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 GRP 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.
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