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GOLDRUSH. III. A Systematic Search of Protoclusters at $z\sim4$ Based on the $>100\,deg^2$ Area, , , , , , , , , и 8 other автор(ы). (2017)cite arxiv:1708.09421Comment: 11 pages, 8 figures, accepted for publication in PASJ special issue.A fundamental metallicity relation for galaxies at z = 0.84 - 1.47 from HiZELS, , , , , , , , и . (2013)cite arxiv:1309.0506Comment: Accepted for publication in MNRAS.Direct evidence for Ly$\alpha$ depletion in the protocluster core, , , , , , , , , и 1 other автор(ы). (2017)cite arxiv:1702.00100Comment: 6 pages, 4 figures, accepted for publication in MNRAS Letter.An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115, , , , , , , , , и 21 other автор(ы). (2017)cite arxiv:1704.03868Comment: ApJ submitted. Comments welcome.Bulge-forming galaxies with an extended rotating disk at z~2, , , , , , , , , и 17 other автор(ы). (2016)cite arxiv:1608.05412Comment: 10 pages, 5 figures, 2 tables, submitted to ApJ.SXDF-ALMA 2-arcmin^2 Deep Survey: Stacking of Rest-Frame Near-Infrared Selected Objects, , , , , , , , , и 17 other автор(ы). (2016)cite arxiv:1609.08772Comment: accepted for publication in ApJ.Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4, , , , , , , , , и 15 other автор(ы). (2017)cite arxiv:1704.06050Comment: 14 pages, 11 figures.The nature of H$\alpha$-selected galaxies along the huge cosmic web at z=0.4 revealed by Subaru Hyper Suprime-Cam survey, , , , , , , , , и 6 other автор(ы). (2017)cite arxiv:1704.05979Comment: 15 pages, 13 figures, submitted to PASJ for publication in the HSC-SSP special issue.Do Galaxy Morphologies Really Affect the Efficiency of Star Formation during the Phase of Galaxy Transition?, , , , , , , , , и 4 other автор(ы). (2019)cite arxiv:1903.03505Comment: 16 pages, 11 figures, accepted for publication in ApJ.Predicting dust extinction properties of star-forming galaxies from H-alpha/UV ratio, , , , , , , , , и 1 other автор(ы). (2015)cite arxiv:1507.04092Comment: 14 pages, 14 figures, Accepted for publication in MNRAS.