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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.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.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.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.A strong He II $łambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?, , , , , , , , , and 1 other author(s). (2022)cite arxiv:2212.04476Comment: Submitted.