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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.VIP: A Python package for high-contrast imaging., , , , , , , , , and 6 other author(s). J. Open Source Softw., 8 (81): 4774 (2023)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.