Fig. 3
Illustration of difficulties in SW data processing on the case of DM And. The upper panel shows raw data. The change in amplitude of this star caused by the Blazko effect is apparent. The detail shows the night HJD 2 453 256, where the vertical shift between data coming from various cameras is demonstrated. The distribution of the positions of the star on the chip in x and y directions during the whole observation period are shown in the bottom part of this figure.
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