The central array of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet, P.R. China) has been put into operation for physics runs. It is made of 130 identical sub-units of 12 RPCs each (”cluster”) covering a surface of about 5800 m 2 with 92% active area. Signals are picked-up by external electrodes of small size, thus allowing the sampling of EAS with high space-time granularity. Shower events are detected at a trigger rate of about 4 kHz. Events with a few particles detected by a single cluster are counted in scaler mode on a time base of 500 milliseconds. Preliminary results from the analysis of events collected in a few months of data taking are presented
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
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 ...
The central array of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet...
The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300ma.s.l., Tibet, P.R...
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the ...
The detection of small size air showers at high altitude allows the search for γ-ray point sources a...
experiment is to operate in the field of High Energy Cosmic Ray Physics with an energy threshold of ...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 ...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
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 ...
The central array of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300 m a.s.l., Tibet...
The setting up of the ARGO detector at the YangBaJing Cosmic Ray Laboratory (4300ma.s.l., Tibet, P.R...
The ARGO-YBJ experiment is in stable data taking since November 2007 at the YangBaJing Cosmic Ray La...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 m...
The ARGO-YBJ detector, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300m a....
The ARGO-YBJ experiment has been in stable data taking from November 2007 till February 2013 at the ...
The detection of small size air showers at high altitude allows the search for γ-ray point sources a...
experiment is to operate in the field of High Energy Cosmic Ray Physics with an energy threshold of ...
The ARGO-YBJ experiment, installed at the Yangbajing Cosmic Ray Laboratory (Tibet, China), at 4300 ...
The ARGO-YBJ detector is an extensive air shower array consisting of a carpet of Resistive Plate Cha...
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 ...