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The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift

, , , , , , , , , , , and . (2022)cite arxiv:2201.03564Comment: 25 pages, 15 figures. Accepted for publication in ApJ.

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The Spectroscopic Properties of Ly\alpha-Emitters at z $\approx$ 2.7: Escaping Gas and Photons from Faint Galaxies, , , and . (2015)cite arxiv:1506.08205.Measuring the Physical Conditions in High-Redshift Star-Forming Galaxies: Insights from KBSS-MOSFIRE, , , , and . (2017)cite arxiv:1711.08820Comment: 24 pages, 20 figures. Submitted to the Astrophysical Journal.The redshift evolution of rest-UV spectroscopic properties in Lyman Break Galaxies at z ~ 2-4, , , , , , , , , and 1 other author(s). (2018)cite arxiv:1803.05912Comment: 27 pages, 14 figures, submitted to ApJ.The BPT Diagram in Cosmological Galaxy Formation Simulations: Understanding the Physics Driving Offsets at High-Redshift, , , , , , , , , and 2 other author(s). (2022)cite arxiv:2201.03564Comment: 25 pages, 15 figures. Accepted for publication in ApJ.Metal-line absorption around $z\approx$2.4 star-forming galaxies in the Keck Baryonic Structure Survey, , , , and . (2014)cite arxiv:1403.0942Comment: Submitted to MNRAS, 21 pages, 12 figures (not including appendices).Detection of hot, metal-enriched outflowing gas around $z\approx\,$2.3 star-forming galaxies in the Keck Baryonic Structure Survey, , , , and . (2014)cite arxiv:1410.8214Comment: Submitted to MNRAS, 14 pages, 9 figures (not including appendices).A High Fraction of Ly-alpha-Emitters Among Galaxies with Extreme Emission Line Ratios at z ~ 2, , , , , , , and . (2016)cite arxiv:1605.04919Comment: 12 pages, 5 figures, 2 tables. Revised version resubmitted to ApJ.Nebular Emission Line Ratios in z~2-3 Star-Forming Galaxies with KBSS-MOSFIRE: Exploring the Impact of Ionization, Excitation, and Nitrogen-to-Oxygen Ratio, , , , , and . (2016)cite arxiv:1608.02587Comment: 28 pages, 26 figures. Submitted to the Astrophysical Journal.The Rest-Frame Optical Spectroscopic Properties of Ly$\alpha$-Emitters at $z\sim2.5$: The Physical Origins of Strong Ly$\alpha$ Emission, , , and . (2016)cite arxiv:1608.07280Comment: 26 pages, 19 figures. Submitted to ApJ. Comments welcome.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.