Contributions to the 32nd International Cosmic Ray Conference (ICRC 2011) by the ANTARES collaboration
arXiv:1112.0478 · doi:10.1016/j.nima.2010.11.157
Abstract
The ANTARES detector, completed in 2008, is the largest neutrino telescope in the Northern hemisphere. It is located at a depth of 2.5 km in the Mediterranean Sea, 40 km off the Toulon shore. The scientific scope of the experiment is very broad, being the search for astrophysical neutrinos the main goal. In this paper we collect the 22 contributions of the ANTARES collaboration to the 32nd International Cosmic Ray Conference (ICRC 2011). At this stage of the experiment the scientific output is very rich and the contributions included in these proceedings cover the main physics results (steady point sources, correlations with GRBs, diffuse fluxes, target of opportunity programs, dark matter, exotic physics, oscillations, etc.) and some relevant detector studies (water optical properties, energy reconstruction, moon shadow, accoustic detection, etc.)
93 pages, collection of proceedings to ICRC2011 by ANTARES collaboration
References in corpus (9)
- Primary particle acceleration above 100 TeV in the shell-type Supernova Remnant RX J1713.7-3946 with deep H.E.S.S. observations
- Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector
- Atmospheric MUons from PArametric formulas: a fast GEnerator for neutrino telescopes (MUPAGE)
- Time Calibration of the ANTARES Neutrino Telescope
- Study of TeV Neutrinos with Upward Showering Muons in Super-Kamiokande
- Simulation of Ultra High Energy Neutrino Interactions in Ice and Water
- Reconstruction methods for acoustic particle detection in the deep sea using clusters of hydrophones
- Signal Classification for Acoustic Neutrino Detection
- The dispersion formula and the light group velocity in a water
Cited by in corpus (9)
- An improved method for measuring muon energy using the truncated mean of dE/dx
- A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007
- Searches for clustering in the time integrated skymap of the ANTARES neutrino telescope
- A New Method for Finding Point Sources in High-energy Neutrino Data
- Searching for High Energy Neutrino counterpart signals; The case of the Fermi Bubbles signal and of Dark Matter annihilation in the inner Galaxy
- Acoustic detection of ultra-high energetic neutrinos - a snap shot
- Recent Results from the ANTARES Neutrino Telescope
- Simulation and Analysis Chain for Acoustic Ultra-high Energy Neutrino Detectors in Water
- High-Energy Neutrino Astronomy: Status and prospects for cosmic-ray physics