Exoplanet Populations beyond Kepler

Pascucci, Ilaria; Mulders, Gijs; Fernandes, Rachel; Gould, Andrew

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Exoplanet Populations beyond Kepler

MPS-Authors

Pascucci, Ilaria
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mulders, Gijs
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Fernandes, Rachel
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gould, Andrew
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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https://ui.adsabs.harvard.edu/abs/2019AAS...23322705P
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Citation

Pascucci, I., Mulders, G., Fernandes, R., & Gould, A. (2019). Exoplanet Populations beyond Kepler. In American Astronomical Society Meeting Abstracts #233.

Cite as: https://hdl.handle.net/21.11116/0000-0005-D2B6-0

Abstract

We present a framework to extend exoplanet occurrence rates beyond the semi-major axis probed by Kepler. Using this framework we find that the most common planet inside the snowline scales with the mass of the central star and it is ~3-10 times less massive than the one outside, as identified via microlensing. By extending the Kepler statistics with RV data, we also find evidence for a drop in the giant planet occurrence rate beyond the snowline. We conclude by discussing the implications of these results on future missions.