ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimized to study small size air showers. It consists of a layer of Resistive Plate Counters (RPCs) covering an area of similar to 6500 m(2) and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m a.s.l. ARGO-YBJ will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics in the range 10 GeV divided by 500 TeV. The sensitivity of ARGO-YBJ to detect high energy GRBs is presented
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate ...
We report on the search for Gamma Ray Bursts (GRBs) in the energy range 1-100GeV in coincidence with...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ ia a detector optimized to study small size air showers. It consists of a layer of Resistiv...
The ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBajing) experiment is designed...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m a...
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 ex...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exp...
Very High Energy Gamma Astronomy is one of the scientific aims of the ARGO-YBJ experiment (YangBaJin...
We report on the search for gamma ray bursts (GRBs) in the energy range1-100 GeV in coincidence with...
Abstract ARGO-YBJ is a "full coverage" air shower detector currently under construction at...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate ...
We report on the search for Gamma Ray Bursts (GRBs) in the energy range 1-100GeV in coincidence with...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimiz...
ARGO-YBJ ia a detector optimized to study small size air showers. It consists of a layer of Resistiv...
The ARGO-YBJ (Astrophysical Radiation Ground-based Observatory at YangBajing) experiment is designed...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m a...
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 ex...
Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ exp...
Very High Energy Gamma Astronomy is one of the scientific aims of the ARGO-YBJ experiment (YangBaJin...
We report on the search for gamma ray bursts (GRBs) in the energy range1-100 GeV in coincidence with...
Abstract ARGO-YBJ is a "full coverage" air shower detector currently under construction at...
Very high energy gamma ray astronomy is one of the scientific goals of the ARGO-YBJ experiment. The ...
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate ...
We report on the search for Gamma Ray Bursts (GRBs) in the energy range 1-100GeV in coincidence with...