Presentation

As a Ph.D. student in astrophysics, I am utilizing high-resolution stellar spectroscopy to explore the Galactic chemical evolution of various elements. My research has so far concentrated on determining fluorine in open clusters, with the objective to establish the most comprehensive and homogeneous database of fluorine abundances across the Galactic disk.

The spectra were obtained using the high-resolution GIANO-B instrument, which operates at the 3.58-meter Galileo National Telescope (TNG) in the near-infrared wavelength range. For analyzing the spectra and deriving stellar parameters, I use the Python version of Spectroscopy Made Easy (PySME). Currently, my study is expanding to include additional elements and clusters. During 2025, I will be at the Nordic Optical Telescope (NOT) on the island of La Palma, following their studentship programme: https://www.not.iac.es/general/studentships/

Publications