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Performances and long-term stability of the LHAASO-KM2A prototype array

Performances and long-term stability of the LHAASO-KM2A prototype array
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摘要 A prototype array for the LHAASO-KM2A, which consists of 42 detector units and fully overlaps the ARGO-YBJ experiment, was set up at the Yangbajing cosmic ray observatory and has been in stable operation since Octoter 2010. The resulting performances of the KM2A electromagnetic particle detector prototypes fully meet the design requirements. Through hybrid observation of cosmic ray showers with the ARGO-YBJ experiment, the performances and long-term stability of the prototype array are tested and the results are consistent with expectation. The cosmic ray moon shadow observed by the prototype array is also presented. A prototype array for the LHAASO-KM2A, which consists of 42 detector units and fully overlaps the ARGO-YBJ experiment, was set up at the Yangbajing cosmic ray observatory and has been in stable operation since Octoter 2010. The resulting performances of the KM2A electromagnetic particle detector prototypes fully meet the design requirements. Through hybrid observation of cosmic ray showers with the ARGO-YBJ experiment, the performances and long-term stability of the prototype array are tested and the results are consistent with expectation. The cosmic ray moon shadow observed by the prototype array is also presented.
出处 《Chinese Physics C》 SCIE CAS CSCD 2014年第2期40-44,共5页 中国物理C(英文版)
基金 Supported by NSFC(11175147) Knowledge Innovation Fund of IHEP,Beijing
关键词 LHAASO-KM2A prototype array PERFORMANCE long-term stability LHAASO-KM2A prototype array performance long-term stability
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参考文献8

  • 1CAO Zhen. Chinese Physics C (HEP & NP), 2010, 34(2): 4, 249 252.
  • 2HE Hai-Hui et al. (LHAASO collaboration). ICRC2009, Poland SHENG Xiang-Dong et al. (LHAASO collaboration). ICRC2011, Chin.
  • 3XIAO Gang et al. (LHAASO collaboration). ICRC2011, China.
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  • 5GU Min-Hao et al. (LHAASO collaboration). ICRC2011, China.
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  • 7Bartoli B et al. The Astrophysical Journal, 2011, 734: 110 (Spp).
  • 8Bartoli Bet al. The Astrophysical Journal, 2011, 734: 110 (Spp).

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