Flare frequency distributions for the flares recovered in our original (black) and denoised (red) samples. The FFDs are separated into simple flares (top left), individual components of complex flares (bottom left), flares on partially convective stars (top middle), flares on fully convective stars (bottom middle), and the full flare samples (top right). Bottom right: Comparison between the simple flares (blue) and individual complex flare components (orange) recovered from the denoised light curves (bottom right). The solid lines indicate linear fits to the double-logarithmic FFD, extrapolated into regimes not directly observed.