A super-Earth and a mini-Neptune around Kepler-59

@article{SaadOlivera2019ASA,
  title={A super-Earth and a mini-Neptune around Kepler-59},
  author={X. Saad-Olivera and Cintia F. Martinez and A Costa de Souza and Fernando V. Roig and David Nesvorn'y},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2019},
  volume={491},
  pages={5238-5247}
}
We characterize the radii and masses of the star and planets in the Kepler-59 system, as well as their orbital parameters. The star parameters are determined through a standard spectroscopic analysis, resulting in a mass of $1.359\pm 0.155\,M_\odot$ and a radius of $1.367\pm 0.078\,R_\odot$. The planetary radii obtained are $1.5\pm 0.1\,R_\oplus$ for the inner and $2.2\pm 0.1\,R_\oplus$ for the outer planet. The orbital parameters and the planetary masses are determined by the inversion of… Expand

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