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The Stellar Initial Mass Function of Ultra-Faint Dwarf Galaxies: Evidence for IMF Variations with Galactic Environment

, , , , , , , , , , and . (2013)cite arxiv:1304.7769Comment: 10 pages, 5 figures, accepted to ApJ.

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High-resolution spectroscopy of the transiting planet host star TrES-1, , , , , , , , and . ASTROPHYSICAL JOURNAL, 616 (2): L167--L170 (December 2004)The Stellar Initial Mass Function of Ultra-Faint Dwarf Galaxies: Evidence for IMF Variations with Galactic Environment, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1304.7769Comment: 10 pages, 5 figures, accepted to ApJ.The Brightest Young Star Clusters in NGC 5253, , , , , , , , , and 36 other author(s). (2015)cite arxiv:1508.04476Comment: 67 pages; 11 figures; 7 tables. Accepted for publication in the Astrophysical Journal.The Metastable Dynamo Model of Stellar Rotational Evolution. Astrophys. J., (Jul 18, 2014)A Lack of Planets in 47 Tucanae from a ITALHubble Space Telescope/ITAL Search, , , , , , , , , and 14 other author(s). The Astrophysical Journal, 545 (1): L47--L51 (December 2000)BWT-based efficient shape matching., , , , , and . SAC, page 1079-1085. ACM, (2007)Development and application of an image acquisition system for characterizing sow behaviors in farrowing stalls., , , and . Comput. Electron. Agric., (2019)