Fig. 17

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Frequency of stars hosting JL planets (corrected for completeness) in individual associations as a function of association mass. Upper panel: masses as obtained by summing the mass of the member stars. Bottom panel: masses corrected for the selection along the galactic Y coordinate. Blue dots are associations with an age <50 Myr; orange squares are associations with a total mass >50 Myr. The open triangle represents the frequency of stars hosting JL planets from the RV surveys. We arbitrarily assumed a mass of 1000 M⊙ for the typical birthplace of stars in these surveys.
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