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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.

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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.Identification of the brightest Ly\alpha\ emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era, , , , , and . (2015)cite arxiv:1502.07355Comment: 20 pages, main results shown in Fig. 6 and Fig. 7, submitted to MNRAS.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.Boötes-HiZELS: an optical to near-infrared survey of emission-line galaxies at $z=0.4-4.7$, , , , , , , and . (2017)cite arxiv:1702.04721Comment: Submitted to MNRAS. Main text 16 pages, 7 Figures.Resolved Lyman-\alpha properties of a luminous Lyman-break galaxy in a large ionised bubble at z = 6.53, , , , , , , and . (2019)cite arxiv:1909.06376Comment: 12 pages, 10 figures. Submitted to MNRAS.Mapping the Dynamics of a Giant Ly-alpha Halo at z=4.1 with MUSE: The Energetics of a Large Scale AGN-Driven Outflow around a Massive, High-Redshift Galaxy, , , , , , , , , and . (2015)cite arxiv:1502.05998Comment: 11 pages, 5 figures. MNRAS in press.Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts, , , , , , , , , and 13 other author(s). (2020)cite arxiv:2007.13859Comment: 22 pages, 13 figures. Accepted for publication in ApJ.