Introduction
My main research concerns the understanding and mitigation of stellar activity. Stellar surface phenomena (such as oscillations, granulation and active regions) can induce apparent radial velocity (RV) variations of several meters per second, mimicking or obscuring potential gravitationally induced planetary signals. Currently, I am investigating the impact of magnetic fields and granulation on spectral line distortions using Sun-as-a-star observations from the Paranal solar ESPRESSO Telescope (PoET).
Project title: Resolving and Solving Solar-type Activity with PoET
Funding scheme: Swiss National Science Foundation (SNSF) Postdoc.Mobility
Grant number: P500PT_230225
Learn More
Here you can find links and overviews of my publications, talks and posters.
