Using full waveform readout with a 9 ns peak-aligned integration window reduces noise and extends reconstructed image lengths for H.E.S.S. I, improving simulated effective area at low energies and promising similar gains at high energies.
Bernl\"ohr, Simulation of Imaging Atmospheric Cherenkov Telescopes with CORSIKA and sim\_telarray, Astropart
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Sensitivity Improvements of Very-High-Energy Gamma-Ray Detection with the Upgraded H.E.S.S. I Cameras using Full Waveform Processing
Using full waveform readout with a 9 ns peak-aligned integration window reduces noise and extends reconstructed image lengths for H.E.S.S. I, improving simulated effective area at low energies and promising similar gains at high energies.