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Fig. A.1


Example lightcurves computed from the model described in Sect. 4.2 (full line: GeV emission; dashed line: TeV emission, taking into account γγ absorption). The orbital period and eccentricity of the binary system is indicated in the title of each plot. The lightcurves are normalised to the maximum value. The systems shown here are a random selection of the systems flagged as detected in Fig. 6. Periastron passage is at phase 0.

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