Periodogram of the light curve of Kepler-1705 after removal of the 3.08d candidate. Top: BLS periodogram on the first 12 quarters in red, on the full dataset in black. Bottom: RIVERS periodogram on the full dataset. The peaks around 9.03d and 11.3d have a non-zero width, implying that subsequent frames had a high confidence from the model. Examples ofriver diagrams for each of these peaks are given in Fig. 7.