Spectra obtained from self-consistent simulations for epochs P03 a); P18 b); IG02 c); and IG07 d). The X-ray data from Swift/XRT, RXTE/PCA, and RXTE/HEXTE (panels a) and b)) or INTEGRAL/ISGRI (panels c) and d)) are shown with blue, red, and green symbols, respectively. Swift/UVOT data, corrected for interstellar reddening, are plotted with magenta symbols for E(B−V) = 0.34 and with yellow symbols for E(B−V) = 0.45. The solid black line is the spectrum obtained from self-consistent simulations and it consists of three major components: (1) the emission from the hot medium produced by synchrotron radiation and Comptonization of disk and synchrotron seed photons with an additional contribution from bremsstrahlung emission (dashed lines); (2) the contribution of irradiated accretion disk (dot-dashed lines); and (3) the Compton reflection hump taken from the best fitting sc compps model fit (dotted lines).