Fig. 2.
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VHE differential energy spectrum of BL Lac for 2015 June between 15 and 28 (blue) and on 2015 June 15 (red). The spectra have been corrected for extragalactic background light absorption using the model of Domínguez et al. (2011). The spectra are fitted with PL and LP models and are shown with black solid lines. The yellow band shows the uncertainty of the fit.
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