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Fig. 9
Transits of CoRoT-25 (left) and CoRoT-26 (right). Top panels: light curve folded by the orbital period (black crosses) and the transit model computed from the most probable value of the different parameters (red line). Bottom panels: residuals after subtraction of this model; the red line is a smoothing over 30 points.
This figure is made of several images, please see below:
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