Recent Highlights from IceCube
arXiv:1311.6519 · doi:10.1007/s13538-014-0224-8
Abstract
The 1 km IceCube neutrino observatory was completed in December, 2010 and is taking data on cosmic-ray muons and neutrinos, extra-terrestrial neutrinos, and setting limits on a variety of exotic phenomena. This proceeding will cover recent IceCube results, with an emphasis on cosmic-rays and on searches for extra-terrestrial neutrinos, with a stress on results that were presented at the 2013 International Cosmic Ray Conference.
9 pages; plenary highlight talk presented at the 2013 Intl.Cosmic Ray Conf. The full collaboration author list is available at http://icecube.wisc.edu/collaboration/authors/current
References in corpus (14)
- Prompt neutrino fluxes from atmospheric charm
- Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube
- IceCube: An Instrument for Neutrino Astronomy
- Search for time-independent neutrino emission from astrophysical sources with 3 years of IceCube data
- Measurement of the Atmospheric flux in IceCube
- IceCube Search for Dark Matter Annihilation in nearby Galaxies and Galaxy Clusters
- Search for Point-Like Sources of Ultra-High Energy Neutrinos at the Pierre Auger Observatory and Improved Limit on the Diffuse Flux of Tau Neutrinos
- The IceCube Neutrino Observatory Part I: Point Source Searches
- PINGU Sensitivity to the Neutrino Mass Hierarchy
- The IceCube Neutrino Observatory Part IV: Searches for Dark Matter and Exotic Particles
- The IceCube Neutrino Observatory Part VI: Ice Properties, Reconstruction and Future Developments
- The IceCube Neutrino Observatory Part III: Cosmic Rays
- The IceCube Neutrino Observatory Part V: Neutrino Oscillations and Supernova Searches
- The IceCube Neutrino Observatory Part II: Atmospheric and Diffuse UHE Neutrino Searches of All Flavors
Cited by in corpus (4)
- Flavor revolution at ICECUBE horizons?
- Photopion Production in Black-Hole Jets and Flat-Spectrum Radio Quasars as PeV Neutrino Sources
- Signals of HE atmospheric muon decay in flight around the Sun's albedo versus astrophysical muon and tau neutrino traces in the Moon's shadow
- UHECR and GRB neutrinos: an incomplete revolution?