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• W1995709019 abstract "The planet occurrence rate for multiple stars is important in two aspects. First, almost half of stellar systems in the solar neighborhood are multiple systems. Second, the comparison of the planet occurrence rate for multiple stars to that for single stars sheds light on the influence of stellar multiplicity on planet formation and evolution. We developed a method of distinguishing planet occurrence rates for single and multiple stars. From a sample of 138 bright (KP <13.5) Kepler multi-planet candidate systems, we compared the stellar multiplicity rate of these planet host stars to that of field stars. Using dynamical stability analyses and archival Doppler measurements, we find that the stellar multiplicity rate of planet host stars is significantly lower than field stars for semi-major axes less than 20 AU, suggesting that planet formation and evolution are suppressed by the presence of a close-in companion star at these separations. The influence of stellar multiplicity at larger separations is uncertain because of search in- completeness due to a limited Doppler observation time baseline and a lack of high resolution imaging observation. We calculated the planet confidence for the sample of mutlti-planet candidates, and find that the planet confidences for KOI 82.01, KOI 115.01, KOI 282.01 and KOI 1781.02 are higher than 99.7% and thus validate the planetary nature of these four planet candidates. This sample of bright Kepler multi-planet candidates with refined stellar and orbital parameters, planet confidence estimation, and nearby stellar companion identification offers a well-characterized sample for future theoretical and observational study." @default.
• W1995709019 created "2016-06-24" @default.
• W1995709019 creator A5014289107 @default.
• W1995709019 creator A5016310949 @default.
• W1995709019 creator A5043091074 @default.
• W1995709019 creator A5085464247 @default.
• W1995709019 date "2014-02-05" @default.
• W1995709019 modified "2023-10-16" @default.
• W1995709019 title "INFLUENCE OF STELLAR MULTIPLICITY ON PLANET FORMATION. I. EVIDENCE OF SUPPRESSED PLANET FORMATION DUE TO STELLAR COMPANIONS WITHIN 20 AU AND VALIDATION OF FOUR PLANETS FROM THE<i>KEPLER</i>MULTIPLE PLANET CANDIDATES" @default.
• W1995709019 cites W1561585778 @default.
• W1995709019 cites W1663574567 @default.
• W1995709019 cites W1678481872 @default.
• W1995709019 cites W1838917337 @default.
• W1995709019 cites W1921943311 @default.
• W1995709019 cites W1983029350 @default.
• W1995709019 cites W1989901708 @default.
• W1995709019 cites W1994657652 @default.
• W1995709019 cites W1995945864 @default.
• W1995709019 cites W2005927107 @default.
• W1995709019 cites W2006224949 @default.
• W1995709019 cites W2010823783 @default.
• W1995709019 cites W2029167399 @default.
• W1995709019 cites W2031043816 @default.
• W1995709019 cites W2031513034 @default.
• W1995709019 cites W2039452097 @default.
• W1995709019 cites W2039658765 @default.
• W1995709019 cites W2060278163 @default.
• W1995709019 cites W2061333070 @default.
• W1995709019 cites W2061759127 @default.
• W1995709019 cites W2070154021 @default.
• W1995709019 cites W2070508637 @default.
• W1995709019 cites W2070606946 @default.
• W1995709019 cites W2076490016 @default.
• W1995709019 cites W2083250837 @default.
• W1995709019 cites W2086813500 @default.
• W1995709019 cites W2097671484 @default.
• W1995709019 cites W2100421763 @default.
• W1995709019 cites W2100833883 @default.
• W1995709019 cites W2102694518 @default.
• W1995709019 cites W2107230547 @default.
• W1995709019 cites W2107596287 @default.
• W1995709019 cites W2112231378 @default.
• W1995709019 cites W2132117032 @default.
• W1995709019 cites W2134476621 @default.
• W1995709019 cites W2136512068 @default.
• W1995709019 cites W2145612370 @default.
• W1995709019 cites W2153298099 @default.
• W1995709019 cites W2153544248 @default.
• W1995709019 cites W2158674056 @default.
• W1995709019 cites W2159133042 @default.
• W1995709019 cites W2160161987 @default.
• W1995709019 cites W2162651321 @default.
• W1995709019 cites W2163377996 @default.
• W1995709019 cites W2164694167 @default.
• W1995709019 cites W2166675540 @default.
• W1995709019 cites W2177545076 @default.
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• W1995709019 cites W2947592794 @default.
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• W1995709019 doi "https://doi.org/10.1088/0004-637x/783/1/4" @default.
• W1995709019 hasPublicationYear "2014" @default.
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