Multiwavelength SED of Cygnus X-3 during the main γ-ray events (non-simultaneous data) and the leptonic model “B” (see main text). Spectral components of the model are the BB emission from the disk (blue short-dashed line), IC scattering of the soft photons from the accretion disk (green solid line), and IC scattering of the soft stellar photons (red solid line). The global SED model curve is indicated by a black solid line. For a detailed description of the datasets, see caption to Fig. 3.