Fig. 2

Lightcurves of PKS 2005-489 during the multi-wavelength campaign from May 22 to July 2, 2009 with observations by the Cherenkov telescope array H.E.S.S., the γ-ray space telescope Fermi, the X-ray satellites RXTE and Swift and the 75-cm optical telescope ATOM. For a better display, the u and uvw2 band data by Swift are shifted by ± 0.5 days. For the H.E.S.S., RXTE and Swift lightcurves a nightly binning was used and the Fermi/LAT lightcurve is shown in a 10-day binning.
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