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Planet Population Statistics With Kepler Q1-Q16: Stellar Effective Temperature Dependence

Authors
Volume
225
Source
SETI Institute
License
Unknown

Abstract

We explore extrasolar planet population statistics and the dependence of planet occurrence rates on stellar effective temperature from analysis of the Kepler Q1-Q16 planet candidate sample. The analysis takes advantage of the recent work on the Q1-Q16 Kepler planet candidate sample, extensive Monte-Carlo transit signal injection and recovery tests of the Kepler Pipeline, and updates to the stellar parameters provided by the Kepler Stellar Working Group. Results focus of intermediate orbital periods, 50< Porb< 300 day, where ...

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