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Future Prospects: Deep Imaging of Galaxy Outskirts using Telescopes Large and Small

, , , , , , , and . (2016)cite arxiv:1612.06415Comment: 27 pages, 10 figures, Invited review, Book chapter in Öutskirts of Galaxies", Eds. J. H. Knapen, J. C. Lee and A. Gil de Paz, Astrophysics and Space Science Library, Springer, in press.

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The evolution of metallicity and metallicity gradients from z=2.7-0.6 with KMOS3D, , , , , , , , , and 21 other author(s). (2016)cite arxiv:1603.01139Comment: submitted to ApJ.The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity, , , , , , , , , and 16 other author(s). (2014)cite arxiv:1406.6056Comment: 19 pages, 17 figures, Resubmitted to ApJ after responding to referee report. Information on ZFOURGE can be found at http://zfourge.tamu.edu.The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1411.0667Comment: 11 pages, 9 figures. Submitted to MNRAS, comments welcome. The official Illustris website can be found at http://www.illustris-project.org/.The Initial Mass Function in the Nearest Strong Lenses from SNELLS: Assessing the Consistency of Lensing, Dynamical, and Spectroscopic Constraints, , , , and . (2016)cite arxiv:1612.00065Comment: Submitted to ApJ.Extensive Globular Cluster Systems Associated with Ultra Diffuse Galaxies in the Coma Cluster, , , , , , , , , and . (2017)cite arxiv:1705.08513Comment: Submitted to ApJ Letters. The black and white panels of Figure 1 make the key point of the paper, hopefully.Spatially Resolved Stellar Kinematics of the Ultra-Diffuse Galaxy Dragonfly 44: II. Constraints on Fuzzy Dark Matter, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1905.10373Comment: 15 pages, 11 figures. Submitted to ApJ, comments are welcome!.On the Random Motion of Nuclear Objects in a Fuzzy Dark Matter Halo, , , , , , and . (2021)cite arxiv:2105.05268Comment: 20 pages, 9 figures, submitted to ApJ.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.First spectroscopic observations of the galaxies that reionized the Universe, , , , , , , , , and 23 other author(s). (2023)cite arxiv:2308.08540Comment: 29 pages, 7 figures, 2 tables.Pixel Color Magnitude Diagrams for Semi-Resolved Stellar Populations: The Star Formation History of Regions within the Disk and Bulge of M31, and . (2016)cite arxiv:1602.05580Comment: 11 pages, 9 figures, submitted to ApJ.