Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for $\nu_e$ and $\nu_\mu$ charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncont...
IceCube, a cubic kilometer detector at the South Pole, is the largest neutrino telescope currently t...
The IceCube Neutrino Observatory has observed a diffuse flux of astrophysical neutrinos with energie...
The measurement of muon energy is critical for many analyses in large Cherenkov detectors, particula...
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volu...
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volu...
IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect ...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
Existing large-volume neutrino telescopes such as ANTARES and IceCube, as well as the future KM3NeT/...
The IceCube project has transformed 1 km3 of deep natural Antarctic ice into a Cherenkov detector. M...
IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. The main goal of IceCu...
The IceCube project has transformed 1 km3 of deep natural Antarctic ice into a Cherenkov detector. M...
As the energy of an incident neutrino cannot be accessed experimentally, muon neutrino energy spectr...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
IceCube, a cubic kilometer detector at the South Pole, is the largest neutrino telescope currently t...
The IceCube Neutrino Observatory has observed a diffuse flux of astrophysical neutrinos with energie...
The measurement of muon energy is critical for many analyses in large Cherenkov detectors, particula...
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volu...
Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volu...
IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect ...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
Existing large-volume neutrino telescopes such as ANTARES and IceCube, as well as the future KM3NeT/...
The IceCube project has transformed 1 km3 of deep natural Antarctic ice into a Cherenkov detector. M...
IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. The main goal of IceCu...
The IceCube project has transformed 1 km3 of deep natural Antarctic ice into a Cherenkov detector. M...
As the energy of an incident neutrino cannot be accessed experimentally, muon neutrino energy spectr...
Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections ar...
IceCube, a cubic kilometer detector at the South Pole, is the largest neutrino telescope currently t...
The IceCube Neutrino Observatory has observed a diffuse flux of astrophysical neutrinos with energie...
The measurement of muon energy is critical for many analyses in large Cherenkov detectors, particula...