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. 11

Comparison of the instrument response functions (effective area, angular resolution, energy bias, and energy resolution) between the current default tail-cut cleaning and the best candidate for the detection criterion, TIME4D_8. The blue shaded region indicates the energy range of interest for the detection criterion.

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