TOI-148 light curves (top) and RVs (bottom) phased to the companion’s orbital period. The red lines in the upper plot show the best-fit transit model to each photometry data set from our EXOFASTv2 analysis described in Sect. 3.4.1. In the lower plot the red line shows the best-fit Keplerian model to the RVs from our EXOFASTv2 analysis.
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.