I obtained my PhD at Paris-Saclay University in France. Then, I worked at CAMK Toruń and at the department of astrophysics and planetary science at Villanova University in the USA. My research focuses on the detection and characterisation of binary and multiple stellar systems using ground- and space-based telescopes such as Solaris, Kepler, K2, and TESS. As a member of the Araucaria Project team, I aim to contribute to the study of close binary stars through the analysis of their eclipse timing variations.