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SUMMARY:Studying of SuperFGD response using stopped cosmic muons
DTSTART;VALUE=DATE-TIME:20261027T162500Z
DTEND;VALUE=DATE-TIME:20261027T163000Z
DTSTAMP;VALUE=DATE-TIME:20261021T015513Z
UID:indico-contribution-6479@cern.ch
DESCRIPTION:Speakers: Nataliya Skrobova ()\nThe SuperFGD (Super Fine-Grain
 ed Detector) is a part of the ND280 near\n detector complex for the T2K an
 d Hyper-Kamiokande experiments. The\n SuperFGD is a fully active and highl
 y granular scintillator neutrino\n detector. It consists of approximately 
 2 million scintillation cubes\,\n which allow for the reconstruction of pa
 rticles traveling in all\n directions. A good understanding of the SuperFG
 D response is crucial\n for detailed Monte Carlo simulations and systemati
 cs estimation for\n further physics analyses. This poster covers the selec
 tion of\n atmospheric muons stopped inside the sensitive volume of the det
 ector\,\n including their decays. Muons were selected by applying geometri
 cal\n constraints and searching for subsequent electrons or positrons. The
 \n reconstructed spectrum of the Michel e-/e+ is useful as another source\
 n of energy scale determination. Reconstruction of Compton electrons\n fol
 lowing positron annihilation allows for the evaluation of the\n SuperFGD e
 ffective low energy threshold\n\nhttps://indico.particle.mephi.ru/event/62
 6/contributions/6479/
LOCATION:Sevastopol hotel Conference Hall 1
URL:https://indico.particle.mephi.ru/event/626/contributions/6479/
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