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The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy

, , , , , , , , , , , , , , , , , , , , , and . (2014)cite arxiv:1406.4503Comment: 26 pages, accepted for publication in ApJ.

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The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy, , , , , , , , , and 12 other author(s). (2014)cite arxiv:1406.4503Comment: 26 pages, accepted for publication in ApJ.The Astropy Problem, , , , , , , , , and 144 other author(s). eprint arXiv:astro-ph.IM/1610.03159, (October 2016)The Dust Attenuation Curve versus Stellar Mass for Emission Line Galaxies at z ~ 2, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1511.00651Comment: Accepted for publication in ApJ.HST Emission Line Galaxies at z ~ 2: Comparing Physical Properties of Lyman Alpha and Optical Emission Line Selected Galaxies, , , , , , , , , and 7 other author(s). (2015)cite arxiv:1512.03063Comment: Accepted to the ApJ. 32 pages, 4 figures, and 2 tables.The Rest-Frame Optical Morphology of Emission Line Galaxies at 2 < z < 3: Evidence for Inside-Out Formation in Low-Mass Galaxies, , , , , , , , and . (2016)cite arxiv:1610.01163Comment: 10 pages, 6 figures, and 2 tables. Submitted to ApJ.