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SILVERRUSH. VIII. Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc at z~6-7: Strong Associations of Dusty Star-Forming Galaxies

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2019)cite arxiv:1902.09555Comment: 17 pages, 11 figures, Accepted for Publication in ApJ.
DOI: 10.3847/1538-4357/ab2cd5

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Empirical Modeling of the Redshift Evolution of the NII/H$\alpha$ ratio for Galaxy Redshift Surveys, , , , , , and . (2017)cite arxiv:1710.00834Comment: 14 pages, 10 figures, 1 table, submitted to ApJ.Dust Properties of CII Detected z $\sim$ 5.5 Galaxies: New HST/WFC3 Near-IR Observations, , , , , , , , , and . (2017)cite arxiv:1707.02980Comment: 9 pages, 3 figures, 1 table. Accepted for publication in The Astrophysical Journal.SILVERRUSH. VIII. Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc at z~6-7: Strong Associations of Dusty Star-Forming Galaxies, , , , , , , , , and 25 other author(s). (2019)cite arxiv:1902.09555Comment: 17 pages, 11 figures, Accepted for Publication in ApJ.Are high redshift Galaxies hot? - Temperature of z > 5 Galaxies and Implications on their Dust Properties, , , , , , , , and . (2017)cite arxiv:1708.07842Comment: 34 pages including Appendix, 18 figures (4 in Appendix), 5 tables (1 in Appendix). Accepted for publication in ApJ.