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The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1611.07038Comment: 11 pages, 6 figures, submitted to ApJ.ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1608.02941Comment: Accepted for publication in ApJ.Herschel protocluster survey: A search for dusty star-forming galaxies in protoclusters at z=2-3, , , , , , , , , and 8 other author(s). (2016)cite arxiv:1605.07370Comment: 15 pages, 5 figures, 12 tables, Accepted for publication in MNRAS.Constraints on the assembly and dynamics of galaxies. II. Properties of kiloparsec-scale clumps in rest-frame optical emission of z ~ 2 star-forming galaxies, , , , , , , , , and 4 other author(s). (2011)cite arxiv:1104.0248 Comment: 29 pages, 11 figures, submitted to Astrophysical Journal.Reconciling the Stellar and Nebular Spectra of High Redshift Galaxies, , , , , and . (2016)cite arxiv:1605.07186Comment: 29 pages, 17 figures. Accepted for publication in the Astrophysical Journal.Strong Nebular Line Ratios in the Spectra of z~2-3 Star-forming Galaxies: First Results from KBSS-MOSFIRE, , , , , , , , , and 4 other author(s). (2014)cite arxiv:1405.5473Comment: 38 pages, 25 figures. Submitted to the Astrophysical Journal. Version with full-resolution figures available at http://www.astro.caltech.edu/~ccs/mos_bpt_submit.pdf.Spectroscopic Measurements of the Far-Ultraviolet Dust Attenuation Curve at z~3, , , and . (2016)cite arxiv:1606.00434Comment: 12 pages, 1 table, 8 figures, accepted to the Astrophysical Journal.Q1549-C25: A Clean Source of Lyman-Continuum Emission at $z=3.15$, , , , , , , and . (2016)cite arxiv:1606.00443Comment: 6 pages, 5 figures, submitted to ApJ Letters.The Lyman Continuum Escape Fraction of The Cosmic Horseshoe: A Test of Indirect Estimates, , , , , , , , and . (2016)cite arxiv:1603.02309Comment: 10 pages, 8 Figures, submitted to the Astrophysical Journal.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.