Abstract

Very High Energy (VHE) gamma-astronomy and cosmic ray physics are the main goals of the ARGO-YBJ experiment. The detector is located in Tibet (People's Republic of China) and is a full coverage Extensive Air Shower array consisting of a carpet of Resistive Plate Chambers (RPCs). Altitude and full coverage ensure an energy threshold of few hundreds of GeV for primary photons detected in shower mode, while the RPC time resolution gives a good pointing accuracy, thus allowing a high sensitivity to gamma-ray sources. The large field of view (FoV) and the high duty-cycle allow the continuous monitor of the Northern sky in the declination band (-10, +70 degrees). The detector operates also in scaler mode in order to look for Gamma Ray Burst (GRB) signals in the range 1-100 GeV in coincidence with GRB detection by satellites. After some detail about the performances of the detector, the present results concerning gamma-astronomy will be presented.

Autore Pugliese

• Bernardini Paolo

Tutti gli autori

• P. Bernardini

Titolo volume/Rivista

POS PROCEEDINGS OF SCIENCE

Anno di pubblicazione

2010

ISSN

1824-8039

ISBN

Non Disponibile

Numero di citazioni Wos

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Numero di citazioni Scopus

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Settori ERC

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Codici ASJC

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