activity
20062009
most citedDetection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

73 citations · 293 across the 11 of their papers we have counts for

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astro-ph200823 cited

Active Galactic Nuclei: Sources for ultra high energy cosmic rays?

P. L. Biermann, J. K. Becker, L. Caramete +11

The origin of ultra high energy cosmic rays promises to lead us to a deeper understanding of the structure of matter. This is possible through the study of particle collisions at c…

astro-ph200832 cited

Frequency spectra of cosmic ray air shower radio emission measured with LOPES

A. Nigl

AIMS: We wish to study the spectral dependence of the radio emission from cosmic-ray air showers around 100 PeV (1017 eV). METHODS: We observe short radio pulses in a broad frequen…

astro-ph200825 cited

Direction identification in radio images of cosmic-ray air showers detected with LOPES and KASCADE

A. Nigl

AIMS: We want to understand the emission mechanism of radio emission from air showers to determine the origin of high-energy cosmic rays. Therefore, we study the geometry of the ai…

astro-ph200821 cited

Geometry reconstruction of fluorescence detectors revisited

D. Kuempel, K. -H. Kampert, M. Risse

The experimental technique of fluorescence light observation is used in current and planned air shower experiments that aim at understanding the origin of ultra-high energy cosmic…

astro-ph200773 cited

Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector

The IceCube Collaboration, A. Achterberg

The IceCube neutrino detector is a cubic kilometer TeV to PeV neutrino detector under construction at the geographic South Pole. The dominant population of neutrinos detected in Ic…

astro-ph200666 cited

Five years of searches for point sources of astrophysical neutrinos with the AMANDA-II neutrino telescope

A. Achterberg

We report the results of a five-year survey of the northern sky to search for point sources of high energy neutrinos. The search was performed on the data collected with the AMANDA…