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Revealing Galaxy Candidates out to $z 16$ with JWST Observations of the Lensing Cluster SMACS0723, , , , , , and . (2022)cite arxiv:2207.12338Comment: 14 pages, 15 figures, 2 tables, submission to MNRAS.Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey, , , , , , , , , and 6 other author(s). (2013)cite arxiv:1305.1399Comment: 15 pages, 13 figures, submitted to ApJ.Low Masses and High Redshifts: The Evolution of the Mass-Metallicity Relation, , , , , , , , , and 8 other author(s). (2013)cite arxiv:1309.4458Comment: Accepted for publication in ApJ Letters.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , and 6 other author(s). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization, , , , , , , , , and 24 other author(s). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.On the influence of physical galaxy properties on Lyman-alpha escape in star-forming galaxies, , , , , , , and . (2013)cite arxiv:1308.6577Comment: 17 pages. Accepted for publication.The Lyman alpha Reference Sample: Extended Lyman alpha Halos Produced at Low Dust Content, , , , , , , , , and 7 other author(s). (2013)cite arxiv:1303.0006Comment: Published in ApJ Letters ~~ 6 pages using emulateapj, 4 figures ~~ Higher-resolution, larger, nicer jpeg versions of Figures 1 and 2 can be found here: http://xayes.org/pub/press_lars.html.Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1402.0510Comment: Accepted for publication in ApJ.Reionization with galaxies and active galactic nuclei, , , , , , , , and . (2020)cite arxiv:2001.06021Comment: Submitted to MNRAS; comments welcome.The Faint-end of the UV Luminosity Function at z~6 to z~8: Combined Constraints from the Hubble Frontier Fields Clusters and Parallels, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1509.06764Comment: 13 pages, 10 figures, 4 tables, submitted to ApJ.