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IceCube Collaboration, S. Shefali, Rasha Abbasi, Markus Ackermann et autres
The prototype station of the Surface Array Enhancement at the IceCube Neutrino Observatory has been taking data in its final design since 2023. This station is part of the planned extension within the footprint of the existing surface array, IceTop. One station …
IceCube-Gen2 Collaboration, Rasha Abbasi, Markus Ackermann, Jenni Adams et autres
IceCube-Gen2 is a proposed neutrino observatory at the South Pole that will build on the success of IceCube and will also serve as a unique detector for cosmic-ray air showers. Analogous to the IceTop surface array over IceCube’s deep optical detector, IceCube-Gen2 …
IceCube Collaboration, Rasha Abbasi, Markus Ackermann, Jenni Adams et autres
IceTop, the km$^2$ surface array of the IceCube Neutrino Observatory at the South Pole, is sensitive to air showers of all primary particles, including gamma rays. In particular, in the PeV energy range, the combination of IceTop and IceCube’s deep optical detector …
IceCube Collaboration, Tista Mukherjee, Rasha Abbasi, Markus Ackermann et autres
The IceCube Neutrino Observatory actively participates in multimessenger follow-ups of gravitational-wave (GW) events. With the release of the Gravitational-Wave Transient Catalogue (GWTC)-2.1 and -3, the sub-threshold GW event information from the third observation run of the LIGO-Virgo-KAGRA (LVK) detectors is publicly available. …
IceCube Collaboration, Rasha Abbasi, Markus Ackermann, Jenni Adams et autres
The IceCube Neutrino Observatory, situated at the geographic South Pole, comprises both a surface component, IceTop, and a deep in-ice component. This unique setup allows for simultaneous measurements of low-energy (∼GeV) and high-energy (≳400GeV) muons generated in cosmic-ray air showers. The correlation …
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