A γhadron separation analysis is described for the observed air shower events with primary energy above 100 TeV based on the Tibet ASγ detector configuration. The shower age and size parameters are fitted from the m...A γhadron separation analysis is described for the observed air shower events with primary energy above 100 TeV based on the Tibet ASγ detector configuration. The shower age and size parameters are fitted from the measured lateral density distribution and used as discrimination variables. According to the MC simulation while taking into account the systematic uncertainty estimated from data and MC comparison, it is found that 70% of the cosmic ray （CR） background can be rejected while more than 78% of the T-rays can be retained. Sensitivity for 100 TeV γ-rays observation can thus be improved by at least 40%.展开更多
基金Supported by Chinese Academy of Sciences (KJCX2-YW-N13)External Cooperation Program of Chinese Academy of Sciences (GJHZ1004)+1 种基金National Natural Science Foundation of China (10725524, 10875132)supported by the Natural Science Foundation of Shandong Province, China (Q2006A02)
文摘A γhadron separation analysis is described for the observed air shower events with primary energy above 100 TeV based on the Tibet ASγ detector configuration. The shower age and size parameters are fitted from the measured lateral density distribution and used as discrimination variables. According to the MC simulation while taking into account the systematic uncertainty estimated from data and MC comparison, it is found that 70% of the cosmic ray （CR） background can be rejected while more than 78% of the T-rays can be retained. Sensitivity for 100 TeV γ-rays observation can thus be improved by at least 40%.
