Fig. 12.
Three-planet candidate EPIC 211314705. Left panels: successively prewhitened BLS spectra, normalized to unity at each panel. The spectra are divided into 2000 bins and only the maxima are shown in each bin. Right panels: folded LCs for each component, zoomed on the transit. Continuous line shows the fit to our transit model. Relative fluxes are in [ppt].
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