Gaussian with variable background best-fits to the spectral time series of the two candidates in Fig. 3. This has been done both before and after stellar pulsationremoval. The best linear fit of the centroid time series and corresponding 1σ- and 2σ-confidence intervals areshown in blue and light blue. The bottom row shows the best-fit amplitude time series.
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.