The Pacific Ocean Neutrino Experiment (P-ONE) is a planned multi-cubic-kilometer neutrino telescope in the Northeast Pacific Ocean off Vancouver Island, British Columbia. Its primary goal is to detect high-energy neutrinos, offering key insights into cosmic ray origins and acceleration mechanisms. Building on two successful pathfinder missions, the collaboration, in partnership with Ocean...
The IceCube neutrino observatory is a Cherenkov light detector in the Antarctic ice sheet, at the South Pole. Composed of a cubic kilometer of detector volume instrumented with over 5000 photo-multiplier tubes, it is the largest neutrino detector in the world, observing neutrinos incident from all directions. Having collected data for 13 years in its current configuration, the IceCube...
The IceCube Neutrino Observatory detects Cherenkov light from neutrino interactions in the Antarctic ice. Despite more than a decade of operation, distinguishing electromagnetic and hadronic showers remains a persistent challenge. Accurately identifying electromagnetic showers provides a charged-current electron-neutrino-rich sample, which plays a pivotal role in Neutrino Mass Ordering...
The P-ONE neutrino observatory is a proposed water Cherenkov detector for the study of astrophysical neutrinos in the TeV-PeV energy range. Upon completion the detector will contain tens of thousands of photo-multiplier tubes in a cubic-kilometer array located on the seafloor at Cascadia basin, just off the shore of Vancouver Island. To accurately reconstruct the type, energy, and direction of...
ARGO is a future dark matter direct-detection experiment based on a liquid argon (LAr) target that is proposed to be built at SNOLAB in the next decade. ARGO will produce leading sensitivity to heavy dark matter searches above 50 GeV/c2. It will also have excellent sensitivity to detect core-collapse supernova neutrinos and produce high-precision measurements of solar neutrinos at and above...
