With construction halfway complete, IceCube is already the most sensitive neutrino telescope ever built. A rearrangement of the final holes of IceCube with increased spacing has been discussed recently to optimize the high energy sensitivity of the detector. Extending this baseline with radio and acoustic instrumentation in the same holes could further improve the high energy response. The goal would be both to detect events and to act as a pathfinder for hybrid detection, towards a possible larger hybrid array. Simulation results for such an array are presented here
An upgrade of the present IceCube surface array (IceTop) with scintillation detectors and possibly r...
The IceCube Neutrino Observatory is a cubic-kilometer Cherenkov telescope buried in the icesheet at ...
The IceCube Neutrino Observatory is a cubic kilometer scale detector deployed in the antarctic ice, ...
In 2013 the IceCube collaboration announced the discovery of a cosmic neutrino flux up to PeV energi...
The IceCube Neutrino Observatory has discovered a diffuse astrophysical flux up to 10 PeV and is now...
At the IceCube Neutrino Observatory, a Surface Array Enhancement is planned, consisting of 32 hybrid...
The IceCube Neutrino Observatory at the South Pole has measured the diffuse astrophysical neutrino f...
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice ...
The next generation of the IceCube Neutrino Observatory, IceCube-Gen2, will constitute a much larger...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
IceTop, the surface array of the IceCube Neutrino Observatory at the geographic South Pole, serves a...
Since the construction of IceCube was completed in 2010/11, the observatory has delivered several ou...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
Multi-detector observations of individual air showers are critical to make significant progress to p...
The IceCube Neutrino Observatory located at the geographic South Pole is composed of two detectors. ...
An upgrade of the present IceCube surface array (IceTop) with scintillation detectors and possibly r...
The IceCube Neutrino Observatory is a cubic-kilometer Cherenkov telescope buried in the icesheet at ...
The IceCube Neutrino Observatory is a cubic kilometer scale detector deployed in the antarctic ice, ...
In 2013 the IceCube collaboration announced the discovery of a cosmic neutrino flux up to PeV energi...
The IceCube Neutrino Observatory has discovered a diffuse astrophysical flux up to 10 PeV and is now...
At the IceCube Neutrino Observatory, a Surface Array Enhancement is planned, consisting of 32 hybrid...
The IceCube Neutrino Observatory at the South Pole has measured the diffuse astrophysical neutrino f...
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice ...
The next generation of the IceCube Neutrino Observatory, IceCube-Gen2, will constitute a much larger...
Abstract: Astrophysical neutrinos in the EeV range (particularly those generated by the interaction ...
IceTop, the surface array of the IceCube Neutrino Observatory at the geographic South Pole, serves a...
Since the construction of IceCube was completed in 2010/11, the observatory has delivered several ou...
Due to the low flux of ultrahigh energetic neutrinos induced in interactions of cosmic rays with the...
Multi-detector observations of individual air showers are critical to make significant progress to p...
The IceCube Neutrino Observatory located at the geographic South Pole is composed of two detectors. ...
An upgrade of the present IceCube surface array (IceTop) with scintillation detectors and possibly r...
The IceCube Neutrino Observatory is a cubic-kilometer Cherenkov telescope buried in the icesheet at ...
The IceCube Neutrino Observatory is a cubic kilometer scale detector deployed in the antarctic ice, ...