145 citations · 160 across the 7 of their papers we have counts for
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A Time-Variability Test for Candidate Neutrino Sources Observed with IceCube
Pranav Dave
Recent studies with IceCube have shown signs of a time-integrated flux of astrophysical neutrinos from point-like sources such as TXS 0506+056 and NGC 1068. Time-variability of thi…
Direction Reconstruction using a CNN for GeV-Scale Neutrinos in IceCube
Shiqi Yu
The IceCube Neutrino Observatory observes neutrinos interacting deep within the South Pole ice. It consists of 5,160 digital optical modules embedded within a cubic kilometer of ic…
A Three-dimensional Reconstruction of Cosmic Ray Events in IceCube
Xinhua Bai, Emily Dvorak, Dennis Soldin +1
The IceCube Neutrino Observatory at the geographic South Pole consists of two components, a km2 surface array IceTop and a km3 in-ice array between 1.5 and 2.5 km below the surface…
Report on Tests and Measurements of Hadronic Interaction Properties with Air Showers
H. P. Dembinski, J. C. Arteaga-Velázquez, L. Cazon +18
We present a summary of recent tests and measurements of hadronic interaction properties with air showers. This report has a special focus on muon density measurements. Several exp…
Measuring the Muon Content of Air Showers with IceTop
Javier G. Gonzalez
IceTop, the surface component of the IceCube detector, has been used to measure the energy spectrum of cosmic ray primaries in the range between 1.58 PeV and 1.26 EeV. It can also…
Disentangling the Air Shower Components Using Scintillation and Water Cherenkov Detectors
Javier G. Gonzalez, Markus Roth, Ralph Engel
We consider a ground array of scintillation and water Cherenkov detectors with the purpose of determining the muon content of air showers. The different response characteristics of…
Mass Composition Sensitivity of an Array of Water Cherenkov and Scintillation Detectors
Javier G. Gonzalez, Ralph Engel, Markus Roth
We consider a hybrid array composed of scintillation and water Cherenkov detectors designed to measure the cosmic ray primary mass composition at energies of about 1 EeV. We have d…