SOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

@article{Santerne2015SOPHIEVO,
  title={SOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period},
  author={A. Santerne and C. Moutou and M. Tsantaki and F. Bouchy and G. H'ebrard and V. Adibekyan and J. Almenara and L. Amard and S. Barros and I. Boisse and A. Bonomo and G. Bruno and B. Courcol and M. Deleuil and O. Demangeon and R. D'iaz and T. Guillot and M. Havel and G. Montagnier and A. Rajpurohit and J. Rey and N. Santos},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2015}
}
While giant extrasolar planets have been studied for more than two decades now, there are still some open questions such as their dominant formation and migration process, as well as their atmospheric evolution in different stellar environments. In this paper, we study a sample of giant transiting exoplanets detected by the Kepler telescope with orbital periods up to 400 days. We first defined a sample of 129 giant-planet candidates that we followed up with the SOPHIE spectrograph (OHP, France… Expand
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