Fig. B.1
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We performed our GMM analysis on various planet samples, from top, all planet candidates and confirmed planets from our sample (A), planet candidates (B) and likely planets (C) obtained from our Triceratops run (Giacalone & Dressing 2020) and confirmed planets from the NASA exoplanet archive (D) with number of planets in parentheses. As it is shown, including the planet candidates not only increases the planet sample; it also helps to reduce the error bars on the peaks and minima and precisely locate the radius valley.
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