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Fig. 2
Light curve of the integral γ-ray flux above 100 GeV during the 2005–2007 MAGIC observing period. The dashed blue line corresponds to the fit result of a linear function to the data points, with a reduced χ2/d.o.f. = 5.66/11 and an average flux of (5.06 ± 0.77) × 10-12 s-1 cm-2.
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