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The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies

, , , , , , , , , , , , , , and . (2016)cite arxiv:1603.02284Comment: 7 pages, 5 figures, to be published in ApJ Letters.

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The MOSDEF Survey: Detection of OIII$łambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1606.04107Comment: 7 pages, 3 figures, 1 table, submitted to ApJ Letters.The Ionizing Photon Production Efficiency ($\xi_ion$) Of Lensed Dwarf Galaxies At $z 2 $, , , , , , , and . (2019)cite arxiv:1912.06152Comment: 16 pages, 6 figures, 1 table, Submitted to ApJ.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.Ultra-faint Ultraviolet Galaxies at z~2 Behind the Lensing Cluster Abell 1689: the Luminosity Function, Dust Extinction and Star Formation Rate Density, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1305.2413Comment: 14 pages, 10 figures, 4 tables, 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 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.The Evolution Of The Faint End Of The UV Luminosity Function During The Peak Epoch Of Star Formation (1<z<3), , , , , , , , , and 2 other author(s). (2016)cite arxiv:1606.00469Comment: 22 pages, 15 figures.The Lyman Continuum escape fraction of emission line-selected $z\sim2.5$ galaxies is less than 15%, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1705.06355Comment: accepted to ApJ Letters.