A novel approach to optimizing the image cleaning performance of Imaging Atmospheric Cherenkov Telescopes: Application to a time-based cleaning for H.E.S.S.

Open Access

Fig. 4

Left: size distribution for gamma MC and off-data events, with corresponding fitted function for the default tail-cut candidate 0916NN2. Right: fitted function for gamma MC (solid line) and off-data (dashed line) for different example cleanings (shown in different colors).

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