Advisor: Anne Lohfink
This project introduces students to high-energy astrophysics through the analysis of X-ray spectra from an active galactic nucleus (AGN). The student will use archival observations from major X-ray observatories to investigate the physical processes occurring near an accreting supermassive black hole. Tasks include reducing and fitting X-ray spectral data, identifying key features such as power-law continua, soft excess emission, and Fe K-alpha lines, and exploring how these components relate to accretion physics and the structure of the inner accretion flow.
The student will gain experience with standard astrophysical analysis tools, statistical model fitting, and the interpretation of observational signatures of black hole activity. Results from the project will help improve our understanding of how energy is generated and released in AGN environments.