Very High Energy Gamma Astronomy is one of the scientific aims of the ARGO-YBJ experiment (YangBaJing, P.R. China), an extensive air shower detector made of a single layer of Resistive Plate Chambers covering a surface of about 6700 m2. The exploitation of the full coverage approach (93% of active area) together with the very high altitude location
Bacci, C., DE VINCENZI, M., Pistilli, P., Parisi, M., Mari, S.M., Bussino, S.A.M., et al. (2008). Study of gamma-hadron discrimination for the ARGO-YBJ experiment. In Proceedings of the 30th International Cosmic Ray Conference (pp.1503-1506). Mexico City : Universidad Nacional Autónoma de México.
Study of gamma-hadron discrimination for the ARGO-YBJ experiment
BACCI, Cesare;DE VINCENZI, Mario;PISTILLI, Pio;PARISI, Mario;MARI, Stefano Maria;BUSSINO, Severino Angelo Maria;CELIO, PAOLA;JAMES, IRINA;MONTINI, PAOLO;
2008-01-01
Abstract
Very High Energy Gamma Astronomy is one of the scientific aims of the ARGO-YBJ experiment (YangBaJing, P.R. China), an extensive air shower detector made of a single layer of Resistive Plate Chambers covering a surface of about 6700 m2. The exploitation of the full coverage approach (93% of active area) together with the very high altitude locationI documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
