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Fig. 4.


VHE SEDs during the nights of highest flux: 13 June, 14 June, and 1 July 2016 (from top to bottom). The black circle and red square markers represent the observed and the EBL-deabsorbed spectra, respectively. These spectra have been unfolded with the instrument response function of MAGIC. The absorption by the EBL has been corrected via the model of Franceschini et al. (2008).

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