A shower array exploiting the full coverage approach with a high segmentation of the readout allow to image the front of atmospheric showers with unprecedented resolution and detail. The grid distance determines the energy threshold (small energy showers are lost in the gap between detectors) and the quality of the shower sampling. Therefore, this experimental solution is needed to detect showers with a threshold in the 100 GeV range. The full coverage approach has been exploited in the ARGO-YBJ experiment. In this contribution we will summarise the advantages of this technique and discuss possible applications in new wide field of view detectors.Comment: Invited Talk to 21st International Symposium on Very High Energy Cosmic Ray Interact...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 ...
The ARGO-YBJ experiment has been in stable data taking for 5 years at the YangBaJing Cosmic Ray Obse...
Antenna arrays are beginning to make important contributions to high energy astroparticle physics su...
Abstract The ARGO-YBJ experiment is designed for the detection of Extensive Air Showers (EAS) in t...
The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines high altitude location...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
Radio-detection is becoming an established technique for the detection of air showers induced by cos...
This proceeding gives a summary of the current status and open questions of the radio technique for ...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
The ARGO-YBJ experiment has two kinds of signals in the shower working mode which allows coverage of...
Ultra high energy (UHE) gamma ray astronomy is an exciting area which has added a new sense of purpo...
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
The ARGO-YBJ experiment is an Extensive Air Shower array currently operating at the high altitude ...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
Very High Energy (VHE) γ-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ experim...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 ...
The ARGO-YBJ experiment has been in stable data taking for 5 years at the YangBaJing Cosmic Ray Obse...
Antenna arrays are beginning to make important contributions to high energy astroparticle physics su...
Abstract The ARGO-YBJ experiment is designed for the detection of Extensive Air Showers (EAS) in t...
The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines high altitude location...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
Radio-detection is becoming an established technique for the detection of air showers induced by cos...
This proceeding gives a summary of the current status and open questions of the radio technique for ...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
The ARGO-YBJ experiment has two kinds of signals in the shower working mode which allows coverage of...
Ultra high energy (UHE) gamma ray astronomy is an exciting area which has added a new sense of purpo...
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
The ARGO-YBJ experiment is an Extensive Air Shower array currently operating at the high altitude ...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
Very High Energy (VHE) γ-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ experim...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 ...
The ARGO-YBJ experiment has been in stable data taking for 5 years at the YangBaJing Cosmic Ray Obse...
Antenna arrays are beginning to make important contributions to high energy astroparticle physics su...