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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.Inferring the IGM Neutral Fraction at z ~ 6-8 with Low-Luminosity Lyman Break Galaxies, , , , , , , , and . (2021)cite arxiv:2111.14912Comment: 11 pages, 7 figures.Early Results from GLASS-JWST. I: Confirmation of Lensed $z\geqslant7$ Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISS, , , , , , , , , and 22 other author(s). (2022)cite arxiv:2207.11387Comment: Submitted to ApJL. 10 pages, 3 figures, 1 table.RELICS: Small Lensed $z\geq5.5$ Galaxies Selected as Potential Lyman Continuum Leakers, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2111.14882.Early results from GLASS-JWST VIII: An Extremely Magnified Blue Supergiant Star at Redshift 2.65 in the Abell 2744 Cluster Field, , , , , , , , , and 11 other author(s). (2022)cite arxiv:2207.11658Comment: 10 pages, 3 figures, submitted to ApJL.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 Grism lens-amplified survey from space (GLASS). VIII. The influence of the cluster properties on Halpha emitter galaxies at 0.3<z<0.7, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1610.04615Comment: submitted to ApJ (17 pages, 10 figures).Spectroscopically Confirmed Lyman-Alpha Emitters from Redshift 5 to 7 Behind Ten Galaxy Cluster Lenses, , , , , , , , , and 3 other author(s). (2020)cite arxiv:2002.08952Comment: 21 pages, 10 figures, submitted to ApJ.A massive interacting galaxy 525 million years after the Big Bang, , , , , , , , , and 17 other author(s). (2023)cite arxiv:2303.00306Comment: 52 pages, 10 figures.ALMA CII detection of a redshift 7 lensed galaxy behind RXJ1347.1-1145, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1610.02099Comment: Submitted for publication to ApJLetters.