activity
19962023
most citedDetection and imaging of atmospheric radio flashes from cosmic ray air showers

336 citations · 2.5k across the 69 of their papers we have counts for

collaborators

71 papers

astro-ph.HE2023★ 5 cited

Latest Analysis Results from the KASCADE-Grande Data

D. Kang, J. C. Arteaga-Velázquez, M. Bertaina +22

KASCADE-Grande, the extension of the multi-detector setup of KASCADE, was devoted to measure the properties of extensive air showers initiated by high-energy cosmic rays in the pri…

astro-ph.IM2022★ 1 cited

LOPES 3D -- studies on the benefits of EAS-radio measurements with vertically aligned antennas

D. Huber, W. D. Apel, J. C. Arteaga-Velazquez +54

The LOPES experiment was a radio interferometer built at the existing air shower array KASCADE-Grande in Karlsruhe, Germany. The last configuration of LOPES was called LOPES 3D and…

astro-ph.HE2022

Results from recent analysis of KASCADE-Grande data

D. Kang, J. C. Arteaga-Velázquez, M. Bertaina +22

KASCADE and its extension array of KASCADE-Grande were devoted to measure individual air showers of cosmic rays in the primary energy range of 100 TeV to 1 EeV. The experiment has…

astro-ph.HE2021

Results from the KASCADE-Grande Data Analysis

D. Kang, W. D. Apel, J. C. Arteaga-Velázquez +45

KASCADE-Grande and its original array of KASCADE were dedicated to measure individual air showers of cosmic rays with great detail in the primary energy range of 100 TeV up to 1 Ee…

astro-ph.HE2021★ 18 cited

Final results of the LOPES radio interferometer for cosmic-ray air showers

W. D. Apel, J. C. Arteaga-Velázquez, L. Bähren +54

LOPES, the LOFAR prototype station, was an antenna array for cosmic-ray air showers operating from 2003 - 2013 within the KASCADE-Grande experiment. Meanwhile, the analysis is fini…

astro-ph.HE2019

Latest results from the KASCADE-Grande data analysis

D. Kang, A. Haungs, W. D. Apel +45

Over the past 20 years, KASCADE and its extension KASCADE-Grande were dedicated to measure high-energy cosmic rays with primary energies of 100 TeV to 1 EeV. The data accumulation…