Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full
Autocorrelation Sample

Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample

We analyzed 3 years of data from the Kepler space mission to derive rotation periods of main-sequence stars below 6500 K. Our automated autocorrelation-based method detected rotation periods between 0.2 and 70 days for 34,030 (25.6%) of the 133,030 main-sequence Kepler targets (excluding known eclip...

書目詳細資料
Main Authors:	McQuillan, A, Mazeh, T, Aigrain, S
格式:	Journal article
語言:	English
出版:	Institute of Physics Publishing 2014

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