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Nature, ISSN 0028-0836, 02/2018, Volume 554, Issue 7693, p. 554
Journal Article
by Scholten, Olaf and van den Berg, Aiaan and Las Cumbres Observatory Grp and ATCA Australia Telescope and LIGO Sci Collaboration & Virgo and KU Collaboration and GROUND and RIMAS RATIR and AGILE Team and ASKAP Australian SKA Pathfinder and IPN Collaboration and LOFAR Collaboration and Salt Grp and VINROUGE Collaboration and Nordic Optical Telescope and MAXI Team and Fermi GBM and Fermi Large Area Telescope and J-GEM and IceCube Collaboration and BOOTES Collaboration and Pi Sky Collaboration and Pan-STARRS and LWA Long Wavelength Array and SKA South Africa MeerKAT and CALET Collaboration and AstroSat Cadmium Zinc Telluride and HAWC Collaboration and GROWTH JAGWAR CALTECH and ATLAS and ePESSTO and DFN Desert Fireball Network and Insight-Hxmt Collaboration and Texas Tech Univ and MASTER Collaboration and TZAC Consortium and Dark Energy Camera GW-EM and GRAWITA GRAvitational Wave and INTERGRAL and Toros Transient Robotic Observat and Chandra Team McGill Univ and H E S S Collaboration and Swift Collaboration and Pierre Auger Collaboration and OzGrav DWF Deeper Wider Faster and IKI-GW Follow-up Collaboration and Euro VLBI Team and High Time Resolution Universe and ANTARES Collaboration and DLT40 Collaboration and ALMA Collaboration and The 1M2H Team and MWA Murchison Widefield Array and The Insight-HXMT Collaboration and The MAXI Team and The Swift Collaboration and The Fermi Large Area Telescope Collaboration and GROND and TOROS: Transient Robotic Observatory of the South Collaboration and Texas Tech University and OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations and MWA: Murchison Widefield Array and GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations and INTEGRAL and RIMAS and RATIR and Pi of the Sky Collaboration and The Chandra Team at McGill University and LWA: Long Wavelength Array and The DLT40 Collaboration and DFN: Desert Fireball Network and LIGO Scientific Collaboration and Virgo Collaboration and ASKAP: Australian SKA Pathfinder and AstroSat Cadmium Zinc Telluride Imager Team and The BOOTES Collaboration and The Pierre Auger Collaboration and ATCA: Australia Telescope Compact Array and SALT Group and H.E.S.S. Collaboration and The Dark Energy Camera GW-EM Collaboration and the DES Collaboration and High Time Resolution Universe Survey and Las Cumbres Observatory Group and GRAWITA: GRAvitational Wave Inaf TeAm and The VINROUGE Collaboration and The CALET Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Brookhaven National Lab. (BNL), Upton, NY (United States) and Los Alamos National Lab. (LANL), Los Alamos, NM (United States) and Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States) and Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States) and Lawrence Berkeley National Laboratory-National Energy Research Scientific Computing Center (NERSC) and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Institutionen för astronomi and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Astrophysical Journal Letters, ISSN 2041-8205, 10/2017, Volume 848, Issue 2, p. L12
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 50 - 53
IceCube, the world's largest high-energy neutrino observatory, built at the South Pole, recently reported evidence of an astrophysical neutrino flux extending... 
R&D | extension | IceCube | IceVeto | neutrino | Astronomy | IceTop | INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY | NEUTRINO DETECTION | TELESCOPE COUNTERS | MULTIPARTICLE SPECTROMETERS | MUONS | SCINTILLATION COUNTERS | SENSITIVITY | SOUTHERN HEMISPHERE | COMPARATIVE EVALUATIONS | CHERENKOV COUNTERS | ASTROPHYSICS | PARTICLE IDENTIFICATION | PEV RANGE | NEUTRINOS
Conference Proceeding
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 150 - 153
The IceCube Neutrino Observatory was designed to detect highly energetic neutrinos. The detector was built as a lattice of 5160 photomultiplier tubes... 
Supernova | IceCube | Neutrino | INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY | NEUTRINO DETECTION | DESIGN | TELESCOPE COUNTERS | MULTIPARTICLE SPECTROMETERS | SCINTILLATION COUNTERS | ANTARCTIC REGIONS | DATA ACQUISITION SYSTEMS | ICE | ALGORITHMS | SUPERNOVAE | ACCURACY | CHERENKOV COUNTERS | PARTICLE IDENTIFICATION
Conference Proceeding
Physical Review letters, ISSN 0031-9007, 05/2010
We report the first observation of an anisotropy in the arrival direction of cosmic rays with energies in the multi TeV region in the Southern sky using data... 
SKY | 79 | DISTRIBUTION | CONFIGURATION | RESOLUTION | MUONS | AMPLITUDES | HARMONICS | NEUTRINOS | ANISOTROPY
Journal Article
Physical Review Letters, ISSN 0031-9007, 05/2010
The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement... 
TELESCOPES | AMANDA | KAONS | 79 | PIONS | atmospheric neutrinos | unfolding | ENERGY RANGE | MUONS | neural net | NEUTRINOS | HADRONS
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 70 - 73
Conference Proceeding
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 7 - 12
The IceCube Neutrino Observatory, completed in December 2010, is located at the geographic South Pole and incorporates a one cubic kilometer neutrino detector... 
cosmic-ray physics | neutrino astronomy | IceCube | IceTop | neutrino telescopes | INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY | NEUTRINO DETECTION | CHERENKOV COUNTERS | TELESCOPE COUNTERS | ASTROPHYSICS | PARTICLE IDENTIFICATION | MULTIPARTICLE SPECTROMETERS | SCINTILLATION COUNTERS | ICE | NEUTRINOS
Conference Proceeding
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 146 - 149
The IceCube Neutrino Observatory is located in the ice near the geographic South Pole. Particle showers from neutrino interactions in the ice produce light... 
South Pole ice | ice anisotropy | photon propagation | INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY | NEUTRINO DETECTION | DATA PROCESSING | PARTICLE IDENTIFICATION | LIGHT SCATTERING | MULTIPARTICLE SPECTROMETERS | LIGHT TRANSMISSION | ICE | NEUTRINOS | SENSORS | ANISOTROPY | VISIBLE RADIATION
Conference Proceeding
Physical Review Letters, ISSN 0031-9007, 01/2010
We present the results of searches for high-energy muon neutrinos from 41 gamma- ray bursts (GRBs) in the northern sky with the IceCube detector in its... 
SKY | TELESCOPES | MUON NEUTRINOS | PRECURSOR | CONFIGURATION | ENERGY RANGE | ASTRONOMY AND ASTROPHYSICS | WINDOWS | SATELLITES | NEUTRINOS | SPECTRA
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 2014, Volume 1630, Issue 1, pp. 180 - 183
The Precision IceCube Next Generation Upgrade (PINGU) will require optical sensors with similar performance as the digital optical modules (DOMs) of IceCube,... 
Digital Optical Module | Digitizer | PINGU | Neutrino Telescope | IceCube | PMT | INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY | MODIFICATIONS | NEUTRINO DETECTION | CHERENKOV COUNTERS | DESIGN | TELESCOPE COUNTERS | PERFORMANCE | PARTICLE IDENTIFICATION | MULTIPARTICLE SPECTROMETERS | SCINTILLATION COUNTERS | SENSORS | ACCURACY
Conference Proceeding
Physical review letter, ISSN 0031-9007, 06/2009
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 and 500 m depth in South Pole ice with better than 1%... 
ACOUSTICS | VELOCITY | EXPLOSIVES | SHEAR | ASTRONOMY AND ASTROPHYSICS | ACOUSTIC DETECTION | NEUTRINOS | REFRACTION | ACCURACY
Journal Article
Physical Review Letter, ISSN 0031-9007, 03/2009
We present a search for point sources of high energy neutrinos using 3.8 years of data recorded by AMANDA-II during 2000-2006. After reconstructing muon tracks... 
SKY | 79 | POINT SOURCES | ENERGY RANGE | MUONS | NEUTRINOS
Journal Article
Physical Review Letter, ISSN 0031-9007, 02/2009
We report on a search with the IceCube detector for high-energy muon neutrinos from GRB080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The... 
TELESCOPES | 79 | FIREBALL MODEL | MUON NEUTRINOS | ENERGY RANGE | NEUTRINOS
Journal Article
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 01/2016, Volume 2016, Issue 1
This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy... 
TELESCOPES | COSMIC MUONS | COSMIC RAY FLUX | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | POINT SOURCES | ASTROPHYSICS | RESOLUTION | COSMIC NEUTRINOS | COSMIC RAY DETECTION | EEV RANGE | ANGULAR CORRELATION
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 11/2014, Volume 1630, Issue 1, p. 149
The IceCube Neutrino Observatory is located in the ice near the geographic South Pole. Particle showers from neutrino interactions in the ice produce light... 
South Pole | Propagation | Anisotropy | Light | Neutrinos
Conference Proceeding
AIP Conference Proceedings, ISSN 0094-243X, 11/2014, Volume 1630, Issue 1, p. 153
The IceCube Neutrino Observatory was designed to detect highly energetic neutrinos. The detector was built as a lattice of 5160 photomultiplier tubes... 
Collapse | Cubic lattice | Supernovae | Search algorithms | Data acquisition systems | Neutrinos | Photomultiplier tubes | Sensors | Background noise | Muons
Conference Proceeding
AIP Conference Proceedings, ISSN 0094-243X, 11/2014, Volume 1630, Issue 1, p. 73
The IceCube neutrino observatory built in the antarctic ice offers unique opportunities in studying high energy neutrino emission from Galactic and... 
Point sources | High energy astronomy | Sensitivity analysis | Pollution sources | Anisotropy | Energy spectra | Searching | Small scale | Neutrinos | Emission analysis | Cosmic rays
Conference Proceeding
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