activity
20102013
most citedAntennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

148 citations · 358 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE201356 cited

Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

Pierre Auger Collaboration

The observation of ultrahigh energy (UHE) neutrinos has become a priority in experimental astroparticle physics. UHE neutrinos can be detected with a variety of techniques. In part…

astro-ph.HE2013

LOPES 3D - vectorial measurements of radio emission from cosmic ray induced air showers

W. D. Apel, J. C. Arteaga, L. Bähren +52

LOPES 3D is able to measure all three components of the electric field vector of the radio emission from air showers. This allows a better comparison with emission models. The meas…

astro-ph.IM2013

LOPES 3D reconfiguration and first measurements

D. Huber, W. D. Apel, J. C. Arteaga +56

The Radio detection technique of high-energy cosmic rays is based on the radio signal emitted by the charged particles in an air shower due to their deflection in the Earth's magne…

astro-ph.HE201326 cited

Thunderstorm Observations by Air-Shower Radio Antenna Arrays

W. D. Apel, J. C. Arteaga, L. Bähren +57

Relativistic, charged particles present in extensive air showers lead to a coherent emission of radio pulses which are measured to identify the shower initiating high-energy cosmic…

astro-ph.IM201317 cited

LOPES-3D, an antenna array for full signal detection of air-shower radio emission

W. D. Apel, J. C. Arteaga, L. Bähren +56

To better understand the radio signal emitted by extensive air-showers and to further develop the radio detection technique of high-energy cosmic rays, the LOPES experiment was rec…

astro-ph.HE201276 cited

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

Pierre Auger Collaboration

The Surface Detector array of the Pierre Auger Observatory can detect neutrinos with energy between 10^17 eV and 10^20 eV from point-like sources across the sky south of +55 deg an…