Fig. 3.
Observed multiwavelength lightcurves zoomed in on Night 2. (a) H.E.S.S. lightcurve derived above an energy threshold of 100 GeV in run-wise time bins. (b) Fermi-LAT lightcurve integrated above 100 MeV in 3 h bins. (c) HE γ-ray photon index measured with Fermi-LAT in 3 h bins. (d) Swift-XRT lightcurve integrated between 2 and 10 keV for individual pointings. (e) Optical R band lightcurve from ATOM and SMARTS for individual pointings. In all panels, only statistical error bars are shown, while horizontal bars mark the observation time.
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