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Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts z~2.3--5

, , , , , , , , , , , and . (2016)cite arxiv:1602.01555Comment: 40 pages (4 appendices), 13 (+9) figures, 3 (+4) tables; AASTeX6, pdflatex; submitted to ApJ.

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Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts z~2.3--5, , , , , , , , , and 2 other author(s). (2016)cite arxiv:1602.01555Comment: 40 pages (4 appendices), 13 (+9) figures, 3 (+4) tables; AASTeX6, pdflatex; submitted to ApJ.Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation, , , , , , , and . (2021)cite arxiv:2101.01219Comment: 17 pages, 12 figures. Submitted to MNRAS.Limits to Rest-Frame Ultraviolet Emission From Far-Infrared-Luminous z~6 Quasar Hosts, , , , , , , , , and 13 other author(s). (2020)cite arxiv:2007.13859Comment: 22 pages, 13 figures. Accepted for publication in ApJ.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.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.The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux, , , , , , and . (2023)cite arxiv:2301.03699.Luminous Lyman-alpha Emitters with Very Blue UV-continuum Slopes at Redshift 5.7 <= z <= 6.6, , , , , , and . (2020)cite arxiv:2002.02028Comment: Published in ApJ on 2020 Feb 1; Authors' version (9 pages); See published version at https://iopscience.iop.org/article/10.3847/1538-4357/ab64ea.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.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.Physical Properties of Spectroscopically-Confirmed Galaxies at $z\ge6$. III. Stellar Populations from SED Modeling with Secure Ly$\alpha$ Emission and Redshifts, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1511.01519Comment: 19 pages, 15 figures, accepted for publication in ApJ.