SOPHIE velocimetry of Kepler transit candidates: a joint photometric, spectroscopic and dynamical analysis of the Kepler-117 system

G. Bruno (1) , J. -M. Almenara (1) , S. C. C. Barros (1) , A. Santerne , R. F. Díaz (1) , M. Deleuil (1) , C. Damiani (1) , A. S. Bonomo , I. Boisse (1) , F. Bouchy (1) , G. Hébrard (2, 3) , G. Montagnier (2, 3)

1 LAM - Laboratoire d'Astrophysique de Marseille
2 OHP - Observatoire de Haute-Provence
3 IAP - Institut d'Astrophysique de Paris

We present the analysis of the multi-planetary system Kepler-117, which is part of our program of observations of Kepler planets. This system is composed of a ~ 30 M_Earth planet in a ~ 19 days orbit and a ~ 2 M_J planet orbiting in ~ 51 days. Both the orbits have low eccentricity. The planets are not close to an exact low-order mean motion resonance, but exhibit significant transit timing variations (TTVs) nevertheless. We perform a combined Markov Chain Monte Carlo fit on all the available data: the Kepler photometry, the TTVs, the radial velocities we obtained with SOPHIE/OHP and the stellar parameters. The prime result is that the modelling of the TTVs allows to increase the precision on the system parameters which are not constrained by the radial velocities alone.

Domaines: Planète et Univers [physics]

G. Bruno, J. -M. Almenara, S. C. C. Barros, A. Santerne, R. F. Díaz, et al.. SOPHIE velocimetry of Kepler transit candidates: a joint photometric, spectroscopic and dynamical analysis of the Kepler-117 system. The Space Photometry Revolution - CoRoT Symposium 3, 2015, à renseigner, Unknown Region. p. 471-476., ⟨10.1051/epjconf/201510106014⟩. ⟨insu-03581047⟩