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A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields

, , , , , , , , , , , , , , , , , , , , , , , and . (2021)cite arxiv:2106.13813Comment: 47 figures, 25 pages, 10 tables, submitted to the Astrophysical Journal.

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Simulating properties of emission line galaxies from Nancy Grace Roman Space Telescope, , , , , , and . (2021)cite arxiv:2109.12216Comment: 12 pages, 12 figures; comments welcome.A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields, , , , , , , , , and 14 other author(s). (2021)cite arxiv:2106.13813Comment: 47 figures, 25 pages, 10 tables, submitted to the Astrophysical Journal.On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2111.05351Comment: 27 pages + Appendix; Submitted to ApJ; Comments welcome.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations, , , , , , , , , and 54 other author(s). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.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.Probing the Bright End of the Rest-Frame Ultraviolet Luminosity Function at z = 8-10 with Hubble Pure-Parallel Imaging, , , , , , , and . (2020)cite arxiv:2002.06209Comment: Accepted to the Astrophysical Journal, 23 pages, 10 Figures.CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST, , , , , , , , , and 57 other author(s). (2022)cite arxiv:2211.05792Comment: 41 pages, 20 figures, 6 tables, submitted to ApJL. Key results in Figures 13-15, discussed in Sections 7 and 8.CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST, , , , , , , , , and 49 other author(s). (2022)cite arxiv:2208.14480Comment: Submitted to ApJ; 12 Pages, 6 Figures.