Fig. 2
Comparison of the Teff, log g, and [Fe/H] we derived by spectroscopy with the ones derived photometrically by Huber et al. (2014) for the 37 targets listed in Table B.2. Open and filled circles are for stars hotter and cooler than the Sun (respectively). The log g of the giant host KOI-5976 is not displayed here for the sake of clarity in the plot.
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.