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Galaxy And Mass Assembly (GAMA): Stellar mass growth of spiral galaxies in the cosmic web

, , , , , , , , , , , , , , , , , , and . (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.

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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.The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization, , , , , , , , , and 24 other author(s). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.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.KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies, , , , , , , , , and 6 other author(s). (2020)cite arxiv:2006.10777Comment: 10 pages, 10 figures, submitted to A&A, comments welcome.