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Rotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample (2014)

First Author: McQuillan A

Attributed to: Astrophysics and Planetary Science at Oxford 2013-16 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1402.5694

Publication URI: https://arxiv.org/abs/1402.5694

Type: Other