Feature Selection Techniques for CR Isotope Identification with the AMS-02 Experiment in Space
Marta Borchiellini, Leandro Mano, Fernando Bar\~ao, Manuela Vecchi

TL;DR
This paper compares machine learning feature selection methods for improving background reduction in cosmic ray isotope identification using the AMS-02 detector, demonstrating that Random Forest outperforms physics-driven approaches.
Contribution
It introduces and evaluates automated feature selection algorithms, particularly Random Forest, for enhancing particle identification accuracy in space-based cosmic ray experiments.
Findings
Random Forest achieved the best background reduction performance.
Machine learning feature selection outperformed physics-driven methods.
Improved isotope identification accuracy in AMS-02 data analysis.
Abstract
Isotopic composition measurements of singly charged cosmic rays (CR) provide essential insights into CR transport in the Galaxy. The Alpha Magnetic Spectrometer (AMS-02) can identify singly charged isotopes up to about 10 GeV/n. However, their identification presents challenges due to the small abundance of CR deuterons compared to the proton background. In particular, a high accuracy for the velocity measured by a ring-imaging Cherenkov detector (RICH) is needed to achieve a good isotopic mass separation over a wide range of energies. The velocity measurement with the RICH is particularly challenging for isotopes due to the low number of photons produced in the Cherenkov rings. This faint signal is easily disrupted by noisy hits leading to a misreconstruction of the particles' ring. Hence, an efficient background reduction process is needed to ensure the quality of the…
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