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A High Space Density of Luminous Lyman Alpha Emitters at z~6.5, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1701.05193Comment: Accepted for publication in ApJ. 20 pages, 13 figures.The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields, , , , , , , , , and 6 other author(s). (2020)cite arxiv:2004.04360Comment: 36 pages, 17 figures, 5 tables. Accepted for publication in The Astrophysical Journal.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.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.The Lyman Continuum escape fraction of emission line-selected $z\sim2.5$ galaxies is less than 15%, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1705.06355Comment: accepted to ApJ Letters.The Lyman Continuum Escape Fraction of Low-Mass Star-Forming Galaxies at z~1, , , , , , , , , and 3 other author(s). (2015)cite arxiv:1511.01998Comment: submitted for second review to ApJ.