Online charge calibration of LHAASO-WCDA---a study with the engineering array
Gao Bo, Chen Ming-Jun, Gu Ming-Hao, Hao Xin-Jun, Li Hui-Cai, Wu, Han-Rong, Yao Zhi-Guo, You Xiao-Hao, Zhou Bin (for the LHAASO collaboration)

TL;DR
This paper presents an online charge calibration method for the LHAASO-WCDA water Cherenkov detector array, demonstrating high-precision calibration techniques tested on a prototype array to support the full-scale project.
Contribution
The study introduces a novel online charge calibration approach for water Cherenkov detectors, validated with a prototype array, enhancing calibration accuracy for the LHAASO-WCDA project.
Findings
Achieved calibration precision within a few percentage points.
Validated calibration methods on a 9-cell prototype array.
Demonstrated feasibility for large-scale deployment.
Abstract
LHAASO-WCDA is a large ground-based water Cherenkov detector array planned to be built at Shangri-La, Yunnan Province, China. As a major component of LHAASO project, the main purpose of LHAASO-WCDA is to survey the northern sky for very-high-energy (above 100 GeV) gamma ray sources. To gain full knowledge of water Cherenkov technique and to well investigate engineering issues, a 9-cell detector array has been built at Yang-Ba-Jing site, neighboring to the ARGO-YBJ experiment. With the array, charge calibration methods for low and high ranges of the PMT readout are studied, whose result shows that a very high precision at several percentages can be reached. These calibration methods are proposed to be applied in the future LHAASO-WCDA project.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Radiation Detection and Scintillator Technologies
