activity
20112025
most citedAn improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory

179 citations · 2.2k across the 52 of their papers we have counts for

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Showing astro-ph.IMShow all

12 papers · 1 filter

astro-ph.IM2022★ 17 cited

A Double Layered Water Cherenkov Detector Array for Gamma-Ray Astronomy

Samridha Kunwar, Hazal Goksu, Jim Hinton +4

Ground-level particle detection is now a well-established approach to TeV gamma-ray astronomy. Detection of Cherenkov light produced in water-filled detection units is a proven and…

astro-ph.IM2021

Science verification of the new FlashCam-based camera in the 28m telescope of H.E.S.S

Gerd Pühlhofer, Konrad Bernlöhr, Baiyang Bi +13

In October 2019 the central 28m telescope of the H.E.S.S. experiment has been upgraded with a new camera. The camera is based on the FlashCam design which has been developed in vie…

astro-ph.IM2021★ 28 cited

TeV emission of Galactic plane sources with HAWC and H.E.S.S

H. Abdalla, F. Aharonian, F. Ait Benkhali +318

The High Altitude Water Cherenkov (HAWC) observatory and the High Energy Stereoscopic System (H.E.S.S.) are two leading instruments in the ground-based very-high-energy gamma-ray d…

astro-ph.IM2019★ 4 cited

Trigger performance verification of the FlashCam prototype camera

S. Sailer, F. Werner, G. Hermann +33

FlashCam is a camera proposed for the medium-sized telescopes of the Cherenkov Telescope Array (CTA). We compare camera trigger rates obtained from measurements with the camera pro…

astro-ph.IM2016★ 32 cited

Performance Verification of the FlashCam Prototype Camera for the Cherenkov Telescope Array

F. Werner, C. Bauer, S. Bernhard +32

The Cherenkov Telescope Array (CTA) is a future gamma-ray observatory that is planned to significantly improve upon the sensitivity and precision of the current generation of Chere…

astro-ph.IM2016★ 103 cited

The Pierre Auger Observatory Upgrade - Preliminary Design Report

The Pierre Auger Collaboration, A. Aab, P. Abreu +462

The Pierre Auger Observatory has begun a major Upgrade of its already impressive capabilities, with an emphasis on improved mass composition determination using the surface detecto…

astro-ph.IM2015★ 13 cited

FlashCam: a fully-digital camera for the medium-sized telescopes of the Cherenkov Telescope Array

G. Pühlhofer, C. Bauer, S. Bernhard +31

The FlashCam group is currently preparing photomultiplier-tube based cameras proposed for the medium-sized telescopes (MST) of the Cherenkov Telescope Array (CTA). The cameras are…

astro-ph.IM2014★ 45 cited

First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers

R. Smida, F. Werner, R. Engel +55

We report the first direct measurement of the overall characteristics of microwave radio emission from extensive air showers. Using a trigger provided by the KASCADE-Grande air sho…

astro-ph.IM2014★ 10 cited

Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America

Pierre Auger Collaboration, Gabriele Curci

The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the mon…

astro-ph.IM2013★ 4 cited

Observation of Polarised Microwave Emission from Cosmic Ray Air Showers

R. Smida, F. Werner, R. Engel +55

We report on the first direct measurement of the basic features of microwave radio emission from extensive air showers. Using a trigger provided by the KASCADE-Grande air shower ar…

astro-ph.IM2012★ 148 cited

Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

P. Abreu, M. Aglietta, M. Ahlers +512

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineer…

astro-ph.IM2012★ 35 cited

The Rapid Atmospheric Monitoring System of the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +508

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10^17 eV. During clear nights with a low illuminated moon fraction, the UV fluo…