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Fig. 5


Fit χ2 distributions for the average spectrum of the February–March flare of 1ES 1011+496 for the five models tested. PWL in blue (dashed line), LP in red (solid line), EPWL in green (dot-dash line) and ELP in pink (dotted line) and SEPWL in light blue (long dash-dot line). The LP red line is overlapping ELP pink line. Notice how all curves converge after reaching the minimum.

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