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The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2

, , , , , , , , , , , and . (2015)cite arxiv:1507.03017Comment: 12 pages, 8 figures, 2 tables, submitted to ApJ.

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The MOSDEF Survey: Broad Emission Lines at z=1.4-3.8, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1710.03230.The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\alpha$ and H$\beta$ emission lines at z ~ 2, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1507.03017Comment: 12 pages, 8 figures, 2 tables, submitted to ApJ.The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1603.02284Comment: 7 pages, 5 figures, to be published in ApJ Letters.The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at $z>4$, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1707.05331Comment: 6 pages, 3 figures, submitted to ApJ Letters.The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, $\xi_ion$, at z~2, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1711.00013Comment: 14 pages, 8 figures, 1 table, submitted to ApJ.The MOSDEF survey: a stellar mass-SFR-metallicity relation exists at $z\sim2.3$, , , , , , , , , and 8 other author(s). (2017)cite arxiv:1711.00224Comment: 18 pages, 7 figures, submitted to ApJ.The MOSDEF survey: the prevalence and properties of galaxy-wide AGN-driven outflows at $z2$, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1703.10255Comment: 22 pages, 16 figures, submitted to ApJ.