Left panel: relative instrumental flux of the approximately 161-day-long UBr binned data set of ε Sco. Middle panel: power density spectrum (in ppm²/μHz) of the binned (grey lines) and interpolated time series (black lines) along with a best global model fit (blue lines) and expected ν_max (vertical red lines). Right panel: squared autocorrelation function of the binned time series (black dots) and a best fit (red line).