'Argo ybj' diaporamas de présentation

The ARGO-YBJ experiment: results and perspectives

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From Tibet to the Southern hemisphere: an RPC-based detector for astroparticle physics

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Measurement of the Cosmic Ray energy spectra by the ARGO-YBJ experiment A. Surdo

ARGO-YBJ. Measurement of the Cosmic Ray energy spectra by the ARGO-YBJ experiment A. Surdo Istituto Nazionale di Fisica Nucleare Sezione di Lecce, Italy (on behalf of the ARGO-YBJ Collaboration). The ARGO-YBJ experiment. ARGO-YBJ. A strophysical R adiation with G round-based

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EAS arrays: ARGO-YBJ and HAWC

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CRTNT Experiment Status

CRTNT Experiment Status. Zhen Cao Institute of High Energy Physics, China RICAP07, Roma, Italy, July, 2007. Introduction Two prototype telescopes Test run on ARGO-YBJ site, Tibet Full scale experiment: 2008 Updates in Physics Summary. Introduction. CRTNT.

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ARGO-YBJ experiment in Tibet

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Study with Sun Shadow Observed by the ARGO -YBJ experiment

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CRTNT Experiment Status

CRTNT Experiment Status. Zhen Cao Institute of High Energy Physics, China 30th ICRC, Merida, Mexico, July, 2007. Introduction Two prototype telescopes Test run on ARGO-YBJ site, Tibet Full scale experiment: 2008 Summary. Introduction. CRTNT. CRTNT : Cosmic Ray Tau Neutrino Telescope

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EUChinaGRID Project

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Measurement of the proton-air inelastic cross section with ARGO-YBJ

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EAS Time Structures with ARGO-YBJ experiment

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Long-term monitor on Mrk 421 using ARGO-YBJ experiment

1. Introduction 2. ARGO-YBJ experiment 3. Result of Mrk 421 Temporal analysis: Light curve, correlation Spectral Energy Distribution :X-ray and TeV Spectral Modeling 4. Summary. Long-term monitor on Mrk 421 using ARGO-YBJ experiment. S.Z Chen (IHEP/CAS/China, chensz@ihep.ac.cn)

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Search for GeV Gamma-Ray Bursts with the ARGO-YBJ Detector in Scaler Mode

Search for GeV Gamma-Ray Bursts with the ARGO-YBJ Detector in Scaler Mode. X.-X. Li , H.-H. He , F.-R. Zhu , S.-Z. Chen on behalf of the ARGO-YBJ collaboration Institute of High Energy Physics 2008.06.27. 2008 Nanjing GRB Conference ,Nanjing, China, 2008, June 23-27. Outline.

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~10 2 /m 2 /secondo

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S. Mastroianni INFN sez. di Napoli On behalf of the ARGO-YBJ Collaboration

The RPC charge Read-Out system of the ARGO-YBJ detector. S. Mastroianni INFN sez. di Napoli On behalf of the ARGO-YBJ Collaboration. Collaboration Institutes: Chinese Academy of Science (CAS) Istituto Nazionale di Fisica Nucleare (INFN).

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