I am leading the development of the DISK-WIND model. This sophisticated state-of-the-art model has been initially developed by Stuart Sim (Sim et al. 2008, Sim et al. 2010a, 2010b) and revisited by Gabriele Matzeu (Matzeu et al. 2022) through 2.5D Monte Carlo radiative transfer code for calculating Compton-thick disc-wind spectra.
The DISK-WIND model takes also into account the effects of radiation transmitted through the wind, including scattering and reflected emission (Fe K included) from the flow and hence I will be able to map the full physics of the system.
X–Ray Accretion Disk-wind Emulator