Improving isotopic identification with \emph{INDRA} Silicon-CsI(\emph{Tl}) telescopes
O. Lopez, M. Parlog, B. Borderie, M.F. Rivet, G. Lehaut, G. Tabacaru,, L. Tassan-got, P. Pawlowski, E. Bonnet, R. Bougault, A. Chbihi, D., Dell'Aquila, J.D. Frankland, E. Galichet, D. Gruyer, M. La Commara, N. Le, Neindre, I. Lombardo, L. Manduci, P. Marini, J.C. Steckmeyer

TL;DR
This paper introduces an improved identification and calibration method called AME for Silicon-CsI(Tl) telescopes, enhancing the ability to determine atomic and mass numbers of nuclear reaction products, especially useful for radioactive beam experiments.
Contribution
The paper presents the AME method, which significantly improves isotopic identification accuracy over traditional techniques in nuclear detection using INDRA telescopes.
Findings
AME method outperforms traditional $\
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Enhanced isotope identification accuracy
Abstract
Profiting from previous works done with the \emph{INDRA} multidetector on the description of the light response of the CsI(\emph{Tl}) crystals to different impinging nuclei, we propose an improved identification-calibration procedure for Silicon-Cesium Iodide (Si-CsI) telescopes, namely an Advanced Mass Estimate (\emph{AME}) method. \emph{AME} is compared to the usual, % simple visual analysis of the corresponding two-dimensional map of type, by using \emph{INDRA} experimental data from nuclear reactions induced by heavy ions in the Fermi energy regime. We show that the capability of such telescopes to identify both the atomic and the mass numbers of light and heavy reaction products, can be quantitatively improved thanks to the proposed approach. This conclusion opens new possibilities to use \emph{INDRA} for…
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Taxonomy
TopicsParticle Detector Development and Performance · Astro and Planetary Science · Planetary Science and Exploration
