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HST Emission Line Galaxies at z ~ 2: The Ly-alpha Escape Fraction

, , , , , , , , , , and . (2014)cite arxiv:1409.8304Comment: 14 pages, 3 figures, Accepted to ApJ.

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HST Emission Line Galaxies at z ~ 2: The Ly-alpha Escape Fraction, , , , , , , , , and 1 other author(s). (2014)cite arxiv:1409.8304Comment: 14 pages, 3 figures, Accepted to 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.Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1505.03877Comment: 18 pages, 6 figures, 4 tables, accepted for publication in ApJ.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 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.