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Design and Performance of the first IceAct Demonstrator at the South Pole
M. G. Aartsen, M. Ackermann, J. Adams +393
In this paper we describe the first results of a compact imaging air-Cherenkov telescope, IceAct, operating in coincidence with the IceCube Neutrino Observatory (IceCube) at the ge…
The IceCube Neutrino Observatory: Instrumentation and Online Systems
IceCube Collaboration, M. G. Aartsen, M. Ackermann +350
The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detect…
IceCube-Gen2 - The Next Generation Neutrino Observatory at the South Pole: Contributions to ICRC 2015
Gen2 Collaboration, M. G. Aartsen, K. Abraham +337
Papers submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube-Gen2 Collaboration.
Improvement in Fast Particle Track Reconstruction with Robust Statistics
M. G. Aartsen, R. Abbasi, Y. Abdou +277
The IceCube project has transformed one cubic kilometer of deep natural Antarctic ice into a Cherenkov detector. Muon neutrinos are detected and their direction inferred by mapping…
Measurement of South Pole ice transparency with the IceCube LED calibration system
IceCube Collaboration, M. G. Aartsen, R. Abbasi +272
The IceCube Neutrino Observatory, approximately 1 km^3 in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by ch…
IceTop: The surface component of IceCube
IceCube Collaboration, R. Abbasi, Y. Abdou +280
IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the…
The Design and Performance of IceCube DeepCore
The IceCube Collaboration
The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a su…
Background studies for acoustic neutrino detection at the South Pole
The IceCube Collaboration, R. Abbasi, Y. Abdou +262
The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the tiny flux of cosmogenic neutrinos expected on Earth. The energy…
Search for astrophysical high energy neutrino point sources with a False Discovery Rate controlling procedure
Bruny Baret, Mathieu Labare, Daniel Bertrand
A systematic multiple hypothesis testing approach is applied to the search for astrophysical sources of high energy neutrinos. The method is based on the maximisation of the detect…
Calibration and Characterization of the IceCube Photomultiplier Tube
The IceCube Collaboration, R. Abbasi, Y. Abdou +256
Over 5,000 PMTs are being deployed at the South Pole to compose the IceCube neutrino observatory. Many are placed deep in the ice to detect Cherenkov light emitted by the products…