activity
20172026
most citedMeasurement of the cosmic-ray energy spectrum above eV using the Pierre Auger Observatory

213 citations · 495 across the 21 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.HE2019

The Pierre Auger Observatory: Contributions to the 36th International Cosmic Ray Conference (ICRC 2019)

The Pierre Auger Collaboration, A. Aab, P. Abreu +383

Contributions of the Pierre Auger Collaboration to the 36th International Cosmic Ray Conference (ICRC 2019), 24 July - 1 August 2019, Madison, Wisconsin, USA.

astro-ph.IM2019

Modeling the Aperture of Radio Instruments for Air-Shower Detection

V. Lenok, P. Bezyazeekov, N. Budnev +21

Sparse digital antenna arrays constitute a promising detection technique for future large-scale cosmic-ray observatories. It has recently been shown that this kind of instrumentati…

astro-ph.HE2019

Seven years of Tunka-Rex operation

D. Kostunin, P. Bezyazeekov, N. Budnev +21

The Tunka Radio Extension (Tunka-Rex) is a digital antenna array located in the Tunka Valley in Siberia, which measures the radio emission of cosmic-ray air-showers with energies u…

astro-ph.IM2019

Advanced Signal Reconstruction in Tunka-Rex with Matched Filtering and Deep Learning

P. Bezyazeekov, N. Budnev, O. Fedorov +21

The Tunka Radio Extension (Tunka-Rex) is a digital antenna array operating in the frequency band of 30-80 MHz, measuring the radio emission of air-showers induced by ultra-high ene…

astro-ph.IM2019

Towards the Tunka-Rex Virtual Observatory

P. Bezyazeekov, N. Budnev, O. Fedorov +21

The Tunka Radio Extension (Tunka-Rex) is a cosmic-ray detector operating since 2012. The detection principle of Tunka-Rex is based on the radio technique, which impacts data acquis…

astro-ph.HE2019

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +389

Neutrinos with energies above eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos…