Fig. 2
CCFs of the diluted eclipsing binaries as a function of radial velocities. Blue and green dot-lines display the observed CCFs and the dashed red lines are the multi-Gaussian fit to the CCFs. The two lower panels are the SDSS finding charts (FC) of KOI-51.01 and KOI-667.01, which present several stars located within 20′′ × 10′′.
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