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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.

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The Stellar Initial Mass Function in Early-Type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients, , , , and . (2016)cite arxiv:1611.09859Comment: Submitted to ApJ. Figure 12 shows the average IMF as a function of radius. Figure 16 compares our results to dynamical and lensing constraints.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!.Ultra-diffuse and Ultra-compact Galaxies in the Frontier Fields Cluster Abell 2744, , , , , and . (2016)cite arxiv:1701.00011.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.A Globular Cluster Toward M87 with a Radial Velocity < -1000 km/s: The First Hypervelocity Cluster, , , , , , and . (2014)cite arxiv:1402.6319Comment: submitted to ApJL, comments welcome.The SLUGGS Survey: Breaking degeneracies between dark matter, anisotropy and the IMF using globular cluster subpopulations in the giant elliptical NGC 5846, , , , , and . (2014)cite arxiv:1401.1501Comment: 16 pages, 8 figures. Accepted for publication on MNRAS.