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No difference in orbital parameters of RV-detected giant planets between 0.1-5 au in single vs multi-stellar systems

, , , , , , , , , , and . (2017)cite arxiv:1704.02326Comment: accepted to AJ; 34 pages, 9 figures, 16 tables, including 7 tables with online supplemental data.

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No difference in orbital parameters of RV-detected giant planets between 0.1-5 au in single vs multi-stellar systems, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1704.02326Comment: accepted to AJ; 34 pages, 9 figures, 16 tables, including 7 tables with online supplemental data.Characterizing K2 Candidate Planetary Systems Orbiting Low-Mass Stars II: Planetary Systems Observed During Campaigns 1-7, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1703.07416Comment: 26 pages, 13 figures, 4, tables. Submitted to ApJ. The associated follow-up observations and vetting plots will be posted to the ExoFOP-K2 website (https://exofop.ipac.caltech.edu/k2/).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.Constraints on the Atmospheric Circulation and Variability of the Eccentric Hot Jupiter XO-3b, , , , , , , , , and 2 other author(s). (Jul 8, 2014)