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- W2086141425 endingPage "112" @default.
- W2086141425 startingPage "112" @default.
- W2086141425 abstract "One of the persistent complications in searches for transiting exoplanets is the low percentage of the detected candidates that ultimately prove to be planets, which significantly increases the load on the telescopes used for the follow-up observations to confirm or reject candidates. Several attempts have been made at creating techniques that can pare down candidate lists without the need of additional observations. Some of these techniques involve a detailed analysis of light curve characteristics; others estimate the stellar density or some proxy thereof. In this paper, we extend upon this second approach, exploring the use of independently-calculated stellar densities to identify the most promising transiting exoplanet candidates. We use a set of CoRoT candidates and the set of known transiting exoplanets to examine the potential of this approach. In particular, we note the possibilities inherent in the high-precision photometry from space missions, which can detect stellar asteroseismic pulsations from which accurate stellar densities can be extracted without additional observations." @default.
- W2086141425 created "2016-06-24" @default.
- W2086141425 creator A5000903454 @default.
- W2086141425 creator A5001152995 @default.
- W2086141425 creator A5002640751 @default.
- W2086141425 date "2010-12-21" @default.
- W2086141425 modified "2023-09-23" @default.
- W2086141425 title "USING STELLAR DENSITIES TO EVALUATE TRANSITING EXOPLANETARY CANDIDATES" @default.
- W2086141425 cites W1582730379 @default.
- W2086141425 cites W1843141233 @default.
- W2086141425 cites W1849668091 @default.
- W2086141425 cites W1971588807 @default.
- W2086141425 cites W1983765941 @default.
- W2086141425 cites W1993424498 @default.
- W2086141425 cites W2000308837 @default.
- W2086141425 cites W2005523748 @default.
- W2086141425 cites W2005704923 @default.
- W2086141425 cites W2012825291 @default.
- W2086141425 cites W2014167557 @default.
- W2086141425 cites W2022875455 @default.
- W2086141425 cites W2024891964 @default.
- W2086141425 cites W2025166706 @default.
- W2086141425 cites W2026795906 @default.
- W2086141425 cites W2028032660 @default.
- W2086141425 cites W2030637050 @default.
- W2086141425 cites W2032631216 @default.
- W2086141425 cites W2033802794 @default.
- W2086141425 cites W2042167448 @default.
- W2086141425 cites W2044929779 @default.
- W2086141425 cites W2045010158 @default.
- W2086141425 cites W2048629276 @default.
- W2086141425 cites W2049260159 @default.
- W2086141425 cites W2055588986 @default.
- W2086141425 cites W2058803738 @default.
- W2086141425 cites W2059170734 @default.
- W2086141425 cites W2061825258 @default.
- W2086141425 cites W2063155255 @default.
- W2086141425 cites W2070313242 @default.
- W2086141425 cites W2083498569 @default.
- W2086141425 cites W2083922144 @default.
- W2086141425 cites W2086348127 @default.
- W2086141425 cites W2088434495 @default.
- W2086141425 cites W2091827517 @default.
- W2086141425 cites W2092470956 @default.
- W2086141425 cites W2093608992 @default.
- W2086141425 cites W2097690918 @default.
- W2086141425 cites W2100659549 @default.
- W2086141425 cites W2101755019 @default.
- W2086141425 cites W2102629003 @default.
- W2086141425 cites W2109652514 @default.
- W2086141425 cites W2111653408 @default.
- W2086141425 cites W2112467312 @default.
- W2086141425 cites W2116760677 @default.
- W2086141425 cites W2117311108 @default.
- W2086141425 cites W2126063541 @default.
- W2086141425 cites W2127054216 @default.
- W2086141425 cites W2132427241 @default.
- W2086141425 cites W2135453706 @default.
- W2086141425 cites W2137800231 @default.
- W2086141425 cites W2138382150 @default.
- W2086141425 cites W2141452174 @default.
- W2086141425 cites W2142220522 @default.
- W2086141425 cites W2151870432 @default.
- W2086141425 cites W2158425183 @default.
- W2086141425 cites W2161797103 @default.
- W2086141425 cites W2164547785 @default.
- W2086141425 cites W2170157299 @default.
- W2086141425 cites W2171872850 @default.
- W2086141425 cites W2596914018 @default.
- W2086141425 cites W3087610601 @default.
- W2086141425 cites W3099054713 @default.
- W2086141425 cites W3099138802 @default.
- W2086141425 cites W3099340235 @default.
- W2086141425 cites W3099358989 @default.
- W2086141425 cites W3100087551 @default.
- W2086141425 cites W3100595602 @default.
- W2086141425 cites W3101309813 @default.
- W2086141425 cites W3101354272 @default.
- W2086141425 cites W3101639305 @default.
- W2086141425 cites W3102050145 @default.
- W2086141425 cites W3102166740 @default.
- W2086141425 cites W3102252448 @default.
- W2086141425 cites W3102272550 @default.
- W2086141425 cites W3102514863 @default.
- W2086141425 cites W3103553886 @default.
- W2086141425 cites W3103849430 @default.
- W2086141425 cites W3104058054 @default.
- W2086141425 cites W3104429002 @default.
- W2086141425 cites W3105143697 @default.
- W2086141425 cites W3105597706 @default.
- W2086141425 cites W3105798469 @default.
- W2086141425 cites W3106087517 @default.
- W2086141425 cites W3121564285 @default.
- W2086141425 cites W3124789757 @default.
- W2086141425 cites W3125839459 @default.
- W2086141425 cites W3126055082 @default.
- W2086141425 cites W4205128532 @default.
- W2086141425 cites W4214859324 @default.