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Calibration of ultraviolet, mid-infrared and radio star formation rate indicators, , , , , , , , , и 5 other автор(ы). (2017)cite arxiv:1709.00183Comment: Accepted for publication in the Astrophysical Journal; 39 pages, 14 figures and 4 tables.The Subaru FMOS Galaxy Redshift Survey (FastSound). III. The mass-metallicity relation and the fundamental metallicity relation at $z\sim1.4$, , , , , , , , , и 6 other автор(ы). (2015)cite arxiv:1508.01512Comment: 14 pages, 10 figures, 2 tables, accepted for publication in PASJ.Synchronized Co-evolution between Supermassive Black Holes and Galaxies Over the Last Seven Billion Years as Revealed by the Hyper Suprime-Cam, , , , , , , , , и 4 other автор(ы). (2021)cite arxiv:2109.02751Comment: 17 pages, 6 figures, accepted by ApJ.A search for Ly-alpha emitters around a concentrated-region of strong Ly-alpha absorbers at z=2.3, , , , , , , , и . (2017)cite arxiv:1703.05756Comment: 15 pages, 15 figures, Accepted for publication to PASJ.First Data Release of the Hyper Suprime-Cam Subaru Strategic Program, , , , , , , , , и 97 other автор(ы). (2017)cite arxiv:1702.08449Comment: 33 pages, 19 figures. Draft paper to be submitted to PASJ special issue in a month. Data available at https://hsc-release.mtk.nao.ac.jp/.ALMA follows streaming of dense gas down to 40 pc from the supermassive black hole in NGC1097, , , , , , , , , и 7 other автор(ы). (2013)cite arxiv:1304.6722Comment: Accepted for Publication in the ApJ Letters.Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XIV. A Candidate Type-II Quasar at z=6.1292, , , , , , , , , и 6 other автор(ы). (2021)cite arxiv:2106.13807Comment: 15 pages, 8 figures, accepted for publication in the Astrophysical Journal.Active Galactic Nucleus Environments and Feedback to Neighboring Galaxies at $z\sim5$ Probed by Lyman-Alpha Emitters, , , , , и . (2017)cite arxiv:1705.04753Comment: 16 pages, 9 figures, Accepted for publication in ApJ.Subaru high-$z$ exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at $5.7 < z < 6.9$, , , , , , , , , и 29 other автор(ы). (2016)cite arxiv:1603.02281Comment: Submitted to 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.