A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals
To date, only 18 exoplanets with radial velocity (RV) semi-amplitude <2 m s<sup>−1</sup> have had their masses directly constrained. The biggest obstacle to RV detection of such exoplanets is variability intrinsic to stars themselves, e.g. nuisance signals arising from surface magneti...
| Principais autores: | , , , , , , , , , , , , , , , , , , , , , , , , |
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| Formato: | Journal article |
| Idioma: | English |
| Publicado em: |
Oxford University Press
2021
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