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Evidence That the Occurrence Rate of Hot Jupiters around Sun-like Stars Decreases with Stellar Age

We investigate how the occurrence rate of giant planets (minimum mass > 0.3 M _Jup ) around Sun-like stars depends on the age, mass, and metallicity of their host stars. We develop a hierarchical Bayesian framework to infer the number of planets per star (NPPS) as a function of both planetary and st...

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Detalles Bibliográficos
Autores principales: Shota Miyazaki, Kento Masuda
Formato: Artigo
Lenguaje:Inglês
Publicado: IOP Publishing 2023-01-01
Colección:The Astronomical Journal
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Acceso en línea:https://doi.org/10.3847/1538-3881/acff71
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