Comparison of periods returned by our method with spot periods from previously studied Kepler stars.
|KIC||8 429 280||7 985 370||7 765 135||5 110 407|
|dΩ / Ωeq||0.049||0.080||0.067||0.053d|
Notes.The periods closest to P1out (P2out) are called P1closest (P2closest).
Periods from a seven-spots fit (Frasca et al. 2011).
Periods from seven-spots fit (Fröhlich et al. 2012).
Periods from nine-spots fit (Fröhlich et al. 2012).
Period and DR coefficient from Roettenbacher et al. (2013).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.