Paper

Calibration Strategy of the JUNO-TAO Experiment

Yan, Wenqi, Hu, Jun, Zhao, Rong, Jolliet, Cécile, Perrot, Frédéric, Zhang, Shuihan, Liu, Caimei, Montini, Paolo, Steiger, Hans, Zamogilnyi, Kirill, Callier, Stéphane, Campeny, Agustin, Jiang, Tao, Li, Daozheng, Li, Ruhui, Rebii, Abdel, Xu, Hangkun, He, Miao, Li, Yichen, Wu, Diru, Liu, Mengchao, Yao, Haifeng, Walker, Pablo, Qian, Xiaohui, Hu, Jianrun, Jiang, Xiaoshan, Druillole, Frederic, Sun, Xilei, He, Yuanqiang, Wang, Zhimin, Selma Conforti Di Lorenzo, Zhan, Liang, Liu, Yunzhe, Zhang, Jie, Ma, Xiaoyan, Anfimov, Nikolay V, Juan Pedro Ochoa-Ricoux, Cerna, Cedric, Li, Min, Wang, Wei, Hou, Shaojing, Abusleme, Angel, Cao, Jun, Yatian Pei, Rybnikov, Arsenij, Ye, Mei, Mari, Stefano M, Gromov, Maxim, Xiao, Xiang, Zhengyong Fei, He, Wei, Petrucci, Fabrizio, Xie, Yuguang, Xie, Zhangquan, Huss, Cédric, Wang, Meifen, Yuan, Chengzhuo, Chen, Yu, Luo, Guang, Roskovec, Bedřich, Hor, Joseph yk, Lombardo, Claudio, Lu, Peizhi, Ding, Yayun, Chepurnov, Alexander, Wang, Derun, Yang, Huan, Fabbri, Andrea, Ji, Xiaolu, Cao, Guofu

2022

Overview

The Taishan Antineutrino Observatory (JUNO-TAO, or TAO) is a satellite detector for the Jiangmen Underground Neutrino Observatory (JUNO). Located near the Taishan reactor, TAO independently measures the reactor's antineutrino energy spectrum with unprecedented energy resolution. To achieve this goal, energy response must be well calibrated. Using the Automated Calibration Unit (ACU) and the Cable Loop System (CLS) of TAO, multiple radioactive sources are deployed to various positions in the detector to perform a precise calibration of energy response. The non-linear energy response can be controlled within 0.6% with different energy points of these radioactive sources. It can be further improved by using \\(^{12}\\rm B\\) decay signals produced by cosmic muons. Through the energy non-uniformity calibration, residual non-uniformity is less than 0.2%. The energy resolution degradation and energy bias caused by the residual non-uniformity can be controlled within 0.05% and 0.3%, respectively. In addition, the stability of other detector parameters, such as the gain of each silicon photo-multiplier, can be monitored with a special ultraviolet LED calibration system.

• Publisher: Cornell University Library, arXiv.org
• Subject: Calibration / Energy / Energy resolution / Energy spectra / Muons / Neutrinos / Nonlinear response / Nonuniformity / Observatories / Sensors