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Improved modeling of in-ice particle showers for IceCube event reconstruction
The IceCube Collaboration
Chair of Experimental Physics with Cosmic Particles
Loyola University Chicago
Deutsches Elektronen-Synchrotron (DESY)
University of Canterbury
University of Wisconsin
Institute of Physics Bhubaneswar
Université Libre de Bruxelles
Niels Bohr Institutet
pro3dure medical GmbH
University of Delaware
Marquette University
Friedrich Alexander Universität Erlangen-Nürnberg
Broad Institute of Harvard University
University of Utah
RWTH Aachen University
South Dakota School of Mines and Technology
University of California, Irvine
Technical University of Munich
University of California at Berkeley
Ohio State University
Max-Planck-lnstitut für Kohlenforschung
Chalmers University of Technology
Uppsala University
University of Rochester
University of Maryland
University of Padova
University of Kansas
Humanoid Technologies Lab (H2T)
Johannes Gutenberg University
Georgia Institute of Technology
University of Adelaide
University of Münster
Drexel University
University of Nevada, Las Vegas
SUNY
Sungkyunkwan University
Massachusetts Institute of Technology
VUB Neurology
The Pennsylvania State University
Eberly College of Science
University of Alabama
Oskar Klein Centre
Centre Hospitalier Universitaire (CHU) Mont-Godinne
Michigan State University
Bergische Universität Wuppertal
Chiba-U
Southern University and A&M College
Academia Sinica Taipei
Humboldt-Universität zu Berlin
University of Wisconsin-Madison
Lawrence Berkeley National Laboratory
Chung-Ang University
Queen's University
University of Tokyo
Clark-Atlanta University
University of Texas at Arlington
University of Alberta
University of Geneva
Columbia University
Yale University
Mercer University at Macon
Ghent University
University of Alaska Anchorage
University of Oxford
University of Wisconsin-River Falls
Research output
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Keyphrases
IceCube
100%
Event Reconstruction
100%
Particle Showers
100%
Ice Particles
100%
Accurate Model
33%
Simplified Model
33%
Monte Carlo Simulation
33%
Angular Resolution
33%
Reconstruction-based
33%
High Energy
33%
Optical Properties
33%
Photomultiplier Tube
33%
Birefringence
33%
Charged Particles
33%
Fast Approximation
33%
Photoelectron Yield
33%
IceCube Neutrino Observatory
33%
Glacial Ice
33%
Cherenkov Light
33%
South Pole Ice
33%
Polycrystalline Structure
33%
Physics
Polycrystalline
100%
Photoelectron
100%
Birefringence
100%
Photomultiplier Tubes
100%
Optical Property
100%
Monte Carlo Method
100%
Observatory
100%
Charged Particle
100%