Add to ORKGThe ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Chambers (RPCs). The main scientific goal of this Chinese-Italian experiment is very high energy (VHE) gamma-ray astronomy. High altitude and full coverage ensure a low energy threshold (few hundreds of GeV for gamma-initiated showers). High duty-cycle and large field of view allow a continuous sky survey. The data collected with the central carpet during the detector debugging have been analysed. First results about detector performances, gamma astronomy and cosmic-ray physics are presented
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian colla...
The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (...
The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
Very High Energy gamma ray astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exper...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exp...
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 ...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ ex...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m a...
Gamma ray astronomy at energies 10^11-10^13 eV, which are strictly related to the identification an...
Gamma ray astronomy at energies 1011 1013 eV, which are strictly related to the identication and stu...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m...
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian colla...
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian colla...
The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (...
The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
Very High Energy gamma ray astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exper...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exp...
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 ...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ ex...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m a...
Gamma ray astronomy at energies 10^11-10^13 eV, which are strictly related to the identification an...
Gamma ray astronomy at energies 1011 1013 eV, which are strictly related to the identication and stu...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m...
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian colla...
The ARGO-YBJ experiment, located at Yangbajing, Tibet, China, performed by a wide Sino-Italian colla...
The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (...
The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P...