Fig. 2
White-colored light curve obtained with GTC/OSIRIS. From top to bottom are i) raw flux time series divided by exposure time, ii) raw light curve (i.e., normalized target-to-reference flux ratios), iii) light curve corrected for systematics, and vi) best-fit residuals. The red line shows the best-fit model. The gap at around +40 min is due to missing raw files in the data archive.
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