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The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1606.00043Comment: 210 pages, 91 figures. Exposure draft. Appendices to the Detailed Science Case can be found at http://mse.cfht.hawaii.edu/docs/.

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The Detailed Science Case for the Maunakea Spectroscopic Explorer: the Composition and Dynamics of the Faint Universe, , , , , , , , , and 167 other author(s). (2016)cite arxiv:1606.00043Comment: 210 pages, 91 figures. Exposure draft. Appendices to the Detailed Science Case can be found at http://mse.cfht.hawaii.edu/docs/.Tracing the cosmic web, , , , , , , , , and 20 other author(s). (2017)cite arxiv:1705.03021Comment: 24 pages, 8 figures, 2 tables. Submitted to MN. Comments Welcome.Paper 1: The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies, , , , , , , , , and 34 other author(s). (2023)cite arxiv:2303.03556Comment: 23 pages, submitted to ApJ.Webb's PEARLS: Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results, , , , , , , , , and 73 other author(s). (2022)cite arxiv:2209.04119Comment: Submitted to AJ, comments welcome. We ask anyone who uses our public PEARLS (NEP TDF) data to refer to this overview paper.xGASS: The Impact of Photometric Bulges on the Scatter of HI Scaling Relations, , , and . (2019)cite arxiv:1909.10202Comment: 22 pages, 13 figures, accepted for publication in the Monthly Notices of the Royal Astronomical Society.Galaxy And Mass Assembly (GAMA): Stellar mass growth of spiral galaxies in the cosmic web, , , , , , , , , and 9 other author(s). (2016)cite arxiv:1601.03391Comment: 16 pages, 15 figures (including one 3D figure that can be interacted with when reading the PDF in Adobe Reader). Accepted for publication in MNRAS on January 13th, 2016.The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux, , , , , , and . (2023)cite arxiv:2301.03699.Measures of Galaxy Environment I - What is "Environment"?, , , , , , , , , and 12 other author(s). (2011)cite arxiv:1109.6328 Comment: 14 pages, 9 figures, 1 table, accepted to MNRAS.DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories, , , , , , , , and . (2022)cite arxiv:2210.13696Comment: 25 pages, 20 figures. Accepted for publication in MNRAS.From rest-frame luminosity functions to observer-frame colourdistributions: tackling the next challenge in cosmological simulations, , , , and . (2020)cite arxiv:2003.11258Comment: 21 pages, 18 figures. Submitted to MNRAS.