Spectral energy distribution of the emission predicted by our model for a generic binary with a system inclination of 30°. The results are shown for the sampled orbital phases (grey) and their average (black). The average spectral distribution is further split into the individual radiative processes: synchrotron (green) and inverse Compton attenuated by γγ -absorption (orange). Inferior (dashed red, ϕ = 0) and superior conjunction (dashed blue, ϕ = 0.5) emissions are highlighted.