Fig. 9

Light curve of PKS 2155-304 of the second flare observed by MAGIC and H.E.S.S. in the night of July 29 − 30, 2006. The flux is shown above an energy of 400 GeV. The MAGIC data (red points) are binned in 10 min intervals while the H.E.S.S. data (gray points) use four minute intervals. The red and the gray area represent the time spans when the MAGIC and the H.E.S.S. spectra shown in Fig. 6 are derived, respectively. The black arrow shows the time when Chandra observed the source.
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