Abstract
The contribution of identification methods to charge systematic errors for heavy-ion Δ E– E multidetector telescopes is studied. In this context, a new identification method is presented in two versions: the first uses one Δ E value and second uses all Δ E data for each event. A Monte Carlo simulation of the response of a solid-state telescope to an isotropic flux of heavy ions is used to test the systematic errors induced by this method and by the Seamster and range methods.
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