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How Lyman Alpha Emission Depends On Galaxy Stellar Mass, , , , , , , , и . (2016)cite arxiv:1604.03113Comment: 4 pages, 5 figures.A Comprehensive Study of Ly$\alpha$ Emission in the High-redshift Galaxy Population, , , , и . (2017)cite arxiv:1706.01886Comment: Accepted for publication in ApJ.IZI: Inferring the Gas Phase Metallicity (Z) and Ionization Parameter (q) of Ionized Nebulae using Bayesian Statistics, , , и . (2014)cite arxiv:1410.8146Comment: 23 pages, 9 figures, Accepted for publication in The Astrophysical Journal (Oct 28 2014).Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE, , , , , , , , , и 9 other автор(ы). (2014)cite arxiv:1402.0510Comment: Accepted for publication in ApJ.Enhanced Abundances in Spiral Galaxies of the Pegasus I Cluster, , и . (2011)cite arxiv:1112.5975Comment: 28 pages, 7 figures, 5 tables. Submitted to ApJ.A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5<z<6.8: Program Overview and a Sample of the Brightest Lyman-alpha Emitters, , , , , , , , , и 9 other автор(ы). (2017)cite arxiv:1708.05249Comment: 18 pages, 11 figures, Accepted for publication in The Astrophysical Journal.HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies, , , , , , , , , и 7 other автор(ы). (2015)cite arxiv:1512.03063Comment: Accepted to the ApJ. 32 pages, 4 figures, and 2 tables.HST Emission Line Galaxies at z ~ 2: The Ly-alpha Escape Fraction, , , , , , , , , и 1 other автор(ы). (2014)cite arxiv:1409.8304Comment: 14 pages, 3 figures, Accepted to ApJ.The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy, , , , , , , , , и 12 other автор(ы). (2014)cite arxiv:1406.4503Comment: 26 pages, accepted for publication in ApJ.An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?, , и . (2015)cite arxiv:1506.02036Comment: 9 pages, 4 figures; accepted for publication in ApJ.