Example light curves of RR Lyrae stars and LPV in the data. For each band we show the valid FoV transits, as well as variability-rejected FoV transits (number in parentheses, data plotted with crosses). In most cases, two FoV transits occur within the 6 h spin period, causing indistinguishable overlapping points in the left panels. Some outliers are not flagged in the exported data (see e.g., the G_RP light curve of the RRc and RRd example); these transits were removed in the more strict outlier rejection used in the SOS Cep and RRL module, as mentioned in Sect. 4.1.