The activities of the Roma Tre Unit consisted in participation of polarimetric data interpretation and of theoretical modeling of polarization properties in accreting systems. In particular, spectra and polarization of the direct radiation from accretion disks around black holes have been studied taking into account the ionization state of the matter, as well as the polarization of reflected radiation from matter around a compact object when illuminated by thermal radiation. In addition, the polarization of the "torus" in Active Galactic Nuclei has been explored by using the MonteCarlo code SKIRT developed at the Ghent University.
IXPE data of Galactic accreting black hole binaries have also been studied and interpreted, highlighting the importance of polarimetry in the understanding of these systems.
| Name & Surname | Role | Effort (PM) |
|---|---|---|
| Prof. Giorgio Matt | Full professor - PI | 6.0 |
| Event | Date | Presenter | Contribution |
|---|---|---|---|
| ASI School on IXPE data analysis for general observers, Rome (I) | 19-23 February 2024 | Giorgio Matt | Invited lecture |
| Accretion Disks: the first 50 years, Bern (CH) | 17-21 June 2024 | Giorgio Matt | Invited talk |
| European Astronomical Society Annual Meeting, Padova (I) | 1-5 July 2024 | Giorgio Matt | Invited talk |
| AGN Polarimetry Research Symposium, Strasbourg (F) | 14-16 October 2024 | Giorgio Matt | Invited talk |
| Frontiers in X-ray polarimetry Academy, L'Aquila (I) | 7-11 April 2025 | Giorgio Matt | Invited lecture |
| Vasto Accretion Meeting 2025, Vasto (I) | 23-27 June 2025 | Giorgio Matt | Invited talk |