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Fig. 1.

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Schematic representation of the method used to compare X-ray and optical data for each temporal bin. The minimum and maximum optical fluxes allowed by the standard afterglow model assuming that there is a single break νopt < νb < νX are indicated by Fm,opt and FM,opt, respectively. We derived FX, Fopt, and the X-ray spectral slope from spectral analysis. Therefore, if Fm,opt < Fopt < FM,opt, we then considered that the optical counterpart is consistent with a single synchrotron spectrum, and we could derive νb. The blue line has no break, the orange line has νb = νX, and the green line has a break between the optical and X-ray bands. We note that our assumption here is that νm < νopt, and it is supported by the observation of βopt > 0 for all the analysed events (see Sect. 3.2) that exclude the case νb = νm.

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