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UVUDF: Ultraviolet Imaging of the Hubble Ultradeep Field with Wide-field Camera 3, , , , , , , , , and 16 other author(s). (2013)cite arxiv:1305.1357Comment: Submitted AJ.RELICS: Small Lensed $z\geq5.5$ Galaxies Selected as Potential Lyman Continuum Leakers, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2111.14882.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.RELICS-DP7: Spectroscopic Confirmation of a Dichromatic Primeval Galaxy at z ~ 7, , , , , , , , , and 5 other author(s). (2020)cite arxiv:2011.08857Comment: 8 pages, 3 figures, 1 table. Submitted to ApJL.The UV Continuum of $z>1$ Star-forming Galaxies in the Hubble Ultraviolet UltraDeep Field, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1407.3680Comment: 7 pages, 4 figures, 1 table. Submitted to ApJL. Revised in response to referee comments.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.Geometric Corroboration of the Earliest Lensed Galaxy at z~10.8 from Robust Free-Form Modelling, , , , , , and . (2016)cite arxiv:1608.06942Comment: arXiv admin note: text overlap with arXiv:1406.2702.A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old, , , , , , , , , and 26 other author(s). (2012)cite arxiv:1204.2305Comment: Submitted to the Nature Journal. 39 Pages, 13 figures.Stellar Properties of z ~ 8 Galaxies in the Reionization Lensing Cluster Survey, , , , , , , , , and 11 other author(s). (2019)cite arxiv:1905.09295Comment: 8 pages, 3 figures, 2 tables.CLASH: Three Strongly Lensed Images of a Candidate z ~ 11 Galaxy, , , , , , , , , and 13 other author(s). (2012)cite arxiv:1211.3663Comment: Accepted for publication in the Astrophysical Journal. 23 pages, 18 figures.