Performance of LHAASO-WCDA and observation of the Crab Nebula as a standard candle

Performance of LHAASO-WCDA and observation of the Crab Nebula as a standard candle
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LHAASO-WCDA 的性能和蟹状星云作为标准烛光的观测

DOI:
10.1088/1674-1137/ac041b
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发表时间:
2021
期刊:
影响因子:
3.6
通讯作者:
Che
Che
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Aharonian F.;An Q.;Axikegu 克古;Bai L. X.;Bai Y. X.;Bao Y. W.;Bastieri D.;Bi X. J.;Bi Y. J.;Cai H.;Cai J. T.;Cao Z.;Cao Z.;Chang J.;Chang J. F.;Chang X. C.;Chen B. M.;Chen J.;Chen L.;Chen L.;Chen L.;Chen M. J.;Chen M. L.;Chen Q. H.;Chen S. H.;Chen S. Z.;Che

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LHAASO实验的第一个水切伦科夫探测器(WCDA-1)自2019年4月以来一直在运行。第一年的数据已经通过观察蟹状星云作为标准蜡烛进行了分析,以测试其性能。WCDA-1实现了每年65 mCU的灵敏度,统计阈值为5
The first Water Cherenkov detector of the LHAASO experiment (WCDA-1) has been operating since April 2019. The data for the first year have been analyzed to test its performance by observing the Crab Nebula as a standard candle. The WCDA-1 achieves a sensitivity of 65 mCU per year, with a statistical threshold of 5