0000000001085757

AUTHOR

X.d. Sheng

showing 1 related works from this author

Scaler mode technique for the ARGO-YBJ detector

2008

The ARGO-YBJ experiment has been designed to study the Extensive Air Showers with an energy threshold lower than that of the existing arrays by exploiting the high altitude location(4300 m a.s.l. in Tibet, P.R. China) and the full ground plane coverage. The lower energy limit of the detector (E $\sim$ 1 GeV) is reached by the scaler mode technique, i.e. recording the counting rate at fixed time intervals. At these energies, transient signals due to local (e.g. Forbush Decreases) and cosmological (e.g. Gamma Ray Bursts) phenomena are expected as a significant variation of the counting rate compared to the background. In this paper the performance of the ARGO-YBJ detector operating in scaler …

Gamma ray burstAstrophysics::High Energy Astrophysical PhenomenaCamere a piani resistiviFOS: Physical sciencesCosmic rayAstrophysicsRivelatori di sciami estesi01 natural sciencesRaggi cosmiciOpticsSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesLimit (music)010303 astronomy & astrophysicsArgoGround planegamma ray bursts cosmic rays extended air showersPhysics010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)DetectorMode (statistics)Astronomy and AstrophysicsSciami estesibusinessGamma-ray burstEnergy (signal processing)
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