The Gaia spectroscopic catalogue of exoplanets and host stars

Open Access

Fig. 22

Vertical Galactic velocity dispersion as a function of planet radius (left panel) and planet mass (right panel). As in Fig. 21, two regimes of planet radius are shown in the right panel. Error bars show the uncertainty in the standard deviation estimated from $\sqrt{σ^{2} / 2 (n - 1)}$ $\sqrt{\sigma^2/2(n-1)}$ .

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