During her Master's Thesis « Impact of the distortion of time on the galaxy angular power spectrum » she worked on forecasting the signal to noise ratio for the SKA experiment by considering the observation of two different populations of galaxies (bright and faint), with the goal of testing General Relativity at large scales of the Universe, under the supervision of Prof. C. Bonvin and Sveva Castello at the University of Geneva.
During her PhD studies, she will work on « Higher-order statistics for neutral hydrogen intensity mapping » as a member of the TITAN project.
