Fig. 5
Light curve in different energy bands during the 2007 observation campaign. From top to bottom: VHE γ-ray flux above 150 GeV as measured by MAGIC, RXTE PCA flux in the 2–10 keV range (Chatterjee et al. 2008), KVA R-band observations and REM infrared observations. For the MAGIC light curve the night by night flux is calculated assuming that 3C 279 always emits γ-rays above 150 GeV.
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