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Fig. 3.


Light curves of PKS 1510–089 of the flare night, JD 2457539. a: VHE γ-ray light curve from H.E.S.S. (red points) and MAGIC (green open squares). The binning is 28 min and 20 min for the H.E.S.S. and MAGIC light curves, respectively. The grey bars mark the systematic uncertainties. b: detected energies from Fermi-LAT above 1 GeV. The clustering of points in two bunches is a result of the orbital motion of the Fermi satellite. c: optical R-band light curve from ATOM showing individual exposures of about 8 min duration each.

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