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Data analysis in the ICARUS (SBN FD) Cosmic Ray Tagging system

Conference ·
DOI:https://doi.org/10.2172/2282439· OSTI ID:2282439
When a cosmic ray particle collides with the upper atmosphere, it creates a shower of particles that transverse down to the Earth’s surface. These cosmogenic particles provide a challenging background in neutrino experiments. The Short Baseline Neutrino (SBN) Program is composed of three Liquid Argon Time Projection Chambers (LArTPCs) that will help us understand the elusive neutrino. Together with a Cosmic Ray Tagger (CRT) system, the ICARUS detector serves as the Far Detector in the SBN Program. The CRT surrounds the detector medium and tags incoming particles allowing us to combat the high flux of comic rays we experience at ICARUS. In this poster, I will show some of the first data analyses done with the fully commissioned CRT system, including studies using CRT timing information and CRT hit reconstruction.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Contributing Organization:
ICARUS
DOE Contract Number:
AC02-07CH11359
OSTI ID:
2282439
Report Number(s):
FERMILAB-POSTER-22-029-ND; oai:inspirehep.net:2743460
Country of Publication:
United States
Language:
English

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