Fig. 2
Differential photometry (GJ 338 B–GJ 338 A) light curves obtained with the LCO and SNO telescopes. First and second panels: first photometric observing season covering a time interval of 22 days; third panel: light curve for the second observing season covering 87 days of continuous monitoring; and fourth and fifth panels: last observing season spanning 50 days. With the exception of the third panel, all photometry is artificially set to a mean value of zero magnitude.
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