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The Radius Distribution of Planets Around Cool Stars

, and . (2013)cite arxiv:1303.3013Comment: 13 pages, 10 figures, published in ApJ.

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The Radius Distribution of Planets Around Cool Stars, and . (2013)cite arxiv:1303.3013Comment: 13 pages, 10 figures, published in ApJ.Friends of Hot Jupiters. IV. Stellar companions beyond 50 AU might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1606.07102Comment: accepted for publication in ApJ; 23 pages including 9 figures and 6 tables.Three statistically validated K2 transiting warm Jupiter exoplanets confirmed as low-mass stars, , , , , , , , , and 4 other author(s). (2017)cite arxiv:1708.08455Comment: Posted on the arXiv for comments from the community. Current version includes corrections following first referee report. To be resubmitted to ApJ Letters.The initial physical conditions of Kepler-36 b & c, and . (Nov 23, 2015)