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 location
2008
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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/271216
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