Fig. 4.
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Effect of the combined absorption at 100 GeV by a population of 1000 O-type stars. Left panel: Example of a light curve (sub-sample) attenuation factor evolution due to flickering absorption on the bulk radiation field in the central Galactic region. Right panel: Power density spectrum of the flickering absorption for one realization of a 999-day light curve (green empty markers) and average over all simulated light curves (black solid markers).
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