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Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15, , , , , , , , , and 19 other author(s). (2022)cite arxiv:2207.09436Comment: Submitted to ApJL, 9 pages, 4 figures.RELICS: Small Lensed $z\geq5.5$ Galaxies Selected as Potential Lyman Continuum Leakers, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2111.14882.An individual star at redshift 1.5 extremely magnified by a galaxy-cluster lens, , , , , , , , , and 35 other author(s). (2017)cite arxiv:1706.10279Comment: Submitted on May 18, 2017. Comments welcome.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.Discovery Of Cold, Pristine Gas Possibly Accreting Onto An Overdensity Of Star-Forming Galaxies At Redshift z ~ 1.6, , , , , , , , , and 5 other author(s). (2011)cite arxiv:1106.1205Comment: 55 pages, 17 figures; submitted to ApJ; the manuscript incorporates the response to the referee report.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.Early results from GLASS-JWST. II: NIRCam extra-galactic imaging and photometric catalog, , , , , , , , , and 19 other author(s). (2022)cite arxiv:2207.11701Comment: Submitted to ApJL; 9 pages, 5 figures, 2 tables.On The Detection Of Ionizing Radiation Arising From Star-Forming Galaxies At Redshift z ~ 3-4 : Looking For Analogs Of "Stellar Reionizers", , , , , , , , , and 8 other author(s). (2012)cite arxiv:1201.5642Comment: Submitted to The Astrophysical Journal, 20 pages, 8 figures, 1 table.