Rotation periods of exoplanet host stars

@article{Simpson2010RotationPO,
  title={Rotation periods of exoplanet host stars},
  author={E. K. Simpson and Sallie L. Baliunas and Gregory W. Henry and Christoph Pfrommer Canadian Institute for Theoretical Astrophysics and University of Southampton and Queen's University of Belfast and Tennessee State University},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={408},
  pages={1666-1679}
}
The stellar rotation periods of 10 exoplanet host stars have been determined using newly analysed Ca II H&K flux records from the Mount Wilson Observatory and Str¨ omgren b, y photometric measurements from Tennessee State University’s automatic photometric telescopes at the Fairborn Observatory. Five of the rotation periods have not previously been reported, with that of HD 130322 very strongly detected at Prot = 26.1 ± 3.5 d. The rotation periods of five other stars have been updated using new… 

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