Open Access

Fig. 5

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Planetary initial mass function for different values of the primary mass (given at the top of each column) and different values of αD (indicated on the right). In each panel, 30 000 formation models have been considered. The y axis presents the fraction of resulting planets in a given mass bin. The solid black line gives the mass function of all planets, whereas the red dashed and blue dotted lines correspond to planets observable assuming respectively a 10 m/s and 1 m/s accuracy spectrograph.

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