586 citations · 870 across the 13 of their papers we have counts for
13 papers
Comparison of the measured atmospheric muon rate with Monte Carlo simulations and sensitivity study for detection of prompt atmospheric muons with KM3NeT
Piotr Kalaczyński
The KM3NeT Collaboration has successfully deployed the first detection units of the next generation undersea neutrino telescopes in the Mediterranean Sea at the two sites in Italy…
Event reconstruction for KM3NeT/ORCA using convolutional neural networks
Sebastiano Aiello, Arnauld Albert, Sergio Alves Garre +229
The KM3NeT research infrastructure is currently under construction at two locations in the Mediterranean Sea. The KM3NeT/ORCA water-Cherenkov neutrino detector off the French coast…
gSeaGen: the KM3NeT GENIE-based code for neutrino telescopes
Sebastiano Aiello, Arnauld Albert, Sergio Alves Garre +233
The gSeaGen code is a GENIE-based application developed to efficiently generate high statistics samples of events, induced by neutrino interactions, detectable in a neutrino telesc…
Radio detection of cosmic rays in [1.7-3.7] MHz: the EXTASIS experiment
Didier Charrier, Richard Dallier, Antony Escudie +4
Since 2003, significant efforts have been devoted to the understanding of the radio emission of extensive air showers above 20 MHz. Despite some studies led until the early ninetie…
Multi-wavelength observation of cosmic-ray air-showers with CODALEMA/EXTASIS
Antony Escudie, Didier Charrier, Richard Dallier +4
Since 2003, significant efforts have been devoted to the understanding of the radio emission of extensive air shower in the range [20-200] MHz. Despite some studies led until the e…
Radio detection of atmospheric air showers of particles
Antony Escudie, Richard Dallier, Didier Charrier +4
Since 2002, the CODALEMA experiment located within the Nançay Radio Observatory studies the ultra-high energy cosmic rays (above 10^{17} eV) arriving in the Earth atmosphere. These…
Influence of a planar boundary on the electric field emitted by a particle shower
Daniel García-Fernández, Benoît Revenu, Antony Escudie +1
The radio detection of cosmic rays consists in the estimation of the properties of a primary cosmic ray by observing the electric field emitted by the extensive air shower (EAS) cr…
Calculations of low-frequency radio emission by cosmic ray-induced particle showers
Daniel García-Fernández, Benoît Revenu, Didier Charrier +3
The radio technique for the detection of high energy cosmic rays consists in measuring the electric field created by the particle showers created inside a medium by the primary cos…
The CODALEMA/EXTASIS experiment: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)
Hervé Carduner, Didier Charrier, Richard Dallier +9
Contributions of the CODALEMA/EXTASIS experiment to the 35th International Cosmic Ray Conference, 12-20 July 2017, Busan, South Korea.
Ultimate precision in cosmic-ray radio detection --- the SKA
Tim Huege, Justin D. Bray, Stijn Buitink +17
As of 2023, the low-frequency part of the Square Kilometre Array will go online in Australia. It will constitute the largest and most powerful low-frequency radio-astronomical obse…
Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory
The Pierre Auger Collaboration, Alexander Aab, Pedro Abreu +461
A measurement of the cosmic-ray spectrum for energies exceeding eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\…
Centrality dependence of high pT hadron suppression in Au+Au collisions at sqrt(sNN)=130 GeV
C. Adler
Inclusive transverse momentum distributions of charged hadrons within 0.2<pT<6.0 GeV/c have been measured over a broad range of centrality for Au+Au collisions at sqrt(sNN)=130 GeV…
Azimuthal anisotropy of K0s and Lambda prduction at mid-rapidity from Au+Au collisions at root s = 130 GeV
STAR collaboration
We report STAR results on the azimuthal anisotropy parameter v2 for strange particles K0S, L and Lbar at midrapidity in Au+Au collisions at sNN = 130 GeV at RHIC. The value of v2 a…