Fig. 4

Residuals of our global modelling, unfolded and binned per 10 min intervals (top), folded with P = 8 h and binned per 5 min intervals (bottom). For the unfolded residuals the expected transit depth for a 2 R⊕ planet orbiting one of the two BD is shown as a red horizontal line, assuming a 0.1 R⊙ radius and the same brightness for both BDs. The same is done for the folded residuals, but assuming a 1 R⊕ planet.
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