A Fast Algorithm for Muon Track Reconstruction and its Application to the ANTARES Neutrino Telescope
ANTARES collaboration: J.A. Aguilar, I. Al Samarai, A. Albert, M., Andre, M. Anghinolfi, G. Anton, S. Anvar, M. Ardid, A.C. Assis Jesus, T., Astraatmadja, J-J. Aubert, R. Auer, B. Baret, S. Basa, M. Bazzotti, V., Bertin, S. Biagi, C. Bigongiari, C. Bogazzi, M. Bou-Cabo

TL;DR
This paper introduces a rapid and robust algorithm for reconstructing upward-going muon tracks induced by neutrinos, enabling real-time event discrimination and supporting multi-messenger astrophysics with the ANTARES telescope.
Contribution
The paper presents a novel fast reconstruction algorithm specifically designed for real-time processing in neutrino telescopes like ANTARES.
Findings
Algorithm achieves high accuracy in muon track reconstruction.
Effective discrimination between neutrino-induced and atmospheric muon events.
Validated performance through Monte Carlo simulations and ANTARES data comparisons.
Abstract
An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained in ANTARES data.
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