Spectral energy distribution of the non-thermal emission predicted in our model for LS 5039 with the total emission power reduced by a factor of 2 for both INFC phase intervals covered in our simulation. Here, we show synchrotron emission in blue and IC emission in green. Results for the first full orbit are shown as solid lines and those for the second full orbit as dotted lines. Additionally, the outer-gap model is shown in dashed orange. The observational data are the same as in Fig. 7.