Direct imaging of exoplanets
Directly image faint planet orbiting bright stars is particularly challenging due to the enormous flux ratio and small separation between them. The goal of my instrumental research is to develop optical and image processing methods to make the first image of an Earth-like planet a reality. In parallel, I specialized in the analysis of young exoplanetary systems to understand the late stages of planetary system formation.
My research complementary integrates instrumental development and observational studies. As astronomical instruments grow in complexity, maximizing their potential requires instrumentation expertise, and the insights gained from on-sky observations are essential for shaping future instrumental advancements.
Publications:

