Fig. 5.
Fast intra-night variability observed in the VHE band on 13 June (left panel) and 1 July (right panel) 2016. The light curves above 300 GeV are constructed with a fixed time-binning of 10 min. Green dashed curve: fit with the function given in Eq. (3); solid red curve: fit with the function given in Eq. (4). See the figure legend for the rise and decay times inferred from the fit. The blue dashed line represents the steady flux of the Crab Nebula above 300 GeV, shown for comparison purposes.
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