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Fig. 2.


(V,Ks) APM distribution of the 1141 TGAS F5V stars located at a distance modulus smaller than six. The red curve represents the fit of the distribution with three Gaussian functions of the same variance. In this case, the positions of the secondary and the tertiary Gaussian functions are smaller by 0.63 and 1.26 mag with respect to that of the primary Gaussian function.

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