Same as in Fig. 6, but for some selected models in Table 2. Left panels: comparison between two models that differ only by the presence (Run 4, solid blue line) or absence (Run 14, solid red line) of the accretion disk. The dotted, dashed, and dot-dashed lines indicate the contributions to the total emission from the shocked ejecta, the shocked disk material, and the shocked plasma from the CBM (EDE and RG wind), respectively. Right panels: comparison between two models that differ in the geometry and density of the EDE (Runs 3 and 4).