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Paper 1: The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies, , , , , , , , , and 34 other author(s). (2023)cite arxiv:2303.03556Comment: 23 pages, submitted to ApJ.Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper.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.Metallicities of Emission-Line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4, , , , , , , , , and 2 other author(s). (2012)cite arxiv:1205.3172Comment: 24 pages with 7 figures.Webb's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results, , , , , , , , , and 73 other author(s). (2022)cite arxiv:2209.04119Comment: Submitted to AJ, comments welcome. We ask anyone who uses our public PEARLS (NEP TDF) data to refer to this overview paper.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.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.