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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.

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The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes, , , , , , , , , and 10 other author(s). (2017)cite arxiv:1706.02704Comment: 11 pages, 8 figures. Submitted for publication in A&A.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.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.The Taipan Galaxy Survey: Scientific Goals and Observing Strategy, , , , , , , , , and 30 other author(s). (2017)cite arxiv:1706.01246Comment: Submitted to PASA; 28 pages, 17 figures, 2 tables.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.