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Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies

, , , , , , , , and . (2021)cite arxiv:2111.14912Comment: 11 pages, 7 figures.

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ELT-MOS White Paper: Science Overview &amp; Requirements, , , , , , , , , and 11 other author(s). (Feb 28, 2013)Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies, , , , , , , , and . (2021)cite arxiv:2111.14912Comment: 11 pages, 7 figures.Deep ALMA redshift search of a z~12 GLASS-JWST galaxy candidate, , , , , , , , , and 13 other author(s). (2022)cite arxiv:2208.13642Comment: Submitted to MNRAS. Comments welcome.The production of ionizing photons in UV-faint z~3-7 galaxies, , , , , , , , , and 13 other author(s). (2022)cite arxiv:2211.12548Comment: 10 pages, 7 figures, submitted to A&A.A large-scale galaxy structure at z = 2.02 associated with the radio galaxy MRC0156-252, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1309.6645Comment: 11 pages, 9 figures, 2 tables, accepted for publication in A&A.The Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1610.04615Comment: submitted to ApJ (17 pages, 10 figures).Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1704.02970.The Universe is Reionizing at z~7: Bayesian Inference of the IGM Neutral Fraction Using Ly$\alpha$ Emission from Galaxies, , , , , , , and . (2017)cite arxiv:1709.05356Comment: 15 pages, 12 figures. Submitted to ApJ.HST Grism Observations of a Gravitationally Lensed Redshift 10 Galaxy, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1709.03992Comment: Submitted to ApJ.A shot in the Dark (Ages): a faint galaxy at $z=9.76$ confirmed with JWST, , , , , , , , , and 35 other author(s). (2022)cite arxiv:2210.15639Comment: Submitted to Nature. 34 pages, 4 main figures, 1 supplementary figure, 2 supplementary tables. Comments are welcome.