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Fig. 10.

image

Large separation as a function of the mixed-mode density. Stars analysed in Sect. 3 are in blue, stars in common with Kuszlewicz et al. (2019a) are in green, stars in common with Corsaro et al. (2017) are in black, stars with planet candidate(s) are in red, and stars with confirmed planet(s) are in yellow.

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