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Fig. 4

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Two subsets of transiting planet host stars (red symbols): solar type (top diagram) and early K-type (bottom diagram). Individual color indices and errors are used to constrain the (B − V) range of the simulated sample for each star and error bars were used to define the box to calculate the statistics (see text). Note that real data points are shown for simulated samples of a wider spectral range for convenience.

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