Correction method applied to MC simulated LST images affected by clouds
arxiv(2024)
Abstract
We present the results of a preliminary study of a correction method applied
to the Imaging Atmospheric Cherenkov Telescope images affected by clouds. The
studied data are Monte Carlo simulations made with CORSIKA, imitating the very
high energy events registered by the Large-Sized Telescopes, a type of
telescope within the future Cherenkov Telescope Array. We implement the cloud
correction method in the ctapipe/lstchain analysis framework. The correction is
based on a simple geometrical model of the emission. We show the effect of the
correction method on the image parameters and the stereo-reconstructed shower
parameters.
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