Seminar around 3 axis :

1. Searching for giant planets by radial velocities, around Main Sequence massives stars (Spectral type A or F). First occurence rate estimation.
2. Searching for giant planets by radial velocities around young stars and near imaging targets.
3. Modelisation of a solar type star’s magnetic activity and impact on the radial velocities.

Seminar by Simon Borgniet, Institut de Planétologie et d’Astrophysique de Grenoble, France.