A schematic diagram of our model’s setup. A hot corona, as in lamppost geometry, is located at height h above the SMBH of mass M and spin a. The warm corona is positioned on top of an accretion disk. The incident flux coming from the hot corona is reprocessed in the warm corona, which is then detected by the observer. The r_in and r_out are the integration limits for our model. We compute the vertical structure using TITAN with the input parameters depicted in the warm corona panel; Γ – photon index, ξ – ionization parameter, N_H – column density, n_H – gas number density, Q – internal heating, and T_BB – the temperate of blackbody radiation from an underlying disk.