Speaker
Description
The ICARUS detector will operate at shallow depth and therefore it will be exposed to the full surface flux of cosmic rays. This poses a problematic background to the electron neutrino appearance analysis. A direct way to suppress this background is to surround the cryostat with a detector capable of tagging incident cosmic muons with high efficiency (~95\%). A cosmic ray tagger (CRT) consists of an organic plastic scintillator, wavelength-shifting fibers, readout by silicon photomultipliers and multi-anode photomultiplier tubes. The installation of the ICARUS Cosmic Ray Tagger (CRT) side wall hardware is complete and commissioning of the system is underway. In this talk, I will present the status of the integration of the CRT readout and analysis of first data from the commissioned side CRT system.
Working group | WG6 |
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