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A Gap in the Mass Distribution for Warm Neptune and Terrestrial Planets

  • Authors: David J. Armstrong, Farzana Meru, Daniel Bayliss, Grant M. Kennedy, and Dimitri Veras

2019 The Astrophysical Journal Letters 880 L1.

  • Provider: AAS Journals

Caption: Figure 3.

Top: two-component GMM fit to the P1 sample with contours showing weighted log probabilities of the combined model. Contour levels are from 2.5 to 8.5 with a spacing of 1 in log probability. The red crosses mark the component means. Bottom: distribution of ΔBIC over 10,000 bootstrap trials when varying the number of components. Blue: ﹩1\to 2﹩, orange: ﹩2\to 3﹩, and green: ﹩3\to 4﹩.

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