , , and 25 other author(s). (2020)cite arxiv:2006.04837Comment: 19 pages, 12 figures; submitted to Astronomy & Astrophysics.The Low-Redshift Lyman Continuum Survey: Optically Thin and Thick Mg II Lines as Probes of Lyman Continuum Escape, , , , , , , , , and 7 other author(s). (2023)cite arxiv:2301.04087Comment: 12 pages, 5 figures, 2 tables, accepted to ApJ.The Stellar Populations of Low-Luminosity Active Galactic Nuclei. I. Ground-based Observations, , , , , , , , and . The Astrophysical Journal, 605 (1): 105 (2004)The Lyman Alpha Reference Sample: V. The impact of neutral ISM kinematics and geometry on Lyman Alpha escape, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1503.01157Comment: 28 pages, 19 figures, 5 tables.The Lyman-alpha Reference Sample: I. Survey outline and first results for Markarian 259, , , , , , , , , and 12 other author(s). (2014)cite arxiv:1409.8347Comment: To appear in ApJ.The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.(Re)Solving Reionization with Ly\alpha: How Bright Ly\alpha Emitters account for the $z\approx2-8$ Cosmic Ionizing Background, , , , , , , , , and 5 other author(s). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid, , , , , , , and . (2021)cite arxiv:2107.01230Comment: 13 pages, 4 figures.Evolutionary synthesis models as a tool and guide towards the first galaxies. (2012)cite arxiv:1202.4870Comment: 32 pages, 19 figures. Chapter to appear in "The First Galaxies - Theoretical Predictions and Observational Clues", Eds. T. Wiklind, V. Bromm, B. Mobasher, Springer Verlag.On the nature of the luminous Lya emitter CR7 and its UV components: physical conditions and JWST predictions, , , , , , , , and . (2017)cite arxiv:1710.08422Comment: Submitted to MNRAS, comments welcomed. 19 pages, 11 figures.