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THE POPULATION OF LONG-PERIOD TRANSITING EXOPLANETS

  • Authors: Daniel Foreman-Mackey, Timothy D. Morton, David W. Hogg, Eric Agol, and Bernhard Schölkopf

2016 The Astronomical Journal 152 206.

  • Provider: AAS Journals

Caption: Figure 9.

Same as Figure 6, converted into the plane of planet mass and semimajor axis. Since the completeness function depends on the planet’s radius and not its mass, a probabilistic mass–radius relationship (Chen & Kipping 2016) was used to convert radius to mass.

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