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The MOSDEF Survey: Mass, Metallicity, and Star-formation Rate at z~2.3

, , , , , , , , , , and . (2014)cite arxiv:1408.2521Comment: 10 pages, 6 figures, submitted to ApJ.

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The MOSDEF Survey: Detection of OIII$łambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1606.04107Comment: 7 pages, 3 figures, 1 table, submitted to ApJ Letters.Direct measurement of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation rates, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1310.4177Comment: Submitted for publication in the Astrophysical Journal.The MOSDEF Survey: The strong agreement between H-alpha and UV-to-FIR star formation rates for z~2 star-forming galaxies, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1603.02284Comment: 7 pages, 5 figures, to be published in ApJ Letters.The MOSDEF Survey: Dissecting the star-formation rate vs. stellar mass relation using H$\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 Evolution and Origin of Ionized Gas Velocity Dispersion from $z\sim2.6$ to $z\sim0.6$ with KMOS$^3D$, , , , , , , , , and 20 other author(s). (2019)cite arxiv:1906.02737Comment: ~30 pages, 16 figures, 9 tables; accepted for publication in ApJ.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 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.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , and 14 other author(s). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.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 MOSDEF Survey: Broad Emission Lines at z=1.4-3.8, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1710.03230.