A Unified Treatment of Kepler Occurrence to Trace Planet Evolution. I. Methodology
We present Kepler exoplanet occurrence rates for planets between 0.5 and 16 R _⊕ and between 1 and 400 days. To measure occurrence, we use a nonparametric method via a kernel density estimator and use bootstrap random sampling for uncertainty estimation. We use a full characterization of completenes...
I tiakina i:
| Ngā kaituhi matua: | , , |
|---|---|
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2023-01-01
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| Rangatū: | The Astronomical Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-3881/acebc8 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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