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Very Compact Dense Galaxy Overdensity with \delta ~ 130 Identified at z ~ 8: Implications for Early Protocluster and Cluster-Core Formation

, , and . (2015)cite arxiv:1509.01751Comment: 8 pages, 10 figures.

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Ly$\alpha$ Emitters with Very Large Ly$\alpha$ Equivalent Widths, EW$_0$(Ly$\alpha$) $200-400$ \AA, at $z2$, , , , , , , , and . (2016)cite arxiv:1611.00777Comment: Accepted for publication in MNRAS; 23 pages with 16 figures.Faint LAEs near z>4.7 CIV absorbers revealed by MUSE, , , , , , , and . (2020)cite arxiv:2001.04453Comment: 21 pages, 23 figures, 3 tables. Submitted to MNRAS.Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 $łe$ z $łe$ 7.0, , , , , , , , , and 37 other author(s). (2019)cite arxiv:1908.07910Comment: ApJ, in press. arXiv admin note: text overlap with arXiv:1803.01861.3D Distribution Map of HI Gas and Galaxies Around an Enormous Ly$\alpha$ Nebula and Three QSOs at $z=2.3$ Revealed by the HI Tomographic Mapping Technique, , , , , , , , , and 15 other author(s). (2019)cite arxiv:1910.02962Comment: 14 pages, 7 figures, submitted to ApJ.SILVERRUSH. XIII. A Catalog of 20,567 Ly$\alpha$ Emitters at $z=2-7$ Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys, , , , , , , , , and 6 other author(s). (2023)cite arxiv:2305.08921Comment: 38 pages, 19 Figures, 5 Tables. Accepted for publication in ApJS.SILVERRUSH. XI. Intensity Mapping for Lya Emission Extending over $100-1000$ comoving kpc around $z\sim2-7$ LAEs with Subaru HSC-SSP and CHORUS Data, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2108.09288.Gaia 400,894 QSO constraint on the energy density of low-frequency gravitational waves, , , and . (2021)cite arxiv:2105.04039Comment: Submitted to Physical Review D.Average Metallicity and Star Formation Rate of Lya Emitters Probed by a Triple Narrow-Band Survey, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1105.2824 Comment: 17 pages, 16 figures. Submitted to ApJ.Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1704.06050Comment: 14 pages, 11 figures.Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program Survey, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1704.06051Comment: 21 pages, 9 figures, 6 tables, submitted to PASJ special issue.