Exoplanet research has reshaped our understanding of planetary systems, uncovering a vast diversity in their architectures and evolution. My work centers on the synergy between Radial Velocities (RVs) and Transit Timing Variations (TTVs) to investigate planetary dynamics, mass distributions, and formation pathways.

I’ve studied tidal orbital decay in close-in planets, explored methods for detecting exomoons, and performed joint RV+TTV analyses to constrain the orbital configurations of multi-planet systems. To address the challenges of observing young stars, I also apply advanced stellar activity mitigation techniques to extract planetary signals from noisy RV datasets.

As a collaborator of the CHEOPS science team, I am currently working on the characterization of resonant multi-planet systems and the study of dynamical phenomena such as apsidal precession in eccentric hot Jupiters to probe their internal structure and tidal dissipation properties (OrbitalWALTZ program, PI: Leonardi, 190 orbits, PR150089).

In parallel, within the GAPS collaboration, I focus on characterizing long-period sub-Neptunes, prime targets for atmospheric studies, and on measuring the masses of planets around young stars, combining photometric follow-up with extreme-precision HARPS-N RV campaigns to understand their composition and early evolution.