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SHARDS Frontier Fields: Physical properties of a low mass Lyman-alpha emitter at z=5.75, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1710.00826Comment: 14 pages, 8 figures, 4 tables. Accepted for publication in ApJ.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.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.The Bursty Star Formation Histories of Low-mass Galaxies at $0.4<z<1$ Revealed by Star Formation Rates Measured from FUV and H$\beta$, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1604.05314Comment: 10 pages, 7 figures. Submitted to ApJ. Comments welcome.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.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.Star Formation in a Stellar Mass Selected Sample of Galaxies to z=3 from the GOODS NICMOS Survey (GNS), , , , , , and . (2011)cite arxiv:1106.2656Comment: 18 pages, 10 figures, accepted for publication in MNRAS.Ultraviolet Through Far-Infrared Spatially Resolved Analysis of the Recent Star Formation in M81 (NGC3031), , , , , , , , , and 7 other author(s). Astrophysics Journal, (2006)cite arxiv:astro-ph/0605605Comment: Accepted for publication in ApJ, 22 pages, 11 figures, 4 tables, the complete data tables can be found in the source.