  The star HD 147379 was recently announced as a host of a low-mass exoplanet
by Reiners et al. (2017). That announcement included a discussion of the
possible detection of a periodic signal in the radial velocity observations
around 21.1 days, which was interpreted as rotational variability of the star.
We have examined the light curve of this star as observed by the KELT transit
survey, and we find a significant periodic signal in the light curve of 22.0064
days, supporting the interpretation of Reiners et al. (2017) of the rotational
variation of the star.
