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Testing metallicity indicators at z~1.4 with the gravitationally lensed galaxy CASSOWARY 20

, , , , , , , and . (2013)cite arxiv:1311.5092Comment: 18 pages, 11 figures, submitted to MNRAS on 20/09/2013.

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Searching for z > 6.5 Analogs Near the Peak of Cosmic Star Formation, , , , , , , and . (2019)cite arxiv:1910.11877Comment: 21 pages, 9 figures, submitted to ApJ.Physical Properties of Galaxies from z=2-4. (2011)cite arxiv:1107.5060Comment: ARA&A Volume 49, in press; 123 pages, 18 figures.Testing metallicity indicators at z~1.4 with the gravitationally lensed galaxy CASSOWARY 20, , , , , , , and . (2013)cite arxiv:1311.5092Comment: 18 pages, 11 figures, submitted to MNRAS on 20/09/2013.The MOSDEF Survey: Measurements of Balmer Decrements and the Dust Attenuation Curve at Redshifts z~1.4-2.6, , , , , , , , , and . (2015)cite arxiv:1504.02782Comment: 24 pages, 2 tables, 24 figures, accepted to the Astrophysical Journal.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.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.High Velocity Dispersion in A Rare Grand Design Spiral Galaxy at Redshift z=2.18, , , , , and . (2012)cite arxiv:1207.4196Comment: Accepted for publication in Nature (July 19 2012). Includes 15-page supplement.The MOSDEF Survey: Mass, Metallicity, and Star-formation Rate at z~2.3, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1408.2521Comment: 10 pages, 6 figures, submitted to ApJ.The Kinematics of CIV in Star-Forming Galaxies at z~1.2, , , and . (2016)cite arxiv:1604.03945Comment: 21 pages, 14 figures, submitted to ApJ.A High Fraction of Ly-alpha-Emitters Among Galaxies with Extreme Emission Line Ratios at z ~ 2, , , , , , , and . (2016)cite arxiv:1605.04919Comment: 12 pages, 5 figures, 2 tables. Revised version resubmitted to ApJ.