Characterization of the HD 17156 planetary system

@article{Barbieri2009CharacterizationOT,
  title={Characterization of the HD 17156 planetary system},
  author={M. Barbieri and R. Alonso and S. Desidera and A. Sozzetti and A. Fiorenzano and J. Almenara and M. Cecconi and R. Claudi and D. Charbonneau and M. Endl and V. Granata and R. Gratton and G. Laughlin and B. Loeillet},
  journal={Astronomy and Astrophysics},
  year={2009},
  volume={503},
  pages={601-612}
}
Aims. To improve the parameters of the HD 17156 system (peculiar due to the eccentric and long orbital period of its transiting planet) and constrain the presence of stellar companions. Methods. Photometric data were acquired for 4 transits, and high precision radial velocity measurements were simultaneously acquired with SARG@TNG for one transit. The template spectra of HD 17156 was used to derive effective temperature, gravity, and metallicity. A fit of the photometric and spectroscopic data… Expand
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