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The integrated stellar content of dark matter halos

, , , , , , , , and . (2011)cite arxiv:1109.0010Comment: Submitted to ApJ. 16 Pages, 11 Figures. Comments Welcome.

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Signatures of unresolved binaries in stellar spectra: implications for spectral fitting, , , , , , , and . (2017)cite arxiv:1709.03983Comment: Submitted to MNRAS. 7 pages, 5 figures.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.A High Stellar Velocity Dispersion and ~100 Globular Clusters for the Ultra Diffuse Galaxy Dragonfly 44, , , , , , , , and . (2016)cite arxiv:1606.06291Comment: Submitted to ApJ Letters.Nebular Continuum and Line Emission in Stellar Population Synthesis Models, , , and . (2016)cite arxiv:1611.08305Comment: 35 pages, 29 figures.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.The SINFONI Nearby Elliptical Lens Locator Survey: Discovery of two new low-redshift strong lenses and implications for the initial mass function in giant early-type galaxies, , and . (2015)cite arxiv:1503.02661Comment: Accepted for publication in MNRAS.Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster, , , , , and . (2014)cite arxiv:1410.8141Comment: Submitted to ApJ Letters. To illustrate how big and fluffy these things are we made a graphic comparing the one with ACS imaging (Fig 4) to several well-known galaxies, if they were at the same distance: http://www.astro.yale.edu/dokkum/coma_udgs/sizes.jpg.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.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.A Simple Model for Quasar Demographics, and . (2012)cite arxiv:1208.3198Comment: 11 pages, 10 figures, submitted to ApJ.