The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at observation of cosmic rays beyond 100 TeV and gamma rays above 1 TeV via observation of the extensive air showers (EAS) caused in the atmosphere. Two common detection techniques are timing arrays and imaging air shower cherenkov telescopes (IACT). Timing arrays yield good directional and energy reconstruction, but provide only mediocre gamma-hadron-separation at their energy threshold. IACTs are good at separation, but since a stereoscopic view of a shower is needed for high reconstruction accuracy, it is difficult to achieve the large effective areas needed for ultra high energy observations. In this work we present the simulations performed to e...
Proceedings of the 30th ICRC, Merida, Mexico (2007). Rogelio Caballero, Juan Carlos D'Olivo, Gustavo...
Abstract: The reconstruction of air shower parameters such as energy and position of shower maximum,...
The TAIGA complex-detector is designed to study gamma and cosmic rays in the energy range above 30 T...
The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at obser...
Up to several 10s of TeV, Imaging Air Cherenkov Telescopes (IACTs) have proven to be the instruments...
This work is a methodical study on hybrid reconstruction techniques for hybrid imaging/timing Cheren...
We present analysis techniques specific to multi-TeV extensive air showers (EAS). Our emphasis is on...
The future of ground based gamma-ray astronomy lies in large arrays of Imaging Atmospheric Cherenkov...
The TAIGA astroparticle observatory is progressing with the deployment of new detector stations. The...
We have used Monte Carlo simulations to investigate the capabilities of a giant air shower observato...
International audienceALTO is a wide field-of-view air shower detector array for very-high-energy (V...
In the last 20 years the ground-based telescopes have opened a new observation window at very high ...
The Tunka Advanced Instrument for Gamma-ray and cosmic ray Astrophysics (TAIGA) is a hybrid experime...
International audienceWe present a new paradigm for the simulation of arrays of Imaging Atmospheric ...
Proceedings of the 30th ICRC, Merida, Mexico (2007). Rogelio Caballero, Juan Carlos D'Olivo, Gustavo...
Abstract: The reconstruction of air shower parameters such as energy and position of shower maximum,...
The TAIGA complex-detector is designed to study gamma and cosmic rays in the energy range above 30 T...
The Tunka Advanced International Gamma-ray and Cosmic ray Astrophysics (TAIGA) project aims at obser...
Up to several 10s of TeV, Imaging Air Cherenkov Telescopes (IACTs) have proven to be the instruments...
This work is a methodical study on hybrid reconstruction techniques for hybrid imaging/timing Cheren...
We present analysis techniques specific to multi-TeV extensive air showers (EAS). Our emphasis is on...
The future of ground based gamma-ray astronomy lies in large arrays of Imaging Atmospheric Cherenkov...
The TAIGA astroparticle observatory is progressing with the deployment of new detector stations. The...
We have used Monte Carlo simulations to investigate the capabilities of a giant air shower observato...
International audienceALTO is a wide field-of-view air shower detector array for very-high-energy (V...
In the last 20 years the ground-based telescopes have opened a new observation window at very high ...
The Tunka Advanced Instrument for Gamma-ray and cosmic ray Astrophysics (TAIGA) is a hybrid experime...
International audienceWe present a new paradigm for the simulation of arrays of Imaging Atmospheric ...
Proceedings of the 30th ICRC, Merida, Mexico (2007). Rogelio Caballero, Juan Carlos D'Olivo, Gustavo...
Abstract: The reconstruction of air shower parameters such as energy and position of shower maximum,...
The TAIGA complex-detector is designed to study gamma and cosmic rays in the energy range above 30 T...