We have used Monte Carlo simulations to investigate the capabilities of a giant air shower observatory designed to detect showers initiated by cosmic rays with energies exceeding 1019 eV. The observatory is to consist of an array of detectors that will characterise the air shower at ground level, and optical detectors to measure the fluorescence light emitted by the shower in the atmosphere. Using these detectors together in a ‘hybrid’ configuration, we find that precise geometrical reconstruction of the shower axis is possible, leading to excellent resolution in energy. The technique is also shown to provide very good reconstruction below 1019 eV, at energies where the ground array is not fully efficient.B.R. Dawson, H.Y. Dai, P. Sommers, ...
The Pierre Auger Observatory detects ultra-high energy cosmic rays by implementing two complementary...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
Very-high-energy $$\gamma $$-ray astronomy based on the measurement of air shower particles at groun...
Current detectors for Very-High-Energy γ-ray astrophysics are either pointing instruments with a sma...
International audienceALTO is a wide field-of-view air shower detector array for very-high-energy (V...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at obser...
The Pierre Auger Observatory is the largest experiment ever designed to detect ultra high energy cos...
A novel detector for ultra-high energy cosmic rays, and its prototype are discussed. It detects even...
In order to investigate discrete sources of ultra‐high energy gamma rays, by studying extensive air ...
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles gre...
The highest energy cosmic rays (>10^19 eV)are hardly explained by common astrophysics. In order to i...
We present a fast one dimensional hybrid method to efficiently simulate extensive air showers up to ...
The Telescope Array (TA) observatory utilizes fluorescence detectors and surface detectors (SDs) to ...
Future detection of Extensive Air Showers (EAS) produced by Ultra High Energy Cosmic Particles by me...
The Pierre Auger Observatory detects ultra-high energy cosmic rays by implementing two complementary...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
Very-high-energy $$\gamma $$-ray astronomy based on the measurement of air shower particles at groun...
Current detectors for Very-High-Energy γ-ray astrophysics are either pointing instruments with a sma...
International audienceALTO is a wide field-of-view air shower detector array for very-high-energy (V...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at obser...
The Pierre Auger Observatory is the largest experiment ever designed to detect ultra high energy cos...
A novel detector for ultra-high energy cosmic rays, and its prototype are discussed. It detects even...
In order to investigate discrete sources of ultra‐high energy gamma rays, by studying extensive air ...
We describe the method devised to reconstruct inclined cosmic-ray air showers with zenith angles gre...
The highest energy cosmic rays (>10^19 eV)are hardly explained by common astrophysics. In order to i...
We present a fast one dimensional hybrid method to efficiently simulate extensive air showers up to ...
The Telescope Array (TA) observatory utilizes fluorescence detectors and surface detectors (SDs) to ...
Future detection of Extensive Air Showers (EAS) produced by Ultra High Energy Cosmic Particles by me...
The Pierre Auger Observatory detects ultra-high energy cosmic rays by implementing two complementary...
Air shower simulation programs are essential tools for the analysis of data from cosmic ray experime...
Very-high-energy $$\gamma $$-ray astronomy based on the measurement of air shower particles at groun...