Signal extraction in atmospheric shower arrays designed for $\rm 200\,GeV-50\,TeV$ $\gamma$-ray astronomy
M. Senniappan, Y. Becherini, M. Punch, S. Thoudam, T. Bylund, G. Kukec, Mezek, J.-P. Ernenwein

TL;DR
This paper introduces SEMLA, a machine learning-based analysis method for atmospheric shower arrays, optimized for detecting gamma rays above 200 GeV, focusing on extragalactic sources like AGNs and GRBs.
Contribution
SEMLA is a novel four-stage machine learning approach that enhances gamma-ray signal extraction and background suppression in atmospheric shower array data.
Findings
SEMLA improves angular and energy resolution.
It effectively suppresses proton background.
Demonstrates adaptability to different experiments.
Abstract
We present the SEMLA (Signal Extraction using Machine Learning for ALTO) analysis method, developed for the detection of rays in the context of the ALTO wide-field-of-view atmospheric shower array R&D project. The scientific focus of ALTO is extragalactic -ray astronomy, so primarily the detection of soft-spectrum -ray sources such as Active Galactic Nuclei and Gamma Ray Bursts. The current phase of the ALTO R&D project is the optimization of sensitivity for such sources and includes a number of ideas which are tested and evaluated through the analysis of dedicated Monte Carlo simulations and hardware testing. In this context, it is important to clarify how data are analysed and how results are being obtained. SEMLA takes advantage of machine learning and comprises four stages: initial event cleaning (stage A), filtering out of poorly…
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