The ARGO‐YBJ experiment has been put in stable data taking at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l.). In this paper we report a few selected results in Gamma‐Ray Astronomy (Crab Nebula and Mrk421 observations, search for high energy tails of Gamma Ray Bursts) and Cosmic Ray Physics (Moon and Sun shadow observations, proton‐air cross section measurement, preliminary measurement of the antiproton∕proton ratio at TeV energies).
Results from ARGO-YBJ / Bartoli, Bruno; Catalanotti, Sergio; D'ETTORRE PIAZZOLI, Benedetto; DI GIROLAMO, Tristano; Iacovacci, Michele; .,. - STAMPA. - 1112:(2009), pp. 148-156. [10.1063/1.3125775]
Results from ARGO-YBJ
BARTOLI, BRUNO;CATALANOTTI, SERGIO;D'ETTORRE PIAZZOLI, BENEDETTO;DI GIROLAMO, TRISTANO;IACOVACCI, MICHELE;
2009
Abstract
The ARGO‐YBJ experiment has been put in stable data taking at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l.). In this paper we report a few selected results in Gamma‐Ray Astronomy (Crab Nebula and Mrk421 observations, search for high energy tails of Gamma Ray Bursts) and Cosmic Ray Physics (Moon and Sun shadow observations, proton‐air cross section measurement, preliminary measurement of the antiproton∕proton ratio at TeV energies).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.