The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines high altitude location and full coverage active area in order to reach low energy threshold at a level of few hundred of GeV. The large field of view (≈ 2 sr) and the high duty cycle (≥ 90%) allow the continuous monitoring of the sky searching for unknown sources and unpredictable events, such as flares in blazar emissions and high energy Gamma-Ray Bursts (GRBs). In this paper I will briefly report on the detector performance and on some preliminary results achieved in γ-ray astronomy
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
Gamma ray astronomy at energies 1011 1013 eV, which are strictly related to the identication and stu...
The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines high altitude locatio...
""The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines. high altitude locat...
The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
for the ARGO-YBJ collaboration Abstract — ARGO-YBJ is an air shower detector made by a continuous ca...
been operated to survey the northern sky for gamma ray sources, transient or steady, for nearly 6 ye...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
ARGO-YBJ is a full coverage air shower array located at the YangBaJing Cosmic Ray Laboratory (Tibet,...
The ARGO-YBJ detector, currently under installation at the Yangbajing Cosmic Ray Laboratory (4300 m ...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
Gamma ray astronomy at energies 1011 1013 eV, which are strictly related to the identication and stu...
The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines high altitude locatio...
""The ARGO-YBJ experiment is an Extensive Air Shower (EAS) array which combines. high altitude locat...
The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
for the ARGO-YBJ collaboration Abstract — ARGO-YBJ is an air shower detector made by a continuous ca...
been operated to survey the northern sky for gamma ray sources, transient or steady, for nearly 6 ye...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
Gamma ray source detection above 30TeV is an encouraging approach for finding galactic cosmic ray or...
ARGO-YBJ is a full coverage air shower array located at the YangBaJing Cosmic Ray Laboratory (Tibet,...
The ARGO-YBJ detector, currently under installation at the Yangbajing Cosmic Ray Laboratory (4300 m ...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
Gamma ray astronomy at energies 1011 1013 eV, which are strictly related to the identication and stu...