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First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift

, , , , , , , , and . (2021)cite arxiv:2103.15862Comment: 11pages, 3 figures, to be submitted to PRL.

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First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift, , , , , , , , and . (2021)cite arxiv:2103.15862Comment: 11pages, 3 figures, to be submitted to PRL.A map of the universe, , , , , , , and . (2003)Gas Loss in Simulated Galaxies as They Fall into Clusters, , and . (2014)cite arxiv:1405.0537Comment: 9 pages, 4 figures, in press of PNAS.The Most Massive Distant Clusters: Determining Omega and sigma_8, and . (1998)cite arxiv:astro-ph/9803277 Comment: 14 pages, 4 Postscript figures, ApJ in press.The Seventh Data Release of the Sloan Digital Sky Survey, , , , , , , , , and 194 other author(s). The Astrophysical Journal Supplement Series, 182 (2): 543 (2009)Dark matter universe. Proceedings of the National Academy of Sciences, 112 (40): 12243--12245 (Oct 6, 2015)The Sloan Digital Sky Survey Quasar Lens Search. V. Final Catalog from the Seventh Data Release, , , , , , , , , and 6 other author(s). (2012)cite arxiv:1203.1087Comment: 42 pages, 2 figures, 6 tables, accepted for publication in AJ; see http://www-utap.phys.s.u-tokyo.ac.jp/~sdss/sqls/ for supplemental information.