Gašper Kukec Mezek

The Cherenkov Telescope Array. Science Goals and Current Status

Rene A. Ong, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič et autres

The Cherenkov Telescope Array (CTA) is the major ground-based gamma-ray observatory planned for the next decade and beyond. Consisting of two large atmospheric Cherenkov telescope arrays (one in the southern hemisphere and one in the northern hemisphere), CTA will have superior angular …

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Mass Composition of Cosmic Rays with Energies above 10[sup]17.2 eV from the Hybrid Data of the Pierre Auger Observatory

Alexey Yushkov, Andrej Filipčič, Gašper Kukec Mezek, Samo Stanič et autres

0 0 1 1 17 7 7. . .

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Estimating the Depth of Shower Maximum using the Surface Detectors of the Pierre Auger Observatory

Carlos José Todero Peixoto, Andrej Filipčič, Gašper Kukec Mezek, Samo Stanič et autres

The Pierre Auger Collaboration has developed a method for estimating the depth of shower maximum (X max ) using the risetime of the signals recorded by the array of water-Cherenkov detectors.The average value of X max is determined for energies above 3 …

The muon component of extensive air showers above 10[sup]17.5 eV measured with the Pierre Auger Observatory

Federico Sánchez, Andrej Filipčič, Gašper Kukec Mezek, Samo Stanič et autres

Direct measurement of the muonic content of extensive air showers between 2 × 10[sup]17 and 2 × 10[sup]18 eV at the Pierre Auger Observatory

A. Aab, Andrej Filipčič, Gašper Kukec Mezek, Samo Stanič et autres

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision.By using an array of prototype underground muon detectors, we have performed the first direct …

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A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

Alexander Aab, Pedro Abreu, Belén Andrada, Martin Erdmann et autres

Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

Pierre Auger Collaboration, Alexander Aab, Gioacchino Alex Anastasi, Qader Dorosti et autres

Pierre Auger Collaboration; Aab, Alexander; Abreu, Pedro; Aglietta, Marco; Albury, Justin M.; Allekotte, Ingomar; Almela, Alejandro; Alvarez Castillo, Jesus; Alvarez-Muñiz, Jaime; Alves Batista, Rafael; Anastasi, Gioacchino Alex; Anchordoqui, Luis; Andrada, Belén; Andringa, Sofia; Aramo, Carla; Araújo Ferreira, Paulo Ricardo; Asorey, Hernán Gonzalo; …

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Search for magnetically-induced signatures in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

A. Aab, Pedro Abreu, L Anchordoqui, Ralph Engel et autres

Measurement of the cosmic-ray energy spectrum above $2.5{\times} 10^{18}$ eV using the Pierre Auger Observatory

Alexander Aab, Pedro Abreu, Luis A. Anchordoqui, Rita dos Anjos et autres

Mass composition of cosmic rays with energies from 10^17.2 eV to 10^20 eV using surface and fluorescence detectors of the Pierre Auger Observatory

Gašper Kukec Mezek

Ultra-high-energy cosmic rays (UHECRs) are highly energetic particles with EeV energies, exceeding the capabilities of man-made colliders. They hold information on extreme astrophysical processes that create them and the medium they traverse on their way towards Earth. However, their mass composition at …

Delčna sestava kozmičnih žarkov ekstremnih energij na observatoriju Pierre Auger

Gašper Kukec Mezek

Cosmic rays with energies above 10^18 eV, usually referred to as ultra-high energy cosmic rays (UHECR), have been a mystery from the moment they have been discovered. Although we have now more information on their extragalactic origin, their direct sources still remain …

Status and performance results from NectarCAM

T. Tavernier, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič et autres

The Cherenkov Telescope Array (CTA) will be the first ground-based observatory for gamma-ray astronomy. With more than a hundred of 4th generation of Imaging Atmospheric Cherenkov Telescopes (IACTs) distributed in two large arrays, CTA will reach unprecedented sensitivity, angular resolution, and spectral …

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