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The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23

, , , , , , , , and . (2016)cite arxiv:1609.05897Comment: 18 pages, 10 figures. Submitted to MNRAS in July. Comments welcome.

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The evolution of the UV luminosity and stellar mass functions of Lyman-alpha emitters from z~2 to z~6, , , , , , , , , and . (2021)cite arxiv:2105.00007Comment: Accepted for publication in MNRAS. 20 pages, 13 figures, 4 tables.The CALYMHA survey: Ly$\alpha$ escape fraction and its dependence on galaxy properties at $z=2.23$, , , , , , and . (2016)cite arxiv:1602.02756Comment: Accepted for publication by MNRAS.The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23, , , , , , , , and . (2016)cite arxiv:1609.05897Comment: 18 pages, 10 figures. Submitted to MNRAS in July. Comments welcome.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.On the UV compactness and morphologies of typical Lyman-a emitters from z~2 to z~6, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1709.04470Comment: 17 pages, 12 figures. Submitted to MNRAS on July 25, 2017. Comments are welcome.