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Evolution of the Ly-alpha luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization ?

, , , , , , , , , , , , , , , , , , , and . (2011)cite arxiv:1105.4235 Comment: 14 pages, 6 figures, submitted to A&A.

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Onset of Cosmic Reionization: Evidence of An Ionized Bubble Merely 680 Myrs after the Big Bang, , , , , , , , , and 7 other author(s). (2020)cite arxiv:2001.00873.First results from Faint Infrared Grism Survey (FIGS): first simultaneous detection of Lyman-\alpha emission and Lyman break from a galaxy at z=7.51, , , , , , , , , and 15 other author(s). (2016)cite arxiv:1605.06519Comment: Resubmitted after incorporating referee's comments.Evolution of the Ly-alpha luminosity function from z = 6.5 to z = 7.7: evidence for the epoch of reionization ?, , , , , , , , , and 10 other author(s). (2011)cite arxiv:1105.4235 Comment: 14 pages, 6 figures, submitted to A&amp;A.The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index, , , , , , , , , and 3 other author(s). (2019)cite arxiv:1909.07888Comment: Accepted for publication in A&A.No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1 z 3.5$, , , , , , , , , and 8 other author(s). (2021)cite arxiv:2109.03662Comment: 18 pages, 11 figures, 1 appendix, submitted to Monthly Notices of the Royal Astronomical Society.