Open Access

Fig. 3.

image

Phase-folded eclipses and radial velocities for SB2 stars in our sample. For both eclipses, the processed Kepler data is shown in light blue dots and the solid black line corresponds to the fit from JKTEBOP. For the radial velocities, red squares (resp. green diamonds) represent the observed radial velocity of the giant (resp. the companion) and the solid red line (resp. the green line) indicates the fit from JKTEBOP.

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