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The interstellar medium in OIII-selected star-forming galaxies at $z\sim3.2$

, , , , , , , , , , , , , and . (2017)cite arxiv:1709.06731Comment: 20 pages, 11 figures, Accepted for publication in ApJ.

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Direct evidence for Ly$\alpha$ depletion in the protocluster core, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1702.00100Comment: 6 pages, 4 figures, accepted for publication in MNRAS Letter.Bulge-forming galaxies with an extended rotating disk at z~2, , , , , , , , , and 17 other author(s). (2016)cite arxiv:1608.05412Comment: 10 pages, 5 figures, 2 tables, submitted to ApJ.Do Galaxy Morphologies Really Affect the Efficiency of Star Formation during the Phase of Galaxy Transition?, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1903.03505Comment: 16 pages, 11 figures, accepted for publication in ApJ.The interstellar medium in OIII-selected star-forming galaxies at $z\sim3.2$, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1709.06731Comment: 20 pages, 11 figures, Accepted for publication in ApJ.Enhanced Star Formation of Less Massive Galaxies in a Proto-Cluster at z=2.5, , , , , , , and . (2016)cite arxiv:1607.04040Comment: 5 pages, 3 figures, 1 table, accepted for publication in the ApJ Letters.