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CLEAR: Boosted Ly$\alpha$ Transmission of the Intergalactic Medium in UV bright Galaxies

, , , , , , , , , , , , , and . (2021)cite arxiv:2111.14863Comment: 21 pages, 9 figures, 2 tables, 1st revision submitted to ApJ.

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The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , and 54 other author(s). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.CLEAR: Boosted Ly$\alpha$ Transmission of the Intergalactic Medium in UV bright Galaxies, , , , , , , , , and 4 other author(s). (2021)cite arxiv:2111.14863Comment: 21 pages, 9 figures, 2 tables, 1st revision submitted to ApJ.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , and 57 other author(s). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.