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  Exoplanet Populations beyond Kepler

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

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Item Permalink: https://hdl.handle.net/21.11116/0000-0005-D2B6-0 Version Permalink: https://hdl.handle.net/21.11116/0000-0005-D2B7-F
Genre: Conference Paper

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https://ui.adsabs.harvard.edu/abs/2019AAS...23322705P (Any fulltext)
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 Creators:
Pascucci, Ilaria1, Author
Mulders, Gijs1, Author
Fernandes, Rachel1, Author
Gould, Andrew1, Author
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1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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 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.

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 Dates: 2019
 Publication Status: Issued
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Title: American Astronomical Society Meeting Abstracts #233
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Start-/End Date: 2019

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Title: American Astronomical Society Meeting Abstracts #233
Source Genre: Proceedings
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