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Cosmic Ray Background Removal With Deep Neural Networks in SBND / SBND Collaboration
In liquid argon time projection chambers exposed to neutrino beams and running on or near surface levels, cosmic muons and other cosmic particles are incident on the detectors while a single neutrino-induced event is being recorded. In practice, this means that data from surface liquid argon time projection chambers will be dominated by cosmic particles, both as a source of event triggers and as the majority of the particle count in true neutrino-triggered events. [...]
arXiv:2012.01301; FERMILAB-PUB-20-641-ND.- 2021-08-24 - 17 p. - Published in : Front. Artif. Intell. 4 (2021) 649917 Fulltext: frai-04-649917 - PDF; 2012.01301 - PDF; fermilab-pub-20-641-nd - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server (fulltext available)

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