Abstract
The YangBaJing Hybrid Array (YBJ-HA) is located at the Yangbajing international cosmic ray observatory, Tibet, China. It consists of 115 scintillation detectors (SDs) and 16 underground water Cherenkov muon detectors (MDA). Its main physical goal is to observe the \(\gamma \)-ray sources in the 100 TeV energy region, so the array must have very good pointing accuracy. To achieve this performance, the time response of the scintillator detectors must have high consistency. This paper introduces a characteristic plane method (offline calibration method) to calibrate the time of each scintillator detector and uses the moon shadow analysis results to test the time calibration accuracy.
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Funding
This work was supported by the Central Government Funds for Local Scientific and Technological Development (Grant No. JDRC2023000009), the Reformation and Development Funds for the Local Region Universities from the Chinese Government in 2023(Grant Nos.00061082,00060858, and 00060867-01), and Tibet University Postgraduate Students’ High-Level Talent Training Plan Project (No.2021-GSP-S037).
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Shao-Zhang Zhao and You-Liang Feng contributed to data analysis. Qi Gao and Tian-Lu Chen contributed to data analysis and detector installation.
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Zhao, S., Chen, T., Gao, Q. et al. Study on the time calibration method of the YangBaJing Hybrid Array. Astrophys Space Sci 369, 36 (2024). https://doi.org/10.1007/s10509-024-04299-2
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DOI: https://doi.org/10.1007/s10509-024-04299-2